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1,802.0766
Cosmological screening and the phantom braneworld model
The scalar and vector cosmological perturbations at all length scales of our Universe are studied in the framework of the phantom braneworld model. The model is characterized by the parameter $\Omega_M\equiv M^3/2m^2H_0$, with $M$ and $m$ the 5- and 4-dimensional Planck scales, respectively, and $H_0$ the Hubble parameter today, while $\Omega_M\rightarrow 0$ recovers the $\Lambda\rm CDM$ model. Ignoring the backreaction due to the peculiar velocities and also the bulk cosmological constant, allows the explicit computation of the gravitational potentials, $\Phi$ and $\Psi$. They exhibit exponentially decreasing screening behaviour characterized by a screening length which is a function of the quasidensity parameter $ \Omega_M$.
gr-qc astro-ph.CO
the scalar and vector cosmological perturbations at all length scales of our universe are studied in the framework of the phantom braneworld model the model is characterized by the parameter omega_mequiv m32m2h_0 with m and m the 5 and 4dimensional planck scales respectively and h_0 the hubble parameter today while omega_mrightarrow 0 recovers the lambdarm cdm model ignoring the backreaction due to the peculiar velocities and also the bulk cosmological constant allows the explicit computation of the gravitational potentials phi and psi they exhibit exponentially decreasing screening behaviour characterized by a screening length which is a function of the quasidensity parameter omega_m
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1,802.07661
The energy equality for the Navier-Stokes equations in bounded domains
In this paper, we provide a sufficient condition of the energy equality for the incompressible Navier-Stokes equations in bounded domains.
math.AP
in this paper we provide a sufficient condition of the energy equality for the incompressible navierstokes equations in bounded domains
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1,802.07662
Dynamics on abelian varieties in positive characteristic
We study periodic points for endomorphisms $\sigma$ of abelian varieties $A$ over algebraically closed fields of positive characteristic $p$. We show that the dynamical zeta function $\zeta_\sigma$ of $\sigma$ is either rational or transcendental, the first case happening precisely when $\sigma^n-1$ is a separable isogeny for all $n$. We call this condition very inseparability and show it is equivalent to the action of $\sigma$ on the local $p$-torsion group scheme being nilpotent. The "false" zeta function $D_\sigma$, in which the number of fixed points of $\sigma^n$ is replaced by the degree of $\sigma^n-1$, is always a rational function. Let $1/\Lambda$ denote its largest real pole and assume no other pole or zero has the same absolute value. Then, using a general dichotomy result for power series proven by Royals and Ward in the appendix, we find that $\zeta_\sigma(z)$ has a natural boundary at $|z|=1/\Lambda$ when $\sigma$ is not very inseparable. We introduce and study tame dynamics, ignoring orbits whose order is divisible by $p$. We construct a tame zeta function $\zeta^*_{\sigma}$ that is always algebraic, and such that $\zeta_\sigma$ factors into an infinite product of tame zeta functions. We briefly discuss functional equations. Finally, we study the length distribution of orbits and tame orbits. Orbits of very inseparable endomorphisms distribute like those of Axiom A systems with entropy $\log \Lambda$, but the orbit length distribution of not very inseparable endomorphisms is more erratic and similar to $S$-integer dynamical systems. We provide an expression for the prime orbit counting function in which the error term displays a power saving depending on the largest real part of a zero of $D_\sigma(\Lambda^{-s})$.
math.NT math.AG math.DS
we study periodic points for endomorphisms sigma of abelian varieties a over algebraically closed fields of positive characteristic p we show that the dynamical zeta function zeta_sigma of sigma is either rational or transcendental the first case happening precisely when sigman1 is a separable isogeny for all n we call this condition very inseparability and show it is equivalent to the action of sigma on the local ptorsion group scheme being nilpotent the false zeta function d_sigma in which the number of fixed points of sigman is replaced by the degree of sigman1 is always a rational function let 1lambda denote its largest real pole and assume no other pole or zero has the same absolute value then using a general dichotomy result for power series proven by royals and ward in the appendix we find that zeta_sigmaz has a natural boundary at z1lambda when sigma is not very inseparable we introduce and study tame dynamics ignoring orbits whose order is divisible by p we construct a tame zeta function zeta_sigma that is always algebraic and such that zeta_sigma factors into an infinite product of tame zeta functions we briefly discuss functional equations finally we study the length distribution of orbits and tame orbits orbits of very inseparable endomorphisms distribute like those of axiom a systems with entropy log lambda but the orbit length distribution of not very inseparable endomorphisms is more erratic and similar to sinteger dynamical systems we provide an expression for the prime orbit counting function in which the error term displays a power saving depending on the largest real part of a zero of d_sigmalambdas
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1,802.07663
Heisenberg-Pauli-Weyl and Donoho-Stark's uncertainty principle for the Weinstein $L^2$-multiplier operators
The aim of this paper is establish the Heisenberg-Pauli-Weyl uncertainty principle and Donho-Stark's uncertainty principle for the Weinstein $L^2$-multiplier operators.
math.CA math.AP
the aim of this paper is establish the heisenbergpauliweyl uncertainty principle and donhostarks uncertainty principle for the weinstein l2multiplier operators
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1,802.07664
Robustness of flow networks against cascading failures under partial load redistribution
We study the robustness of flow networks against cascading failures under a partial load redistribution model. In particular, we consider a flow network of $N$ lines with initial loads $L_1, \ldots, L_N$ and free-spaces (i.e., redundant space) $S_1, \ldots, S_N$ that are independent and identically distributed with joint distribution $P_{LS}(x,y)=\mathbb{P}(L \leq x, S \leq y)$. The capacity $C_i$ is the maximum load allowed on line $i$, and is given by $C_i=L_i + S_i$. When a line fails due to overloading, it is removed from the system and $(1-\varepsilon)$-fraction of the load it was carrying (at the moment of failing) gets redistributed equally among all remaining lines in the system; hence we refer to this as the {\it partial} load redistribution model. The rest (i.e., $\varepsilon$-fraction) of the load is assumed to be lost or absorbed, e.g., due to advanced circuitry disconnecting overloaded power lines or an inter-connected network/material absorbing a fraction of the flow from overloaded lines. We analyze the robustness of this flow network against random attacks that remove a $p$-fraction of the lines. Our contributions include (i) deriving the final fraction of alive lines $n_{\infty}(p,\varepsilon)$ for all $p, \varepsilon \in (0,1)$ and confirming the results via extensive simulations; (ii) showing that partial redistribution might lead to (depending on the parameter $0<\varepsilon \leq 1$) the order of transition at the critical attack size $p^{*}$ changing from first to second-order; and (iii) proving analytically that flow networks achieve maximum robustness (quantified by the area $\int_{0}^{1} n_{\infty}(p,\varepsilon) \mathrm{d}p$) when all lines have the same free-space regardless of their initial load. The optimality of equal free-space allocation is also confirmed on real-world data from the UK National Power Grid.
physics.soc-ph
we study the robustness of flow networks against cascading failures under a partial load redistribution model in particular we consider a flow network of n lines with initial loads l_1 ldots l_n and freespaces ie redundant space s_1 ldots s_n that are independent and identically distributed with joint distribution p_lsxymathbbpl leq x s leq y the capacity c_i is the maximum load allowed on line i and is given by c_il_i s_i when a line fails due to overloading it is removed from the system and 1varepsilonfraction of the load it was carrying at the moment of failing gets redistributed equally among all remaining lines in the system hence we refer to this as the it partial load redistribution model the rest ie varepsilonfraction of the load is assumed to be lost or absorbed eg due to advanced circuitry disconnecting overloaded power lines or an interconnected networkmaterial absorbing a fraction of the flow from overloaded lines we analyze the robustness of this flow network against random attacks that remove a pfraction of the lines our contributions include i deriving the final fraction of alive lines n_inftypvarepsilon for all p varepsilon in 01 and confirming the results via extensive simulations ii showing that partial redistribution might lead to depending on the parameter 0varepsilon leq 1 the order of transition at the critical attack size p changing from first to secondorder and iii proving analytically that flow networks achieve maximum robustness quantified by the area int_01 n_inftypvarepsilon mathrmdp when all lines have the same freespace regardless of their initial load the optimality of equal freespace allocation is also confirmed on realworld data from the uk national power grid
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1,802.07665
Distributed Hypothesis Testing Over Discrete Memoryless Channels
A distributed binary hypothesis testing (HT) problem involving two parties, one referred to as the observer and the other as the detector is studied. The observer observes a discrete memoryless source (DMS) and communicates its observations to the detector over a discrete memoryless channel (DMC). The detector observes another DMS correlated with that at the observer, and performs a binary HT on the joint distribution of the two DMS's using its own observed data and the information received from the observer. The trade-off between the type I error probability and the type II error-exponent of the HT is explored. Single-letter lower bounds on the optimal type II error-exponent are obtained by using two different coding schemes, a separate HT and channel coding scheme and a joint HT and channel coding scheme based on hybrid coding for the matched bandwidth case. Exact single-letter characterization of the same is established for the special case of testing against conditional independence, and it is shown to be achieved by the separate HT and channel coding scheme. An example is provided where the joint scheme achieves a strictly better performance than the separation based scheme.
cs.IT math.IT
a distributed binary hypothesis testing ht problem involving two parties one referred to as the observer and the other as the detector is studied the observer observes a discrete memoryless source dms and communicates its observations to the detector over a discrete memoryless channel dmc the detector observes another dms correlated with that at the observer and performs a binary ht on the joint distribution of the two dmss using its own observed data and the information received from the observer the tradeoff between the type i error probability and the type ii errorexponent of the ht is explored singleletter lower bounds on the optimal type ii errorexponent are obtained by using two different coding schemes a separate ht and channel coding scheme and a joint ht and channel coding scheme based on hybrid coding for the matched bandwidth case exact singleletter characterization of the same is established for the special case of testing against conditional independence and it is shown to be achieved by the separate ht and channel coding scheme an example is provided where the joint scheme achieves a strictly better performance than the separation based scheme
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1,802.07666
Classical large deviations theorems on complete Riemannian manifolds
We generalize classical large deviations theorems to the setting of complete Riemannian manifolds. We prove the analogue of Mogulskii's theorem for geodesic random walks via a general approach using visocity solutions for Hamilton-Jacobi equations. As a corollary, we also obtain the analogue of Cram\'er's theorem. The approach also provides a new proof of Schilder's theorem. Additionally, we provide a proof of Schilder's theorem by using an embedding into Euclidean space, together with Freidlin-Wentzell theory.
math.PR math-ph math.DG math.MP
we generalize classical large deviations theorems to the setting of complete riemannian manifolds we prove the analogue of mogulskiis theorem for geodesic random walks via a general approach using visocity solutions for hamiltonjacobi equations as a corollary we also obtain the analogue of cramers theorem the approach also provides a new proof of schilders theorem additionally we provide a proof of schilders theorem by using an embedding into euclidean space together with freidlinwentzell theory
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1,802.07667
On higher-dimensional Courant algebroids
We define the transgression functor which associates to a (higher-dimensional) Courant algebroid on a manifold a Lie algebroid on the shifted tangent bundle of the manifold.
math.QA math.DG math.SG
we define the transgression functor which associates to a higherdimensional courant algebroid on a manifold a lie algebroid on the shifted tangent bundle of the manifold
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1,802.07668
A model for system uncertainty in reinforcement learning
This work provides a rigorous framework for studying continuous time control problems in uncertain environments. The framework considered models uncertainty in state dynamics as a measure on the space of functions. This measure is considered to change over time as agents learn their environment. This model can be seem as a variant of either Bayesian reinforcement learning or adaptive control. We study necessary conditions for locally optimal trajectories within this model, in particular deriving an appropriate dynamic programming principle and Hamilton-Jacobi equations. This model provides one possible framework for studying the tradeoff between exploration and exploitation in reinforcement learning.
math.OC
this work provides a rigorous framework for studying continuous time control problems in uncertain environments the framework considered models uncertainty in state dynamics as a measure on the space of functions this measure is considered to change over time as agents learn their environment this model can be seem as a variant of either bayesian reinforcement learning or adaptive control we study necessary conditions for locally optimal trajectories within this model in particular deriving an appropriate dynamic programming principle and hamiltonjacobi equations this model provides one possible framework for studying the tradeoff between exploration and exploitation in reinforcement learning
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1,802.07669
On the convergence of partial sums with respect to Vilenkin system on the martingale Hardy spaces
In this paper we derive characterizations of boundedness of the subsequences of partial sums with respect to Vilenkin system on the martingale Hardy spaces when $ 0<p<1 $. Moreover, we find necessary and sufficient conditions for the modulus of continuity of $f\in H_{p}$ martingales, which provide convergence of subsequences of partial sums on the martingale Hardy spaces. It is also proved that these results are the best possible in a special sense. As applications, both some well-known and new results are pointed out.
math.CA
in this paper we derive characterizations of boundedness of the subsequences of partial sums with respect to vilenkin system on the martingale hardy spaces when 0p1 moreover we find necessary and sufficient conditions for the modulus of continuity of fin h_p martingales which provide convergence of subsequences of partial sums on the martingale hardy spaces it is also proved that these results are the best possible in a special sense as applications both some wellknown and new results are pointed out
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1,802.0767
Investigation of radio pulsar emission features using power spectra
Since 2013 round-the-clock monitoring of the sky is carried out simultaneously in 96 space beams using the high-sensitivity radio telescope of LPA (Large Phased Array) at the frequency 110.25 MHz. These observations are made under the program of the interplanetary plasma investigation. The same data is used for the search for pulsars by means of the power spectra. For the increase of the pulsar search sensitivity the summation to 500-600 of power spectra corresponding to the different days of the observations is made. In the integrated spectra of the known pulsars, besides expected improvement of a signal-to-noise ($S/N$) ratio for the frequency harmonics, were showed some features which are explored in the paper. We present 27 strongest pulsars which are in the field of declinations $21\degr - 42\degr$ at which the connection of observable details in the integrated power spectra with the presence of pulsar periods of the second ($P_2$) and third ($P_3$) class has been discovered. The empirical relations for the calculation of these periods are obtained. The value $P_2$ is estimated for 26 pulsars, and for 15 sources it is made for the first time. The value $P_3$ is estimated for 13 pulsars, from them for 5 sources they are given for the first time.
astro-ph.HE astro-ph.SR
since 2013 roundtheclock monitoring of the sky is carried out simultaneously in 96 space beams using the highsensitivity radio telescope of lpa large phased array at the frequency 11025 mhz these observations are made under the program of the interplanetary plasma investigation the same data is used for the search for pulsars by means of the power spectra for the increase of the pulsar search sensitivity the summation to 500600 of power spectra corresponding to the different days of the observations is made in the integrated spectra of the known pulsars besides expected improvement of a signaltonoise sn ratio for the frequency harmonics were showed some features which are explored in the paper we present 27 strongest pulsars which are in the field of declinations 21degr 42degr at which the connection of observable details in the integrated power spectra with the presence of pulsar periods of the second p_2 and third p_3 class has been discovered the empirical relations for the calculation of these periods are obtained the value p_2 is estimated for 26 pulsars and for 15 sources it is made for the first time the value p_3 is estimated for 13 pulsars from them for 5 sources they are given for the first time
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1,802.07671
Stokes waves with constant vorticity: I. numerical computation
Periodic traveling waves are numerically computed in a constant vorticity flow subject to the force of gravity. The Stokes wave problem is formulated via a conformal mapping as a nonlinear pseudo-differential equation, involving a periodic Hilbert transform for a strip, and solved by the Newton-GMRES method. It works well with a fast Fourier transform and is more effective than a boundary integral method. The result is in excellent agreement, qualitatively and quantitatively, with earlier ones. For strong positive vorticity, in the finite or infinite depth, overhanging profiles are found as the steepness increases and tend to a touching wave, whose profile self-intersects somewhere along the trough line, trapping an air bubble; the numerical solutions become unphysical as the steepness increases further and make a gap in the wave speed versus steepness plane; a touching wave then takes over and the physical solutions follow in the wave speed versus steepness plane until they ultimately tend to an extreme wave, which exhibits a sharp corner at the crest. Overhanging waves of nearly maximum heights are found to approach rigid body rotation of a fluid disk as the strength of positive vorticity increases.
physics.flu-dyn
periodic traveling waves are numerically computed in a constant vorticity flow subject to the force of gravity the stokes wave problem is formulated via a conformal mapping as a nonlinear pseudodifferential equation involving a periodic hilbert transform for a strip and solved by the newtongmres method it works well with a fast fourier transform and is more effective than a boundary integral method the result is in excellent agreement qualitatively and quantitatively with earlier ones for strong positive vorticity in the finite or infinite depth overhanging profiles are found as the steepness increases and tend to a touching wave whose profile selfintersects somewhere along the trough line trapping an air bubble the numerical solutions become unphysical as the steepness increases further and make a gap in the wave speed versus steepness plane a touching wave then takes over and the physical solutions follow in the wave speed versus steepness plane until they ultimately tend to an extreme wave which exhibits a sharp corner at the crest overhanging waves of nearly maximum heights are found to approach rigid body rotation of a fluid disk as the strength of positive vorticity increases
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1,802.07672
Learning Multiple Categories on Deep Convolution Networks
Deep convolution networks have proved very successful with big datasets such as the 1000-classes ImageNet. Results show that the error rate increases slowly as the size of the dataset increases. Experiments presented here may explain why these networks are very effective in solving big recognition problems. If the big task is made up of multiple smaller tasks, then the results show the ability of deep convolution networks to decompose the complex task into a number of smaller tasks and to learn them simultaneously. The results show that the performance of solving the big task on a single network is very close to the average performance of solving each of the smaller tasks on a separate network. Experiments also show the advantage of using task specific or category labels in combination with class labels.
cs.CV
deep convolution networks have proved very successful with big datasets such as the 1000classes imagenet results show that the error rate increases slowly as the size of the dataset increases experiments presented here may explain why these networks are very effective in solving big recognition problems if the big task is made up of multiple smaller tasks then the results show the ability of deep convolution networks to decompose the complex task into a number of smaller tasks and to learn them simultaneously the results show that the performance of solving the big task on a single network is very close to the average performance of solving each of the smaller tasks on a separate network experiments also show the advantage of using task specific or category labels in combination with class labels
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1,802.07673
Non-Malleable Codes for Small-Depth Circuits
We construct efficient, unconditional non-malleable codes that are secure against tampering functions computed by small-depth circuits. For constant-depth circuits of polynomial size (i.e. $\mathsf{AC^0}$ tampering functions), our codes have codeword length $n = k^{1+o(1)}$ for a $k$-bit message. This is an exponential improvement of the previous best construction due to Chattopadhyay and Li (STOC 2017), which had codeword length $2^{O(\sqrt{k})}$. Our construction remains efficient for circuit depths as large as $\Theta(\log(n)/\log\log(n))$ (indeed, our codeword length remains $n\leq k^{1+\epsilon})$, and extending our result beyond this would require separating $\mathsf{P}$ from $\mathsf{NC^1}$. We obtain our codes via a new efficient non-malleable reduction from small-depth tampering to split-state tampering. A novel aspect of our work is the incorporation of techniques from unconditional derandomization into the framework of non-malleable reductions. In particular, a key ingredient in our analysis is a recent pseudorandom switching lemma of Trevisan and Xue (CCC 2013), a derandomization of the influential switching lemma from circuit complexity; the randomness-efficiency of this switching lemma translates into the rate-efficiency of our codes via our non-malleable reduction.
cs.CC cs.CR cs.IT math.IT
we construct efficient unconditional nonmalleable codes that are secure against tampering functions computed by smalldepth circuits for constantdepth circuits of polynomial size ie mathsfac0 tampering functions our codes have codeword length n k1o1 for a kbit message this is an exponential improvement of the previous best construction due to chattopadhyay and li stoc 2017 which had codeword length 2osqrtk our construction remains efficient for circuit depths as large as thetalognloglogn indeed our codeword length remains nleq k1epsilon and extending our result beyond this would require separating mathsfp from mathsfnc1 we obtain our codes via a new efficient nonmalleable reduction from smalldepth tampering to splitstate tampering a novel aspect of our work is the incorporation of techniques from unconditional derandomization into the framework of nonmalleable reductions in particular a key ingredient in our analysis is a recent pseudorandom switching lemma of trevisan and xue ccc 2013 a derandomization of the influential switching lemma from circuit complexity the randomnessefficiency of this switching lemma translates into the rateefficiency of our codes via our nonmalleable reduction
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1,802.07674
Odd-time reversal $PT$ symmetry induced by anti-$PT$-symmetric medium
We introduce an optical system (a coupler) obeying parity-time ($PT$) symmetry with odd-time reversal, $T^2=-1$. It is implemented with two birefringent waveguides embedded in an anti-$PT$-symmetric medium. The system possesses properties which are untypical for most physical systems with the conventional even-time reversal. Having symmetry-protected degeneracy of the linear modes, the coupler allows for realization of a coherent switch operating with a superposition of binary states which are distinguished by their polarizations. When a Kerr nonlinearity is taken into account, each linear state, being double degenerated, bifurcates into several distinct nonlinear modes, some of which are dynamically stable. The nonlinear modes are characterized by amplitude and by polarization and come in $PT$-conjugate pairs.
physics.optics nlin.PS
we introduce an optical system a coupler obeying paritytime pt symmetry with oddtime reversal t21 it is implemented with two birefringent waveguides embedded in an antiptsymmetric medium the system possesses properties which are untypical for most physical systems with the conventional eventime reversal having symmetryprotected degeneracy of the linear modes the coupler allows for realization of a coherent switch operating with a superposition of binary states which are distinguished by their polarizations when a kerr nonlinearity is taken into account each linear state being double degenerated bifurcates into several distinct nonlinear modes some of which are dynamically stable the nonlinear modes are characterized by amplitude and by polarization and come in ptconjugate pairs
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1,802.07675
Exact Correlators from Conformal Ward Identities in Momentum Space and the Perturbative $TJJ$ Vertex
We present a general study of 3-point functions of conformal field theory in momentum space, following a reconstruction method for tensor correlators, based on the solution of the conformal Ward identities (CWI' s), introduced in recent works by Bzowski, McFadden and Skenderis (BMS). We investigate and detail the structure of the CWI's, their non-perturbative solutions and the transition to momentum space, comparing them to perturbation theory by taking QED as an example. We then proceed with an analysis of the $TJJ$ correlator, presenting independent and detailed re-derivations of the conformal equations in the reconstruction method of BMS, originally formulated using a minimal tensor basis in the transverse traceless sector. A careful comparison with a second basis introduced in previous studies shows that this correlator is affected by one anomaly pole in the graviton (T) line, induced by renormalization. The result shows that the origin of the anomaly, in this correlator, should be necessarily attributed to the exchange of a massless effective degree of freedom. Our results are then exemplified in massless QED at one-loop in $d$-dimensions, expressed in terms of perturbative master integrals. An independent analysis of the Fuchsian character of the solutions, which bypasses the 3K integrals, is also presented. We show that the combination of field theories at one-loop - with a specific field content of degenerate massless scalar and fermions - is sufficient to generate the complete non-perturbative solution, in agreement with a previous study in coordinate space. The result shows that free conformal field theories, in specific dimensions, arrested at one-loop, reproduce the general result for the $TJJ$. Analytical checks of this correspondence are presented in $d=3,4$ and $5$ spacetime dimensions[..].
hep-th hep-ph
we present a general study of 3point functions of conformal field theory in momentum space following a reconstruction method for tensor correlators based on the solution of the conformal ward identities cwi s introduced in recent works by bzowski mcfadden and skenderis bms we investigate and detail the structure of the cwis their nonperturbative solutions and the transition to momentum space comparing them to perturbation theory by taking qed as an example we then proceed with an analysis of the tjj correlator presenting independent and detailed rederivations of the conformal equations in the reconstruction method of bms originally formulated using a minimal tensor basis in the transverse traceless sector a careful comparison with a second basis introduced in previous studies shows that this correlator is affected by one anomaly pole in the graviton t line induced by renormalization the result shows that the origin of the anomaly in this correlator should be necessarily attributed to the exchange of a massless effective degree of freedom our results are then exemplified in massless qed at oneloop in ddimensions expressed in terms of perturbative master integrals an independent analysis of the fuchsian character of the solutions which bypasses the 3k integrals is also presented we show that the combination of field theories at oneloop with a specific field content of degenerate massless scalar and fermions is sufficient to generate the complete nonperturbative solution in agreement with a previous study in coordinate space the result shows that free conformal field theories in specific dimensions arrested at oneloop reproduce the general result for the tjj analytical checks of this correspondence are presented in d34 and 5 spacetime dimensions
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1,802.07676
Nonlinear stability of source defects in oscillatory media
In this paper, we prove the nonlinear stability under localized perturbations of spectrally stable time-periodic source defects of reaction-diffusion systems. Consisting of a core that emits periodic wave trains to each side, source defects are important as organizing centers of more complicated flows. Our analysis uses spatial dynamics combined with an instantaneous phase-tracking technique to obtain detailed pointwise estimates describing perturbations to lowest order as a phase-shift radiating outward at a linear rate plus a pair of localized approximately Gaussian excitations along the phase-shift boundaries; we show that in the wake of these outgoing waves the perturbed solution converges time-exponentially to a space-time translate of the original source pattern.
math.AP math.DS
in this paper we prove the nonlinear stability under localized perturbations of spectrally stable timeperiodic source defects of reactiondiffusion systems consisting of a core that emits periodic wave trains to each side source defects are important as organizing centers of more complicated flows our analysis uses spatial dynamics combined with an instantaneous phasetracking technique to obtain detailed pointwise estimates describing perturbations to lowest order as a phaseshift radiating outward at a linear rate plus a pair of localized approximately gaussian excitations along the phaseshift boundaries we show that in the wake of these outgoing waves the perturbed solution converges timeexponentially to a spacetime translate of the original source pattern
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1,802.07677
Can Microsoft Academic assess the early citation impact of in-press articles? A multi-discipline exploratory analysis
Many journals post accepted articles online before they are formally published in an issue. Early citation impact evidence for these articles could be helpful for timely research evaluation and to identify potentially important articles that quickly attract many citations. This article investigates whether Microsoft Academic can help with this task. For over 65,000 Scopus in-press articles from 2016 and 2017 across 26 fields, Microsoft Academic found 2-5 times as many citations as Scopus, depending on year and field. From manual checks of 1,122 Microsoft Academic citations not found in Scopus, Microsoft Academic's citation indexing was faster but not much wider than Scopus for journals. It achieved this by associating citations to preprints with their subsequent in-press versions and by extracting citations from in-press articles. In some fields its coverage of scholarly digital libraries, such as arXiv.org, was also an advantage. Thus, Microsoft Academic seems to be a more comprehensive automatic source of citation counts for in-press articles than Scopus.
cs.DL
many journals post accepted articles online before they are formally published in an issue early citation impact evidence for these articles could be helpful for timely research evaluation and to identify potentially important articles that quickly attract many citations this article investigates whether microsoft academic can help with this task for over 65000 scopus inpress articles from 2016 and 2017 across 26 fields microsoft academic found 25 times as many citations as scopus depending on year and field from manual checks of 1122 microsoft academic citations not found in scopus microsoft academics citation indexing was faster but not much wider than scopus for journals it achieved this by associating citations to preprints with their subsequent inpress versions and by extracting citations from inpress articles in some fields its coverage of scholarly digital libraries such as arxivorg was also an advantage thus microsoft academic seems to be a more comprehensive automatic source of citation counts for inpress articles than scopus
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1,802.07678
On a Modified Klein-Gordon Equation with Vacuum-Energy Contributions
We define a modified covariant Klein-Gordon (KG) equation containing quantum vacuum contributions arising from the self-interaction of matter with its own internal kinetic energy. The modified KG equation is exemplified for a variety of vacuum fields and various properties of the equation are articulated thereof. Generalized commutation and Energy-Momentum relations are characterized for a null vacuum-phase scenario of the proposed vacuum field $\lambda$. Within this limited scenario, a representation theorem is introduced suggesting that one can equally modify the spacetime structure or momentum operator in articulating the proposed quantum theory. Such a modified KG equation is further shown to eliminate infrared and the ultraviolet divergences in the generalized Klein-Gordon propagator.
gr-qc
we define a modified covariant kleingordon kg equation containing quantum vacuum contributions arising from the selfinteraction of matter with its own internal kinetic energy the modified kg equation is exemplified for a variety of vacuum fields and various properties of the equation are articulated thereof generalized commutation and energymomentum relations are characterized for a null vacuumphase scenario of the proposed vacuum field lambda within this limited scenario a representation theorem is introduced suggesting that one can equally modify the spacetime structure or momentum operator in articulating the proposed quantum theory such a modified kg equation is further shown to eliminate infrared and the ultraviolet divergences in the generalized kleingordon propagator
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1,802.07679
The STELLA Apparatus for Particle-Gamma Coincidence Fusion Measurements with Nanosecond Timing
The STELLA (STELlar LAboratory) experimental station for the measurement of deep sub-barrier light heavy-ion fusion cross sections has been installed at the Androm\`{e}de accelerator at the Institut de Physique Nucl\'{e}aire, Orsay (France). The setup is designed for the direct experimental determination of heavy-ion fusion cross sections as low as tens of picobarn. The detection concept is based on the coincident measurement of emitted gamma rays with the UK FATIMA (FAst TIMing Array) and evaporated charged particles using a silicon detector array. Key developments relevant to reaching the extreme sub-barrier fusion region are a rotating target mechanism to sustain beam intensities above 10$\mu$A, an ultra-high vacuum to prevent carbon built-up and gamma charged-particle timing in the order of nanoseconds sufficient to separate proton and alpha particles.
physics.ins-det
the stella stellar laboratory experimental station for the measurement of deep subbarrier light heavyion fusion cross sections has been installed at the andromede accelerator at the institut de physique nucleaire orsay france the setup is designed for the direct experimental determination of heavyion fusion cross sections as low as tens of picobarn the detection concept is based on the coincident measurement of emitted gamma rays with the uk fatima fast timing array and evaporated charged particles using a silicon detector array key developments relevant to reaching the extreme subbarrier fusion region are a rotating target mechanism to sustain beam intensities above 10mua an ultrahigh vacuum to prevent carbon builtup and gamma chargedparticle timing in the order of nanoseconds sufficient to separate proton and alpha particles
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1,802.0768
Gravitational lensing by wormholes supported by electromagnetic, scalar, and quantum effects
Wormholes are one of the most interesting topological features in spacetime, offering a rat run between two vastly separated regions of the universe. In this paper, we study the deflection angle of light by wormholes, which are supported by electric charge, magnetic charge, and scalar fields in the weak field limit approximation. To this end, we apply new geometric methods -- the Gauss-Bonnet theorem and the optical geometry -- to compute the deflection angles. We also verify our findings by using the well-known geodesics method. There exists a similarity between the charge and the quantum corrections on a black hole solution, which has been recently discussed in the context of the relativistic Bohmian quantum mechanics. By replacing classical geodesics with Bohmian trajectories, we introduce a new wormhole solution, whose having matter sources and anisotropic pressure supported by Bohmian quantum effects. The problem of fulfillment of the energy conditions of the Morris-Thorne traversable wormhole is also discussed.
gr-qc
wormholes are one of the most interesting topological features in spacetime offering a rat run between two vastly separated regions of the universe in this paper we study the deflection angle of light by wormholes which are supported by electric charge magnetic charge and scalar fields in the weak field limit approximation to this end we apply new geometric methods the gaussbonnet theorem and the optical geometry to compute the deflection angles we also verify our findings by using the wellknown geodesics method there exists a similarity between the charge and the quantum corrections on a black hole solution which has been recently discussed in the context of the relativistic bohmian quantum mechanics by replacing classical geodesics with bohmian trajectories we introduce a new wormhole solution whose having matter sources and anisotropic pressure supported by bohmian quantum effects the problem of fulfillment of the energy conditions of the morristhorne traversable wormhole is also discussed
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1,802.07681
Quantum heat engine based on level degeneracy
We study a quantum Stirling cycle which extracts work using quantized energy levels of a potential well. The work and the efficiency of the engine depend on the length of the potential well, and the Carnot efficiency is approached in a low temperature limiting case. We show that the lack of information about the position of the particle inside the potential well can be converted into useful work without resorting to any measurement. In the low temperature limit, we calculate the amount of work extractable from distinguishable particles, fermions, and bosons.
quant-ph cond-mat.stat-mech
we study a quantum stirling cycle which extracts work using quantized energy levels of a potential well the work and the efficiency of the engine depend on the length of the potential well and the carnot efficiency is approached in a low temperature limiting case we show that the lack of information about the position of the particle inside the potential well can be converted into useful work without resorting to any measurement in the low temperature limit we calculate the amount of work extractable from distinguishable particles fermions and bosons
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1,802.07682
Stability and error analysis of an implicit Milstein finite difference scheme for a two-dimensional Zakai SPDE
In this article, we propose an implicit finite difference scheme for a two-dimensional parabolic stochastic partial differential equation (SPDE) of Zakai type. The scheme is based on a Milstein approximation to the stochastic integral and an alternating direction implicit (ADI) discretisation of the elliptic term. We prove its mean-square stability and convergence in L2 of first order in time and second order in space, by Fourier analysis, in the presence of Dirac initial data. Numerical tests confirm these findings empirically.
math.NA
in this article we propose an implicit finite difference scheme for a twodimensional parabolic stochastic partial differential equation spde of zakai type the scheme is based on a milstein approximation to the stochastic integral and an alternating direction implicit adi discretisation of the elliptic term we prove its meansquare stability and convergence in l2 of first order in time and second order in space by fourier analysis in the presence of dirac initial data numerical tests confirm these findings empirically
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1,802.07683
Data Deluge in Astrophysics: Photometric Redshifts as a Template Use Case
Astronomy has entered the big data era and Machine Learning based methods have found widespread use in a large variety of astronomical applications. This is demonstrated by the recent huge increase in the number of publications making use of this new approach. The usage of machine learning methods, however is still far from trivial and many problems still need to be solved. Using the evaluation of photometric redshifts as a case study, we outline the main problems and some ongoing efforts to solve them.
astro-ph.IM
astronomy has entered the big data era and machine learning based methods have found widespread use in a large variety of astronomical applications this is demonstrated by the recent huge increase in the number of publications making use of this new approach the usage of machine learning methods however is still far from trivial and many problems still need to be solved using the evaluation of photometric redshifts as a case study we outline the main problems and some ongoing efforts to solve them
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1,802.07684
Multiscale finite elements through advection-induced coordinates for transient advection-diffusion equations
Long simulation times in climate sciences typically require coarse grids due to computational constraints. Nonetheless, unresolved subscale information significantly influences the prognostic variables and can not be neglected for reliable long term simulations. This is typically done via parametrizations but their coupling to the coarse grid variables often involves simple heuristics. We explore a novel up-scaling approach inspired by multi-scale finite element methods. These methods are well established in porous media applications, where mostly stationary or quasi stationary situations prevail. In advection-dominated problems arising in climate simulations the approach needs to be adjusted. We do so by performing coordinate transforms that make the effect of transport milder in the vicinity of coarse element boundaries. The idea of our method is quite general and we demonstrate it as a proof-of-concept on a one-dimensional passive advection-diffusion equation with oscillatory background velocity and diffusion.
math.NA cs.DS physics.comp-ph
long simulation times in climate sciences typically require coarse grids due to computational constraints nonetheless unresolved subscale information significantly influences the prognostic variables and can not be neglected for reliable long term simulations this is typically done via parametrizations but their coupling to the coarse grid variables often involves simple heuristics we explore a novel upscaling approach inspired by multiscale finite element methods these methods are well established in porous media applications where mostly stationary or quasi stationary situations prevail in advectiondominated problems arising in climate simulations the approach needs to be adjusted we do so by performing coordinate transforms that make the effect of transport milder in the vicinity of coarse element boundaries the idea of our method is quite general and we demonstrate it as a proofofconcept on a onedimensional passive advectiondiffusion equation with oscillatory background velocity and diffusion
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1,802.07685
Non-equilibrium Solute Capture in Passivating Oxide Films
If all humans vanished tomorrow, almost every metal structure would collapse within a century or less, the metal converting to an oxide. In applications ranging from the mature technology of nuts and bolts to high technology batteries, nuclear fuels and turbine engines, protective oxide films are critical to limiting oxidation. To date models of these oxide films have assumed that they form thermodynamic equilibrium stable or metastable phases doped within thermodynamic solubility limits. Here we demonstrate experimentally and theoretically the formation of unusual non-equilibrium oxide phases, that can be predicted using a scientific framework for solute capture at a moving oxide/substrate interface. The theory shows that solute capture is likely a generic process for many electrochemical processes, and suggests that similar phenomena yielding non-equilibrium phases can occur and be predicted for a wide range of other processes involving solid-fluid and solid-solid chemical reactions.
cond-mat.mtrl-sci
if all humans vanished tomorrow almost every metal structure would collapse within a century or less the metal converting to an oxide in applications ranging from the mature technology of nuts and bolts to high technology batteries nuclear fuels and turbine engines protective oxide films are critical to limiting oxidation to date models of these oxide films have assumed that they form thermodynamic equilibrium stable or metastable phases doped within thermodynamic solubility limits here we demonstrate experimentally and theoretically the formation of unusual nonequilibrium oxide phases that can be predicted using a scientific framework for solute capture at a moving oxidesubstrate interface the theory shows that solute capture is likely a generic process for many electrochemical processes and suggests that similar phenomena yielding nonequilibrium phases can occur and be predicted for a wide range of other processes involving solidfluid and solidsolid chemical reactions
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1,802.07686
Double scaling in the relaxation time in the $\beta$-FPUT model
We consider the original $\beta$-Fermi-Pasta-Ulam-Tsingou ($\beta$-FPUT) system; numerical simulations and theoretical arguments suggest that, for a finite number of masses, a statistical equilibrium state is reached independently of the initial energy of the system. Using ensemble averages over initial conditions characterized by different Fourier random phases, we numerically estimate the time scale of equipartition and we find that for very small nonlinearity it matches the prediction based on exact wave-wave resonant interactions theory. We derive a simple formula for the nonlinear frequency broadening and show that when the phenomenon of overlap of frequencies takes place, a different scaling for the thermalization time scale is observed. Our result supports the idea that Chirikov overlap criterium { identifies} a transition region between two different relaxation time scaling.
nlin.CD
we consider the original betafermipastaulamtsingou betafput system numerical simulations and theoretical arguments suggest that for a finite number of masses a statistical equilibrium state is reached independently of the initial energy of the system using ensemble averages over initial conditions characterized by different fourier random phases we numerically estimate the time scale of equipartition and we find that for very small nonlinearity it matches the prediction based on exact wavewave resonant interactions theory we derive a simple formula for the nonlinear frequency broadening and show that when the phenomenon of overlap of frequencies takes place a different scaling for the thermalization time scale is observed our result supports the idea that chirikov overlap criterium identifies a transition region between two different relaxation time scaling
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1,802.07687
Stochastic Video Generation with a Learned Prior
Generating video frames that accurately predict future world states is challenging. Existing approaches either fail to capture the full distribution of outcomes, or yield blurry generations, or both. In this paper we introduce an unsupervised video generation model that learns a prior model of uncertainty in a given environment. Video frames are generated by drawing samples from this prior and combining them with a deterministic estimate of the future frame. The approach is simple and easily trained end-to-end on a variety of datasets. Sample generations are both varied and sharp, even many frames into the future, and compare favorably to those from existing approaches.
cs.CV cs.AI cs.LG stat.ML
generating video frames that accurately predict future world states is challenging existing approaches either fail to capture the full distribution of outcomes or yield blurry generations or both in this paper we introduce an unsupervised video generation model that learns a prior model of uncertainty in a given environment video frames are generated by drawing samples from this prior and combining them with a deterministic estimate of the future frame the approach is simple and easily trained endtoend on a variety of datasets sample generations are both varied and sharp even many frames into the future and compare favorably to those from existing approaches
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1,802.07688
Generalized Wandzura Wilczek Relations and Orbital Angular Momentum
New Lorentz Invariance Relations (LIRs) were presented between twist-three Generalized Parton Distributions (GPDs) and transverse momentum, $k_T$, moments of twist-two Generalized Transverse Momentum-Dependent Distributions (GTMDs). By implementing both these LIRs and the QCD Equations of Motion in the quark quark correlation function, we generated a new series of Wandzura Wilczek (WW) relations in the off-forward sector. Two of these WW relations take on a particularly interesting physical meaning in that they provide a clear interpretation of the QCD structure of Orbital Angular Momentum (OAM) in the nucleon. In particular, they provide a solution to the outstanding puzzle of how OAM could be simultaneously described by twist-two GTMDs and twist-three GPDs. Additional relations were discussed, in particular, for the helicity configurations that can be detected analyzing specific spin asymmetries: one corresponding to a longitudinally polarized quark in an unpolarized proton, associated with spin-orbit correlations, and one for transverse proton polarization, as a generalization of the relation obeyed by the $g_2$ structure function; finally, we defined a relation connecting the off-forward extension of the Sivers function to an off-forward Qiu-Sterman term.
hep-ph
new lorentz invariance relations lirs were presented between twistthree generalized parton distributions gpds and transverse momentum k_t moments of twisttwo generalized transverse momentumdependent distributions gtmds by implementing both these lirs and the qcd equations of motion in the quark quark correlation function we generated a new series of wandzura wilczek ww relations in the offforward sector two of these ww relations take on a particularly interesting physical meaning in that they provide a clear interpretation of the qcd structure of orbital angular momentum oam in the nucleon in particular they provide a solution to the outstanding puzzle of how oam could be simultaneously described by twisttwo gtmds and twistthree gpds additional relations were discussed in particular for the helicity configurations that can be detected analyzing specific spin asymmetries one corresponding to a longitudinally polarized quark in an unpolarized proton associated with spinorbit correlations and one for transverse proton polarization as a generalization of the relation obeyed by the g_2 structure function finally we defined a relation connecting the offforward extension of the sivers function to an offforward qiusterman term
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1,802.07689
Exact spirally symmetric galactic dynamos
This paper extends the results of an earlier paper on scale invariant galactic spiral magnetic modes to time dependent, scale invariant, spirals. The examples given are all exact in that they may be described in terms of hypergeometric functions. We restrict the discussion to an infinitely conducting medium in order to avoid earlier approximation, which limited the solutions to cones lying within about twenty degrees to the plane. The magnetic disc spirals, `X type" poloidal fields, and the recent discovery of rotation measure screens in edge-on galactic halos were all recovered in such solutions.
astro-ph.GA
this paper extends the results of an earlier paper on scale invariant galactic spiral magnetic modes to time dependent scale invariant spirals the examples given are all exact in that they may be described in terms of hypergeometric functions we restrict the discussion to an infinitely conducting medium in order to avoid earlier approximation which limited the solutions to cones lying within about twenty degrees to the plane the magnetic disc spirals x type poloidal fields and the recent discovery of rotation measure screens in edgeon galactic halos were all recovered in such solutions
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1,802.0769
Strong thermal $SO(10)$-inspired leptogenesis in the light of recent results from long-baseline neutrino experiments
We confront recent experimental results on neutrino mixing parameters with the requirements from strong thermal $SO(10)$-inspired leptogenesis, where the asymmetry is produced from next-to-lightest right-handed neutrinos $N_2$ independently of the initial conditions. There is a nice agreement with latest global analyses supporting $\sin\delta < 0$ and normal ordering at $ \sim 95\%$ C.L. On the other hand, the more stringent experimental lower bound on the atmospheric mixing angle starts to corner strong thermal $SO(10)$-inspired leptogenesis. Prompted and encouraged by this rapid experimental advance, we obtain a precise determination of the allowed region in the plane $\delta$ versus $\theta_{23}$. We confirm that for the benchmark case $\alpha_2 \equiv m_{D2} / m_{\rm charm}= 5 \, $, where $m_{D2}$ is the intermediate neutrino Dirac mass setting the $N_2$ mass, and initial pre-existing asymmetry $N_{B-L}^{\rm p, i} = 10^{-3}$, the bulk of solutions lies in the first octant. Though most of the solutions are found outside the $95\%$ C.L. experimental region, there is still a big allowed fraction that does not require a too fine-tuned choice of the Majorana phases so that the neutrinoless double beta decay effective neutrino mass allowed range is still $m_{ee}\simeq [10,30]\,{\rm meV}$. We also show how the constraints depend on $N_{B-L}^{\rm p, i}$ and $\alpha_2$. In particular, we show that the current best fit, ($\theta_{23},\delta)\simeq (47^{\circ}, -130^{\circ})$, can be reproduced for $N_{B-L}^{\rm p, i} = 10^{-3}$ and $\alpha_2 = 6$. Such large values for $\alpha_2$ have been recently obtained in a few realistic fits within $SO(10)$-inspired models. Finally, we also obtain that current neutrino data rule out $N_{B-L}^{\rm p, i} \gtrsim 0.1$ for $\alpha_2 \lesssim 4.7$.
hep-ph
we confront recent experimental results on neutrino mixing parameters with the requirements from strong thermal so10inspired leptogenesis where the asymmetry is produced from nexttolightest righthanded neutrinos n_2 independently of the initial conditions there is a nice agreement with latest global analyses supporting sindelta 0 and normal ordering at sim 95 cl on the other hand the more stringent experimental lower bound on the atmospheric mixing angle starts to corner strong thermal so10inspired leptogenesis prompted and encouraged by this rapid experimental advance we obtain a precise determination of the allowed region in the plane delta versus theta_23 we confirm that for the benchmark case alpha_2 equiv m_d2 m_rm charm 5 where m_d2 is the intermediate neutrino dirac mass setting the n_2 mass and initial preexisting asymmetry n_blrm p i 103 the bulk of solutions lies in the first octant though most of the solutions are found outside the 95 cl experimental region there is still a big allowed fraction that does not require a too finetuned choice of the majorana phases so that the neutrinoless double beta decay effective neutrino mass allowed range is still m_eesimeq 1030rm mev we also show how the constraints depend on n_blrm p i and alpha_2 in particular we show that the current best fit theta_23deltasimeq 47circ 130circ can be reproduced for n_blrm p i 103 and alpha_2 6 such large values for alpha_2 have been recently obtained in a few realistic fits within so10inspired models finally we also obtain that current neutrino data rule out n_blrm p i gtrsim 01 for alpha_2 lesssim 47
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1,802.07691
Global synchronization of partially forced Kuramoto oscillators on Networks
We study the synchronization of Kuramoto oscillators on networks where only a fraction of them is subjected to a periodic external force. When all oscillators receive the external drive the system always synchronize with the periodic force if its intensity is sufficiently large. Our goal is to understand the conditions for global synchronization as a function of the fraction of nodes being forced and how these conditions depend on network topology, strength of internal couplings and intensity of external forcing. Numerical simulations show that the force required to synchronize the network with the external drive increases as the inverse of the fraction of forced nodes. However, for a given coupling strength, synchronization does not occur below a critical fraction, no matter how large is the force. Network topology and properties of the forced nodes also affect the critical force for synchronization. We develop analytical calculations for the critical force for synchronization as a function of the fraction of forced oscillators and for the critical fraction as a function of coupling strength. We also describe the transition from synchronization with the external drive to spontaneous synchronization.
nlin.AO
we study the synchronization of kuramoto oscillators on networks where only a fraction of them is subjected to a periodic external force when all oscillators receive the external drive the system always synchronize with the periodic force if its intensity is sufficiently large our goal is to understand the conditions for global synchronization as a function of the fraction of nodes being forced and how these conditions depend on network topology strength of internal couplings and intensity of external forcing numerical simulations show that the force required to synchronize the network with the external drive increases as the inverse of the fraction of forced nodes however for a given coupling strength synchronization does not occur below a critical fraction no matter how large is the force network topology and properties of the forced nodes also affect the critical force for synchronization we develop analytical calculations for the critical force for synchronization as a function of the fraction of forced oscillators and for the critical fraction as a function of coupling strength we also describe the transition from synchronization with the external drive to spontaneous synchronization
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1,802.07692
Centralized Volatility Reduction for Electricity Markets
Increased penetration of wind energy will make electricity market prices more volatile. As a result, market participants will bear increased financial risks, which impact investment decisions and in turn, makes it harder to achieve sustainable energy goals. As a remedy, in this paper, we propose an insurance market that complements any wholesale market design. Our mechanism can be run by any suitable financial entity such as an independent system operator, with the aim of reducing the financial impacts of volatile prices. We provide theoretical guarantees, analytically characterize the outcomes over a copperplate power system example, and numerically explore the same for a modified IEEE 14-bus test system.
math.OC
increased penetration of wind energy will make electricity market prices more volatile as a result market participants will bear increased financial risks which impact investment decisions and in turn makes it harder to achieve sustainable energy goals as a remedy in this paper we propose an insurance market that complements any wholesale market design our mechanism can be run by any suitable financial entity such as an independent system operator with the aim of reducing the financial impacts of volatile prices we provide theoretical guarantees analytically characterize the outcomes over a copperplate power system example and numerically explore the same for a modified ieee 14bus test system
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1,802.07693
RStore: A Distributed Multi-version Document Store
We address the problem of compactly storing a large number of versions (snapshots) of a collection of keyed documents or records in a distributed environment, while efficiently answering a variety of retrieval queries over those, including retrieving full or partial versions, and evolution histories for specific keys. We motivate the increasing need for such a system in a variety of application domains, carefully explore the design space for building such a system and the various storage-computation-retrieval trade-offs, and discuss how different storage layouts influence those trade-offs. We propose a novel system architecture that satisfies the key desiderata for such a system, and offers simple tuning knobs that allow adapting to a specific data and query workload. Our system is intended to act as a layer on top of a distributed key-value store that houses the raw data as well as any indexes. We design novel off-line storage layout algorithms for efficiently partitioning the data to minimize the storage costs while keeping the retrieval costs low. We also present an online algorithm to handle new versions being added to system. Using extensive experiments on large datasets, we demonstrate that our system operates at the scale required in most practical scenarios and often outperforms standard baselines, including a delta-based storage engine, by orders-of-magnitude.
cs.DB
we address the problem of compactly storing a large number of versions snapshots of a collection of keyed documents or records in a distributed environment while efficiently answering a variety of retrieval queries over those including retrieving full or partial versions and evolution histories for specific keys we motivate the increasing need for such a system in a variety of application domains carefully explore the design space for building such a system and the various storagecomputationretrieval tradeoffs and discuss how different storage layouts influence those tradeoffs we propose a novel system architecture that satisfies the key desiderata for such a system and offers simple tuning knobs that allow adapting to a specific data and query workload our system is intended to act as a layer on top of a distributed keyvalue store that houses the raw data as well as any indexes we design novel offline storage layout algorithms for efficiently partitioning the data to minimize the storage costs while keeping the retrieval costs low we also present an online algorithm to handle new versions being added to system using extensive experiments on large datasets we demonstrate that our system operates at the scale required in most practical scenarios and often outperforms standard baselines including a deltabased storage engine by ordersofmagnitude
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1,802.07694
Homoclinic Bifurcations of the Merging Strange Attractors in the Lorenz-like System
In this article we construct the parameter region where the existence of a homoclinic orbit to a zero equilibrium state of saddle type in the Lorenz-like system will be analytically proved in the case of a nonnegative saddle value. Then, for a qualitative description of the different types of homoclinic bifurcations, a numerical analysis of the detected parameter region is carried out to discover several new interesting bifurcation scenarios.
math.DS
in this article we construct the parameter region where the existence of a homoclinic orbit to a zero equilibrium state of saddle type in the lorenzlike system will be analytically proved in the case of a nonnegative saddle value then for a qualitative description of the different types of homoclinic bifurcations a numerical analysis of the detected parameter region is carried out to discover several new interesting bifurcation scenarios
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1,802.07695
Quadric Inclusion Programs: an LMI Approach to H[infinity]-Model Identification
Practical application of H[infinity] robust control relies on system identification of a valid model-set, described by a linear system in feedback with a stable norm-bounded uncertainty, which must explains all possible (or at least all previously measured) behavior for the control plant. Such models can be viewed as norm-bounded inclusions in the frequency domain, and this note introduces the "Quadric Inclusion Program" that can identify inclusions from input--output data as a convex problem. We prove several key properties of this algorithm and give a geometric interpretation for its behavior. While we stress that the inclusion fitting is outlier-sensitive by design, we offer a method to mitigate the effect of measurement noise. We apply this method to robustly approximate simulated frequency domain data using orthonormal basis functions. The result compares favorably with a least squares approach that satisfies the same data inclusion requirements.
math.OC cs.SY math.DS
practical application of hinfinity robust control relies on system identification of a valid modelset described by a linear system in feedback with a stable normbounded uncertainty which must explains all possible or at least all previously measured behavior for the control plant such models can be viewed as normbounded inclusions in the frequency domain and this note introduces the quadric inclusion program that can identify inclusions from inputoutput data as a convex problem we prove several key properties of this algorithm and give a geometric interpretation for its behavior while we stress that the inclusion fitting is outliersensitive by design we offer a method to mitigate the effect of measurement noise we apply this method to robustly approximate simulated frequency domain data using orthonormal basis functions the result compares favorably with a least squares approach that satisfies the same data inclusion requirements
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1,802.07696
A likelihood ratio approach to sequential change point detection for a general class of parameters
In this paper we propose a new approach for sequential monitoring of a parameter of a $d$-dimensional time series, which can be estimated by approximately linear functionals of the empirical distribution function. We consider a closed-end-method, which is motivated by the likelihood ratio test principle and compare the new method with two alternative procedures. We also incorporate self-normalization such that estimation of the long-run variance is not necessary. We prove that for a large class of testing problems the new detection scheme has asymptotic level $\alpha$ and is consistent. The asymptotic theory is illustrated for the important cases of monitoring a change in the mean, variance and correlation. By means of a simulation study it is demonstrated that the new test performs better than the currently available procedures for these problems.Finally the methodology is illustrated by a small data example investigating index prices from the dot-com bubble.
math.ST stat.ME stat.TH
in this paper we propose a new approach for sequential monitoring of a parameter of a ddimensional time series which can be estimated by approximately linear functionals of the empirical distribution function we consider a closedendmethod which is motivated by the likelihood ratio test principle and compare the new method with two alternative procedures we also incorporate selfnormalization such that estimation of the longrun variance is not necessary we prove that for a large class of testing problems the new detection scheme has asymptotic level alpha and is consistent the asymptotic theory is illustrated for the important cases of monitoring a change in the mean variance and correlation by means of a simulation study it is demonstrated that the new test performs better than the currently available procedures for these problemsfinally the methodology is illustrated by a small data example investigating index prices from the dotcom bubble
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1,802.07697
Approximation Algorithms for Cascading Prediction Models
We present an approximation algorithm that takes a pool of pre-trained models as input and produces from it a cascaded model with similar accuracy but lower average-case cost. Applied to state-of-the-art ImageNet classification models, this yields up to a 2x reduction in floating point multiplications, and up to a 6x reduction in average-case memory I/O. The auto-generated cascades exhibit intuitive properties, such as using lower-resolution input for easier images and requiring higher prediction confidence when using a computationally cheaper model.
cs.LG cs.AI cs.NE
we present an approximation algorithm that takes a pool of pretrained models as input and produces from it a cascaded model with similar accuracy but lower averagecase cost applied to stateoftheart imagenet classification models this yields up to a 2x reduction in floating point multiplications and up to a 6x reduction in averagecase memory io the autogenerated cascades exhibit intuitive properties such as using lowerresolution input for easier images and requiring higher prediction confidence when using a computationally cheaper model
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1,802.07698
Gaussian Free Field in the background of correlated random clusters, formed by metallic nanoparticles
The effect of metallic nano-particles (MNPs) on the electrostatic potential of a disordered 2D dielectric media is considered. The disorder in the media is assumed to be white-noise Coulomb impurities with normal distribution. To realize the correlations between the MNPs we have used the Ising model with an artificial temperature $T$ that controls the number of MNPs as well as their correlations. In the $T\rightarrow 0$ limit, one retrieves the Gaussian free field (GFF), and in the finite temperature the problem is equivalent to a GFF in iso-potential islands. The problem is argued to be equivalent to a scale-invariant random surface with some critical exponents which vary with $T$ and correspondingly are correlation-dependent. Two type of observables have been considered: local and global quantities. We have observed that the MNPs soften the random potential and reduce its statistical fluctuations. This softening is observed in the local as well as the geometrical quantities. The correlation function of the electrostatic and its total variance are observed to be logarithmic just like the GFF, i.e. the roughness exponent remains zero for all temperatures, whereas the proportionality constants scale with $T-T_c$. The fractal dimension of iso-potential lines ($D_f$), the exponent of the distribution function of the gyration radius ($\tau_r$), and the loop lengths ($\tau_l$), and also the exponent of the loop Green function $x_l$ change in terms of $T-T_c$ in a power-law fashion, with some critical exponents reported in the text. Importantly we have observed that $D_f(T)-D_f(T_c)\sim\frac{1}{\sqrt{\xi(T)}}$, in which $\xi(T)$ is the spin correlation length in the Ising model.
cond-mat.stat-mech
the effect of metallic nanoparticles mnps on the electrostatic potential of a disordered 2d dielectric media is considered the disorder in the media is assumed to be whitenoise coulomb impurities with normal distribution to realize the correlations between the mnps we have used the ising model with an artificial temperature t that controls the number of mnps as well as their correlations in the trightarrow 0 limit one retrieves the gaussian free field gff and in the finite temperature the problem is equivalent to a gff in isopotential islands the problem is argued to be equivalent to a scaleinvariant random surface with some critical exponents which vary with t and correspondingly are correlationdependent two type of observables have been considered local and global quantities we have observed that the mnps soften the random potential and reduce its statistical fluctuations this softening is observed in the local as well as the geometrical quantities the correlation function of the electrostatic and its total variance are observed to be logarithmic just like the gff ie the roughness exponent remains zero for all temperatures whereas the proportionality constants scale with tt_c the fractal dimension of isopotential lines d_f the exponent of the distribution function of the gyration radius tau_r and the loop lengths tau_l and also the exponent of the loop green function x_l change in terms of tt_c in a powerlaw fashion with some critical exponents reported in the text importantly we have observed that d_ftd_ft_csimfrac1sqrtxit in which xit is the spin correlation length in the ising model
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1,802.07699
Splay--density coupling in semiflexible main-chain nematic polymers with hairpins
We establish a macroscopic description of the splay--density coupling in semiflexible main-chain nematic polymers with hairpins, using a vectorial continuity constraint for the "recovered" polar order of the chain tangents and introducing chain backfolds (hairpins) as its new type of sources besides chain ends. We treat both types of sources on a unified basis as a mixture of two ideal gases with fixed composition. Performing detailed Monte Carlo simulations of nematic monodomain melts of "soft" worm-like chains with variable length and flexibility, we show via their structure factors that the chain backfolding weakens the splay--density coupling, and demonstrate how this weakening can be consistently quantified on the macroscopic level. We also probe and discuss the deviations from the noninteracting gas idealization of the chain ends and backfolds.
cond-mat.soft
we establish a macroscopic description of the splaydensity coupling in semiflexible mainchain nematic polymers with hairpins using a vectorial continuity constraint for the recovered polar order of the chain tangents and introducing chain backfolds hairpins as its new type of sources besides chain ends we treat both types of sources on a unified basis as a mixture of two ideal gases with fixed composition performing detailed monte carlo simulations of nematic monodomain melts of soft wormlike chains with variable length and flexibility we show via their structure factors that the chain backfolding weakens the splaydensity coupling and demonstrate how this weakening can be consistently quantified on the macroscopic level we also probe and discuss the deviations from the noninteracting gas idealization of the chain ends and backfolds
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1,802.077
A rainbow blow-up lemma
We prove a rainbow version of the blow-up lemma of Koml\'os, S\'ark\"ozy and Szemer\'edi for $\mu n$-bounded edge colourings. This enables the systematic study of rainbow embeddings of bounded degree spanning subgraphs. As one application, we show how our blow-up lemma can be used to transfer the bandwidth theorem of B\"ottcher, Schacht and Taraz to the rainbow setting. It can also be employed as a tool beyond the setting of $\mu n$-bounded edge colourings. Kim, K\"uhn, Kupavskii and Osthus exploit this to prove several rainbow decomposition results. Our proof methods include the strategy of an alternative proof of the blow-up lemma given by R\"odl and Ruci\'nski, the switching method, and the partial resampling algorithm developed by Harris and Srinivasan.
math.CO
we prove a rainbow version of the blowup lemma of komlos sarkozy and szemeredi for mu nbounded edge colourings this enables the systematic study of rainbow embeddings of bounded degree spanning subgraphs as one application we show how our blowup lemma can be used to transfer the bandwidth theorem of bottcher schacht and taraz to the rainbow setting it can also be employed as a tool beyond the setting of mu nbounded edge colourings kim kuhn kupavskii and osthus exploit this to prove several rainbow decomposition results our proof methods include the strategy of an alternative proof of the blowup lemma given by rodl and rucinski the switching method and the partial resampling algorithm developed by harris and srinivasan
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1,802.07701
Statistics on some classes of knot shadows
The present paper is concerned with the enumeration of the state diagrams for some classes of knot shadows endowed with the usual connected sum operation. We focus on shadows that are recursively generated by knot shadows with up to 3 crossings, and for which the enumeration problem is solved with the help of generating polynomials.
math.CO
the present paper is concerned with the enumeration of the state diagrams for some classes of knot shadows endowed with the usual connected sum operation we focus on shadows that are recursively generated by knot shadows with up to 3 crossings and for which the enumeration problem is solved with the help of generating polynomials
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1,802.07702
ARRIVAL: Next Stop in CLS
We study the computational complexity of ARRIVAL, a zero-player game on $n$-vertex switch graphs introduced by Dohrau, G\"{a}rtner, Kohler, Matou\v{s}ek, and Welzl. They showed that the problem of deciding termination of this game is contained in $\text{NP} \cap \text{coNP}$. Karthik C. S. recently introduced a search variant of ARRIVAL and showed that it is in the complexity class PLS. In this work, we significantly improve the known upper bounds for both the decision and the search variants of ARRIVAL. First, we resolve a question suggested by Dohrau et al. and show that the decision variant of ARRIVAL is in $\text{UP} \cap \text{coUP}$. Second, we prove that the search variant of ARRIVAL is contained in CLS. Third, we give a randomized $\mathcal{O}(1.4143^n)$-time algorithm to solve both variants. Our main technical contributions are (a) an efficiently verifiable characterization of the unique witness for termination of the ARRIVAL game, and (b) an efficient way of sampling from the state space of the game. We show that the problem of finding the unique witness is contained in CLS, whereas it was previously conjectured to be FPSPACE-complete. The efficient sampling procedure yields the first algorithm for the problem that has expected runtime $\mathcal{O}(c^n)$ with $c<2$.
cs.CC
we study the computational complexity of arrival a zeroplayer game on nvertex switch graphs introduced by dohrau gartner kohler matouvsek and welzl they showed that the problem of deciding termination of this game is contained in textnp cap textconp karthik c s recently introduced a search variant of arrival and showed that it is in the complexity class pls in this work we significantly improve the known upper bounds for both the decision and the search variants of arrival first we resolve a question suggested by dohrau et al and show that the decision variant of arrival is in textup cap textcoup second we prove that the search variant of arrival is contained in cls third we give a randomized mathcalo14143ntime algorithm to solve both variants our main technical contributions are a an efficiently verifiable characterization of the unique witness for termination of the arrival game and b an efficient way of sampling from the state space of the game we show that the problem of finding the unique witness is contained in cls whereas it was previously conjectured to be fpspacecomplete the efficient sampling procedure yields the first algorithm for the problem that has expected runtime mathcalocn with c2
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1,802.07703
Verifying detailed fluctuation relations for discrete feedback-controlled quantum dynamics
Discrete quantum feedback control consists of a managed dynamics according to the information acquired by a previous measurement. Energy fluctuations along such dynamics satisfy generalized fluctuation relations, which are useful tools to study the thermodynamics of systems far away from equilibrium. Due to the practical challenge to assess energy fluctuations in the quantum scenario, the experimental verification of detailed fluctuation relations in the presence of feedback control remains elusive. We present a feasible method to experimentally verify detailed fluctuation relations for discrete feedback control quantum dynamics. Two detailed fluctuation relations are developed and employed. The method is based on a quantum interferometric strategy that allows the verification of fluctuation relations in the presence of feedback control. An analytical example to illustrate the applicability of the method is discussed. The comprehensive technique introduced here can be experimentally implemented at a microscale with the current technology in a variety of experimental platforms.
quant-ph cond-mat.stat-mech
discrete quantum feedback control consists of a managed dynamics according to the information acquired by a previous measurement energy fluctuations along such dynamics satisfy generalized fluctuation relations which are useful tools to study the thermodynamics of systems far away from equilibrium due to the practical challenge to assess energy fluctuations in the quantum scenario the experimental verification of detailed fluctuation relations in the presence of feedback control remains elusive we present a feasible method to experimentally verify detailed fluctuation relations for discrete feedback control quantum dynamics two detailed fluctuation relations are developed and employed the method is based on a quantum interferometric strategy that allows the verification of fluctuation relations in the presence of feedback control an analytical example to illustrate the applicability of the method is discussed the comprehensive technique introduced here can be experimentally implemented at a microscale with the current technology in a variety of experimental platforms
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1,802.07704
On the Fr{\o}yshov invariant and monopole Lefschetz number
Given an involution on a rational homology 3-sphere $Y$ with quotient the $3$-sphere, we prove a formula for the Lefschetz number of the map induced by this involution in the reduced monopole Floer homology. This formula is motivated by a variant of Witten's conjecture relating the Donaldson and Seiberg--Witten invariants of 4-manifolds. A key ingredient is a skein-theoretic argument, making use of an exact triangle in monopole Floer homology, that computes the Lefschetz number in terms of the Murasugi signature of the branch set and the sum of Fr{\o}yshov invariants associated to spin structures on $Y$. We discuss various applications of our formula in gauge theory, knot theory, contact geometry, and 4-dimensional topology.
math.GT
given an involution on a rational homology 3sphere y with quotient the 3sphere we prove a formula for the lefschetz number of the map induced by this involution in the reduced monopole floer homology this formula is motivated by a variant of wittens conjecture relating the donaldson and seibergwitten invariants of 4manifolds a key ingredient is a skeintheoretic argument making use of an exact triangle in monopole floer homology that computes the lefschetz number in terms of the murasugi signature of the branch set and the sum of froyshov invariants associated to spin structures on y we discuss various applications of our formula in gauge theory knot theory contact geometry and 4dimensional topology
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1,802.07705
Regularity results for a class of generalized surface quasi-geostrophic equations
We show a global existence result of weak solutions for a class of generalized Surface Quasi-Geostrophic equation in the inviscid case. We also prove the global regularity of such solutions for the equation with slightly supercritical dissipation, which turns out to correspond to a logarithmically supercritical diffusion due to the singular nature of the velocity. Our last result is the eventual regularity in the supercritical cases for such weak solutions. The main idea in the proof of the existence part is based on suitable commutator estimates along with a careful cutting into low/high frequencies and inner/outer spatial scales to pass to the limit; while the proof of both the global regularity result and the eventual regularity for the supercritical diffusion are essentially based on the use of the so-called modulus of continuity method.
math.AP math-ph math.MP
we show a global existence result of weak solutions for a class of generalized surface quasigeostrophic equation in the inviscid case we also prove the global regularity of such solutions for the equation with slightly supercritical dissipation which turns out to correspond to a logarithmically supercritical diffusion due to the singular nature of the velocity our last result is the eventual regularity in the supercritical cases for such weak solutions the main idea in the proof of the existence part is based on suitable commutator estimates along with a careful cutting into lowhigh frequencies and innerouter spatial scales to pass to the limit while the proof of both the global regularity result and the eventual regularity for the supercritical diffusion are essentially based on the use of the socalled modulus of continuity method
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1,802.07706
Stability analysis and control chaos for fractional 5D Maxwell-Bloch model
In this paper we investigate the dynamical behavior of fractional differential system associated to 5D Maxwell-Bloch model in terms of fractional Caputo derivatives.
math.DS
in this paper we investigate the dynamical behavior of fractional differential system associated to 5d maxwellbloch model in terms of fractional caputo derivatives
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1,802.07707
Logarithmic means \dots]{On the N\"orlund logarithmic means with respect to Vilenkin system in the martingale Hardy space $H_{1}$
In this paper we prove and discuss a new divergence result of N\"orlund logarithmic means with respect to Vilenkin system in Hardy space $H_1. $
math.CA
in this paper we prove and discuss a new divergence result of norlund logarithmic means with respect to vilenkin system in hardy space h_1
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1,802.07708
A Radial Measurement of the Galaxy Tidal Alignment Magnitude with BOSS Data
The anisotropy of galaxy clustering in redshift space has long been used to probe the rate of growth of cosmological perturbations. However, if galaxies are aligned by large-scale tidal fields, then a sample with an orientation-dependent selection effect has an additional anisotropy imprinted onto its correlation function. We use the LOWZ and CMASS catalogs of SDSS-III BOSS Data Release 12 to divide galaxies into two sub-samples based on their offset from the Fundamental Plane, which should be correlated with orientation. These sub-samples must trace the same underlying cosmology, but have opposite orientation-dependent selection effects. We measure the clustering parameters of each sub-sample and compare them in order to calculate the dimensionless parameter $B$, a measure of how strongly galaxies are aligned by gravitational tidal fields. We found that for CMASS (LOWZ), the measured $B$ was $-0.024 \pm 0.015$ ($-0.030 \pm 0.016$). This result can be compared to the theoretical predictions of Hirata 2009, who argued that since galaxy formation physics does not depend on the direction of the observer, the same intrinsic alignment parameters that describe galaxy-ellipticity correlations should also describe intrinsic alignments in the radial direction. We find that the ratio of observed to theoretical values is $0.51\pm 0.32$ ($0.77\pm0.41$) for CMASS (LOWZ). We combine the results to obtain a total ${\rm {Obs}/{Theory}} = 0.61\pm 0.26$. This measurement constitutes evidence (between 2 and 3$\sigma$) for radial intrinsic alignments, and is consistent with theoretical expectations ($<2\sigma$ difference).
astro-ph.CO
the anisotropy of galaxy clustering in redshift space has long been used to probe the rate of growth of cosmological perturbations however if galaxies are aligned by largescale tidal fields then a sample with an orientationdependent selection effect has an additional anisotropy imprinted onto its correlation function we use the lowz and cmass catalogs of sdssiii boss data release 12 to divide galaxies into two subsamples based on their offset from the fundamental plane which should be correlated with orientation these subsamples must trace the same underlying cosmology but have opposite orientationdependent selection effects we measure the clustering parameters of each subsample and compare them in order to calculate the dimensionless parameter b a measure of how strongly galaxies are aligned by gravitational tidal fields we found that for cmass lowz the measured b was 0024 pm 0015 0030 pm 0016 this result can be compared to the theoretical predictions of hirata 2009 who argued that since galaxy formation physics does not depend on the direction of the observer the same intrinsic alignment parameters that describe galaxyellipticity correlations should also describe intrinsic alignments in the radial direction we find that the ratio of observed to theoretical values is 051pm 032 077pm041 for cmass lowz we combine the results to obtain a total rm obstheory 061pm 026 this measurement constitutes evidence between 2 and 3sigma for radial intrinsic alignments and is consistent with theoretical expectations 2sigma difference
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1,802.07709
Magnonic Spin-Transfer Torque in Ferromagnet/Antiferromagnet/Ferromagnet Trilayer
In an antiferromagnet (AF) with uniaxial anisotropy, spin-up and spin-down magnons coexist and form an intrinsic degree of freedom resembling electrons. When polarized by an adjacent ferromagnet (F), a magnonic pure spin current can be thermally generated in an AF. We explore thermal magnon transport in an insulating F/AF/F trilayer where propagating magnons inside the AF spacer can transfer angular momenta between the two Fs. We find that a sufficiently large temperature gradient can switch the downstream F via magnonic spin-transfer torque if it is initially antiparallel with the upstream F. A reciprocal switching is achievable by reversing the temperature gradient. Using typical material parameters, we estimate the threshold to be less than 1 K/nm at room temperature, which can be reduced by raising temperature and enhancing the interfacial exchange coupling.
cond-mat.mes-hall cond-mat.mtrl-sci quant-ph
in an antiferromagnet af with uniaxial anisotropy spinup and spindown magnons coexist and form an intrinsic degree of freedom resembling electrons when polarized by an adjacent ferromagnet f a magnonic pure spin current can be thermally generated in an af we explore thermal magnon transport in an insulating faff trilayer where propagating magnons inside the af spacer can transfer angular momenta between the two fs we find that a sufficiently large temperature gradient can switch the downstream f via magnonic spintransfer torque if it is initially antiparallel with the upstream f a reciprocal switching is achievable by reversing the temperature gradient using typical material parameters we estimate the threshold to be less than 1 knm at room temperature which can be reduced by raising temperature and enhancing the interfacial exchange coupling
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1,802.0771
Medical Volume Reconstruction Techniques
Medical visualization is the use of computers to create 3D images from medical imaging data sets, almost all surgery and cancer treatment in the developed world relies on it.Volume visualization techniques includes iso-surface visualization, mesh visualization and point cloud visualization techniques, these techniques have revolutionized medicine. Much of modern medicine relies on the 3D imaging that is possible with magnetic resonance imaging (MRI) scanners, functional magnetic resonance imaging (fMRI)scanners, positron emission tomography (PET) scanners, ultrasound imaging (US) scanners, X-Ray scanners, bio-marker microscopy imaging scanners and computed tomography (CT) scanners, which make 3D images out of 2D slices. The primary goal of this report is the application-oriented optimization of existing volume rendering methods providing interactive frame rates. Techniques are presented for traditional alpha-blending rendering, surface-shaded display, maximum intensity projection (MIP), and fast previewing with fully interactive parameter control. Different preprocessing strategies are proposed for interactive iso-surface rendering and fast previewing, such as the well-known marching cube algorithm.
cs.GR
medical visualization is the use of computers to create 3d images from medical imaging data sets almost all surgery and cancer treatment in the developed world relies on itvolume visualization techniques includes isosurface visualization mesh visualization and point cloud visualization techniques these techniques have revolutionized medicine much of modern medicine relies on the 3d imaging that is possible with magnetic resonance imaging mri scanners functional magnetic resonance imaging fmriscanners positron emission tomography pet scanners ultrasound imaging us scanners xray scanners biomarker microscopy imaging scanners and computed tomography ct scanners which make 3d images out of 2d slices the primary goal of this report is the applicationoriented optimization of existing volume rendering methods providing interactive frame rates techniques are presented for traditional alphablending rendering surfaceshaded display maximum intensity projection mip and fast previewing with fully interactive parameter control different preprocessing strategies are proposed for interactive isosurface rendering and fast previewing such as the wellknown marching cube algorithm
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1,802.07711
The electromagnetic multipole moments of the charged open-flavor $Z_{\bar cq}$ states
The electromagnetic multipole moments of the open-flavor $Z_{\bar cq}$ states are investigated by assuming a diquark-antidiquark picture for their internal structure and quantum numbers $J^{PC} = 1^{+-}$ for their spin-parity. In particular, their magnetic and quadrupole moments are extracted in the framework of light-cone QCD sum rule by the help of the photon distribution amplitudes. The electromagnetic multipole moments of the open-flavor $Z_{\bar cq}$ states are important dynamical observables, which encode valuable information on their underlying structure. The results obtained for the magnetic moments of different structures are considerably large and can be measured in future experiments. We obtain very small values for the quadrupole moments of $Z_{\bar cq}$ states indicating a nonspherical charge distribution.
hep-ph hep-ex hep-lat
the electromagnetic multipole moments of the openflavor z_bar cq states are investigated by assuming a diquarkantidiquark picture for their internal structure and quantum numbers jpc 1 for their spinparity in particular their magnetic and quadrupole moments are extracted in the framework of lightcone qcd sum rule by the help of the photon distribution amplitudes the electromagnetic multipole moments of the openflavor z_bar cq states are important dynamical observables which encode valuable information on their underlying structure the results obtained for the magnetic moments of different structures are considerably large and can be measured in future experiments we obtain very small values for the quadrupole moments of z_bar cq states indicating a nonspherical charge distribution
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1,802.07712
Condition numbers of stochastic mean payoff games and what they say about nonarchimedean semidefinite programming
Semidefinite programming can be considered over any real closed field, including fields of Puiseux series equipped with their nonarchimedean valuation. Nonarchimedean semidefinite programs encode parametric families of classical semidefinite programs, for sufficiently large values of the parameter. Recently, a correspondence has been established between nonarchimedean semidefinite programs and stochastic mean payoff games with perfect information. This correspondence relies on tropical geometry. It allows one to solve generic nonarchimedean semidefinite feasibility problems, of large scale, by means of stochastic game algorithms. In this paper, we show that the mean payoff of these games can be interpreted as a condition number for the corresponding nonarchimedean feasibility problems. This number measures how close a feasible instance is from being infeasible, and vice versa. We show that it coincides with the maximal radius of a ball in Hilbert's projective metric, that is included in the feasible set. The geometric interpretation of the condition number relies in particular on a duality theorem for tropical semidefinite feasibility programs. Then, we bound the complexity of the feasibility problem in terms of the condition number. We finally give explicit bounds for this condition number, in terms of the characteristics of the stochastic game. As a consequence, we show that the simplest algorithm to decide whether a stochastic mean payoff game is winning, namely value iteration, has a pseudopolynomial complexity when the number of random positions is fixed.
math.OC cs.GT math.CO
semidefinite programming can be considered over any real closed field including fields of puiseux series equipped with their nonarchimedean valuation nonarchimedean semidefinite programs encode parametric families of classical semidefinite programs for sufficiently large values of the parameter recently a correspondence has been established between nonarchimedean semidefinite programs and stochastic mean payoff games with perfect information this correspondence relies on tropical geometry it allows one to solve generic nonarchimedean semidefinite feasibility problems of large scale by means of stochastic game algorithms in this paper we show that the mean payoff of these games can be interpreted as a condition number for the corresponding nonarchimedean feasibility problems this number measures how close a feasible instance is from being infeasible and vice versa we show that it coincides with the maximal radius of a ball in hilberts projective metric that is included in the feasible set the geometric interpretation of the condition number relies in particular on a duality theorem for tropical semidefinite feasibility programs then we bound the complexity of the feasibility problem in terms of the condition number we finally give explicit bounds for this condition number in terms of the characteristics of the stochastic game as a consequence we show that the simplest algorithm to decide whether a stochastic mean payoff game is winning namely value iteration has a pseudopolynomial complexity when the number of random positions is fixed
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1,802.07713
Cutting Lemma and Union Lemma for the Domination Game
Two new techniques are introduced into the theory of the domination game. The cutting lemma bounds the game domination number of a partially dominated graph with the game domination number of suitably modified partially dominated graph. The union lemma bounds the S-game domination number of a disjoint union of paths using appropriate weighting functions. Using these tools a conjecture asserting that the so-called three legged spiders are game domination critical graphs is proved. An extended cutting lemma is also derived and all game domination critical trees on 18, 19, and 20 vertices are listed.
math.CO
two new techniques are introduced into the theory of the domination game the cutting lemma bounds the game domination number of a partially dominated graph with the game domination number of suitably modified partially dominated graph the union lemma bounds the sgame domination number of a disjoint union of paths using appropriate weighting functions using these tools a conjecture asserting that the socalled three legged spiders are game domination critical graphs is proved an extended cutting lemma is also derived and all game domination critical trees on 18 19 and 20 vertices are listed
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1,802.07714
Detecting Learning vs Memorization in Deep Neural Networks using Shared Structure Validation Sets
The roles played by learning and memorization represent an important topic in deep learning research. Recent work on this subject has shown that the optimization behavior of DNNs trained on shuffled labels is qualitatively different from DNNs trained with real labels. Here, we propose a novel permutation approach that can differentiate memorization from learning in deep neural networks (DNNs) trained as usual (i.e., using the real labels to guide the learning, rather than shuffled labels). The evaluation of weather the DNN has learned and/or memorized, happens in a separate step where we compare the predictive performance of a shallow classifier trained with the features learned by the DNN, against multiple instances of the same classifier, trained on the same input, but using shuffled labels as outputs. By evaluating these shallow classifiers in validation sets that share structure with the training set, we are able to tell apart learning from memorization. Application of our permutation approach to multi-layer perceptrons and convolutional neural networks trained on image data corroborated many findings from other groups. Most importantly, our illustrations also uncovered interesting dynamic patterns about how DNNs memorize over increasing numbers of training epochs, and support the surprising result that DNNs are still able to learn, rather than only memorize, when trained with pure Gaussian noise as input.
stat.ML cs.LG
the roles played by learning and memorization represent an important topic in deep learning research recent work on this subject has shown that the optimization behavior of dnns trained on shuffled labels is qualitatively different from dnns trained with real labels here we propose a novel permutation approach that can differentiate memorization from learning in deep neural networks dnns trained as usual ie using the real labels to guide the learning rather than shuffled labels the evaluation of weather the dnn has learned andor memorized happens in a separate step where we compare the predictive performance of a shallow classifier trained with the features learned by the dnn against multiple instances of the same classifier trained on the same input but using shuffled labels as outputs by evaluating these shallow classifiers in validation sets that share structure with the training set we are able to tell apart learning from memorization application of our permutation approach to multilayer perceptrons and convolutional neural networks trained on image data corroborated many findings from other groups most importantly our illustrations also uncovered interesting dynamic patterns about how dnns memorize over increasing numbers of training epochs and support the surprising result that dnns are still able to learn rather than only memorize when trained with pure gaussian noise as input
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1,802.07715
Theory of open quantum dynamics with hybrid noise
We develop a theory to describe dynamics of a non-stationary open quantum system interacting with a hybrid environment, which includes high-frequency and low-frequency noise components. One part of the system-bath interaction is treated in a perturbative manner, whereas the other part is considered exactly. This approach allows us to derive a set of master equations where the relaxation rates are expressed as convolutions of the Bloch-Redfield and Marcus formulas. Our theory enables analysis of systems that have extremely small energy gaps in the presence of a realistic environment. As an illustration, we apply the theory to the 16-qubit quantum annealing problem with dangling qubits and show good agreement with experimental results.
quant-ph cond-mat.stat-mech
we develop a theory to describe dynamics of a nonstationary open quantum system interacting with a hybrid environment which includes highfrequency and lowfrequency noise components one part of the systembath interaction is treated in a perturbative manner whereas the other part is considered exactly this approach allows us to derive a set of master equations where the relaxation rates are expressed as convolutions of the blochredfield and marcus formulas our theory enables analysis of systems that have extremely small energy gaps in the presence of a realistic environment as an illustration we apply the theory to the 16qubit quantum annealing problem with dangling qubits and show good agreement with experimental results
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1,802.07716
Sampling real algebraic varieties for topological data analysis
Topological data analysis (TDA) provides a growing body of tools for computing geometric and topological information about spaces from a finite sample of points. We present a new adaptive algorithm for finding provably dense samples of points on real algebraic varieties given a set of defining polynomials. The algorithm utilizes methods from numerical algebraic geometry to give formal guarantees about the density of the sampling and it also employs geometric heuristics to reduce the size of the sample. As TDA methods consume significant computational resources that scale poorly in the number of sample points, our sampling minimization makes applying TDA methods more feasible. We provide a software package that implements the algorithm and also demonstrate the implementation with several examples.
math.AT math.AG math.NA
topological data analysis tda provides a growing body of tools for computing geometric and topological information about spaces from a finite sample of points we present a new adaptive algorithm for finding provably dense samples of points on real algebraic varieties given a set of defining polynomials the algorithm utilizes methods from numerical algebraic geometry to give formal guarantees about the density of the sampling and it also employs geometric heuristics to reduce the size of the sample as tda methods consume significant computational resources that scale poorly in the number of sample points our sampling minimization makes applying tda methods more feasible we provide a software package that implements the algorithm and also demonstrate the implementation with several examples
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1,802.07717
Resummation of diagrammatic series with zero convergence radius for strongly correlated fermions
We demonstrate that summing up series of Feynman diagrams can yield unbiased accurate results for strongly-correlated fermions even when the convergence radius vanishes. We consider the unitary Fermi gas, a model of non-relativistic fermions in three-dimensional continuous space. Diagrams are built from partially-dressed or fully-dressed propagators of single particles and pairs. The series is resummed by a conformal-Borel transformation that incorporates the large-order behavior and the analytic structure in the Borel plane, which are found by the instanton approach. We report highly accurate numerical results for the equation of state in the normal unpolarized regime, and reconcile experimental data with the theoretically conjectured fourth virial coefficient.
cond-mat.quant-gas
we demonstrate that summing up series of feynman diagrams can yield unbiased accurate results for stronglycorrelated fermions even when the convergence radius vanishes we consider the unitary fermi gas a model of nonrelativistic fermions in threedimensional continuous space diagrams are built from partiallydressed or fullydressed propagators of single particles and pairs the series is resummed by a conformalborel transformation that incorporates the largeorder behavior and the analytic structure in the borel plane which are found by the instanton approach we report highly accurate numerical results for the equation of state in the normal unpolarized regime and reconcile experimental data with the theoretically conjectured fourth virial coefficient
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1,802.07718
High statistics lattice study of stress tensor correlators in pure $SU(3)$ gauge theory
We compute the Euclidean correlators of the stress tensor in pure $SU(3)$ Yang-Mills theory at finite temperature at zero and finite spatial momenta with lattice simulations. We perform continuum extrapolations using $N_\tau=10,12,16,20$ lattices with renormalized anisotropy 2. We use these correlators to estimate the shear viscosity of the gluon plasma in the deconfined phase. For $T=1.5T_c$ we obtain $\eta/s=0.17(2)$.
hep-lat
we compute the euclidean correlators of the stress tensor in pure su3 yangmills theory at finite temperature at zero and finite spatial momenta with lattice simulations we perform continuum extrapolations using n_tau10121620 lattices with renormalized anisotropy 2 we use these correlators to estimate the shear viscosity of the gluon plasma in the deconfined phase for t15t_c we obtain etas0172
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1,802.07719
Unlimited Accumulation of Electromagnetic Energy Using Time-Varying Reactive Elements
Accumulation of energy by reactive elements is limited by the amplitude of time-harmonic external sources. In the steady-state regime, all incident power is fully reflected back to the source, and the stored energy does not increase in time, although the external source continuously supplies energy. Here, we show that this claim is not true if the reactive element is time-varying, and time-varying lossless loads of a transmission line or lossless metasurfaces can accumulate electromagnetic energy supplied by a time-harmonic source continuously in time without any theoretical limit. We analytically derive the required time dependence of the load reactance and show that it can be in principle realized as a series connection of mixers and filters. Furthermore, we prove that properly designing time-varying LC circuits one can arbitrarily engineer the time dependence of the current in the circuit fed by a given time-harmonic source. As an example, we theoretically demonstrate a circuit with a linearly increasing current through the inductor. Such LC circuits can accumulate huge energy from both the time-harmonic external source and the pump which works on varying the circuit elements in time. Finally, we discuss how this stored energy can be released in form of a time-compressed pulse.
physics.app-ph
accumulation of energy by reactive elements is limited by the amplitude of timeharmonic external sources in the steadystate regime all incident power is fully reflected back to the source and the stored energy does not increase in time although the external source continuously supplies energy here we show that this claim is not true if the reactive element is timevarying and timevarying lossless loads of a transmission line or lossless metasurfaces can accumulate electromagnetic energy supplied by a timeharmonic source continuously in time without any theoretical limit we analytically derive the required time dependence of the load reactance and show that it can be in principle realized as a series connection of mixers and filters furthermore we prove that properly designing timevarying lc circuits one can arbitrarily engineer the time dependence of the current in the circuit fed by a given timeharmonic source as an example we theoretically demonstrate a circuit with a linearly increasing current through the inductor such lc circuits can accumulate huge energy from both the timeharmonic external source and the pump which works on varying the circuit elements in time finally we discuss how this stored energy can be released in form of a timecompressed pulse
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1,802.0772
Dark quarkonium formation in the early universe
The relic abundance of heavy stable particles charged under a confining gauge group can be depleted by a second stage of annihilations near the deconfinement temperature. This proceeds via the formation of quarkonia-like states, in which the heavy pair subsequently annihilates. The size of the quarkonium formation cross section was the subject of some debate. We estimate this cross section in a simple toy model. The dominant process can be viewed as a rearrangement of the heavy and light quarks, leading to a geometric cross section of hadronic size. In contrast, processes in which only the heavy constituents are involved lead to mass-suppressed cross sections. These results apply to any scenario with bound states of sizes much larger than their inverse mass, such as U(1) models with charged particles of different masses, and can be used to construct ultra-heavy dark-matter models with masses above the na\"ive unitarity bound. They are also relevant for the cosmology of any stable colored relic.
hep-ph
the relic abundance of heavy stable particles charged under a confining gauge group can be depleted by a second stage of annihilations near the deconfinement temperature this proceeds via the formation of quarkonialike states in which the heavy pair subsequently annihilates the size of the quarkonium formation cross section was the subject of some debate we estimate this cross section in a simple toy model the dominant process can be viewed as a rearrangement of the heavy and light quarks leading to a geometric cross section of hadronic size in contrast processes in which only the heavy constituents are involved lead to masssuppressed cross sections these results apply to any scenario with bound states of sizes much larger than their inverse mass such as u1 models with charged particles of different masses and can be used to construct ultraheavy darkmatter models with masses above the naive unitarity bound they are also relevant for the cosmology of any stable colored relic
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1,802.07721
Discussion on "Sparse graphs using exchangeable random measures" by Francois Caron and Emily B. Fox
This is a discussion on "Sparse graphs using exchangeable random measures" by Francois Caron and Emily B. Fox, published in Journal of the Royal Statistical Society, Series B, 2017.
stat.ME
this is a discussion on sparse graphs using exchangeable random measures by francois caron and emily b fox published in journal of the royal statistical society series b 2017
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1,802.07722
Generalized entropy formalism and a new holographic dark energy model
Recently, the R\'{e}nyi and Tsallis generalized entropies have extensively been used in order to study various cosmological and gravitational setups. Here, using a special type of generalized entropy, a generalization of both the R\'{e}nyi and Tsallis entropy, together with holographic principle, we build a new model for holographic dark energy. Thereinafter, considering a flat FRW universe, filled by a pressureless component and the new obtained dark energy model, the evolution of cosmos has been investigated showing satisfactory results and behavior. In our model, the Hubble horizon plays the role of IR cutoff, and there is no mutual interaction between the cosmos components. Our results indicate that the generalized entropy formalism may open a new window to become more familiar with the nature of spacetime and its properties.
gr-qc hep-th
recently the renyi and tsallis generalized entropies have extensively been used in order to study various cosmological and gravitational setups here using a special type of generalized entropy a generalization of both the renyi and tsallis entropy together with holographic principle we build a new model for holographic dark energy thereinafter considering a flat frw universe filled by a pressureless component and the new obtained dark energy model the evolution of cosmos has been investigated showing satisfactory results and behavior in our model the hubble horizon plays the role of ir cutoff and there is no mutual interaction between the cosmos components our results indicate that the generalized entropy formalism may open a new window to become more familiar with the nature of spacetime and its properties
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1,802.07723
Possible Photometric Signatures of Moderately Advanced Civilizations: The Clarke Exobelt
This paper puts forward a possible new indicator for the presence of moderately advanced civilizations on transiting exoplanets. The idea is to examine the region of space around a planet where potential geostationary or geosynchronous satellites would orbit (herafter, the Clarke exobelt). Civilizations with a high density of devices and/or space junk in that region, but otherwise similar to ours in terms of space technology (our working definition of "moderately advanced"), may leave a noticeable imprint on the light curve of the parent star. The main contribution to such signature comes from the exobelt edge, where its opacity is maximum due to geometrical projection. Numerical simulations have been conducted for a variety of possible scenarios. In some cases, a Clarke exobelt with a fractional face-on opacity of ~1E-4 would be easily observable with existing instrumentation. Simulations of Clarke exobelts and natural rings are used to quantify how they can be distinguished by their light curve.
astro-ph.EP astro-ph.SR
this paper puts forward a possible new indicator for the presence of moderately advanced civilizations on transiting exoplanets the idea is to examine the region of space around a planet where potential geostationary or geosynchronous satellites would orbit herafter the clarke exobelt civilizations with a high density of devices andor space junk in that region but otherwise similar to ours in terms of space technology our working definition of moderately advanced may leave a noticeable imprint on the light curve of the parent star the main contribution to such signature comes from the exobelt edge where its opacity is maximum due to geometrical projection numerical simulations have been conducted for a variety of possible scenarios in some cases a clarke exobelt with a fractional faceon opacity of 1e4 would be easily observable with existing instrumentation simulations of clarke exobelts and natural rings are used to quantify how they can be distinguished by their light curve
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1,802.07724
Feasibility Study for BioLEIR
The biomedical community asked CERN to investigate the possibility to transform the Low Energy Ion Ring (LEIR) accelerator into a multidisciplinary, biomedical research facility (BioLEIR) that could provide ample, high-quality beams of a range of light ions suitable for clinically oriented fundamental research on cell cultures and for radiation instrumentation development. BioLEIR would be operated when LEIR is not providing heavy ions for the CERN physics programme. The study group was mandated to write a Feasibility Study Report, using high-level engineering estimates based on previous experience, with the aim to: - collect the requirements for such a facility from the biomedical community in close collaboration with the International Strategy Committee for CERN Medical Applications; - determine a coherent set of beam parameters, based on the requirements; - explore whether the beam requirements can be met throughout the facility, from the source to the biomedical end-stations; - perform a feasibility study of the facility, taking into consideration the overall CERN schedules and programmes; - favour simplicity and robustness of the facility design, while minimizing the cost of maintenance and operation; - establish a high-level costing of material and personnel needed for project implementation; - describe the preferred installation scenario; - perform a high-level risk analysis for the project; - identify the areas of potential difficulty, and the required R&D should the study go ahead and become a project.
physics.ins-det physics.acc-ph
the biomedical community asked cern to investigate the possibility to transform the low energy ion ring leir accelerator into a multidisciplinary biomedical research facility bioleir that could provide ample highquality beams of a range of light ions suitable for clinically oriented fundamental research on cell cultures and for radiation instrumentation development bioleir would be operated when leir is not providing heavy ions for the cern physics programme the study group was mandated to write a feasibility study report using highlevel engineering estimates based on previous experience with the aim to collect the requirements for such a facility from the biomedical community in close collaboration with the international strategy committee for cern medical applications determine a coherent set of beam parameters based on the requirements explore whether the beam requirements can be met throughout the facility from the source to the biomedical endstations perform a feasibility study of the facility taking into consideration the overall cern schedules and programmes favour simplicity and robustness of the facility design while minimizing the cost of maintenance and operation establish a highlevel costing of material and personnel needed for project implementation describe the preferred installation scenario perform a highlevel risk analysis for the project identify the areas of potential difficulty and the required rd should the study go ahead and become a project
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1,802.07725
Increased Heat Transport in Ultra-Hot Jupiter Atmospheres Through H$_2$ Dissociation/Recombination
A new class of exoplanets is beginning to emerge: planets whose dayside atmospheres more closely resemble stellar atmospheres as most of their molecular constituents dissociate. The effects of the dissociation of these species will be varied and must be carefully accounted for. Here we take the first steps towards understanding the consequences of dissociation and recombination of molecular hydrogen (H$_2$) on atmospheric heat recirculation. Using a simple energy balance model with eastward winds, we demonstrate that H$_2$ dissociation/recombination can significantly increase the day$-$night heat transport on ultra-hot Jupiters (UHJs): gas giant exoplanets where significant H$_2$ dissociation occurs. The atomic hydrogen from the highly irradiated daysides of UHJs will transport some of the energy deposited on the dayside towards the nightside of the planet where the H atoms recombine into H$_2$; this mechanism bears similarities to latent heat. Given a fixed wind speed, this will act to increase the heat recirculation efficiency; alternatively, a measured heat recirculation efficiency will require slower wind speeds after accounting for H$_2$ dissociation/recombination.
astro-ph.EP
a new class of exoplanets is beginning to emerge planets whose dayside atmospheres more closely resemble stellar atmospheres as most of their molecular constituents dissociate the effects of the dissociation of these species will be varied and must be carefully accounted for here we take the first steps towards understanding the consequences of dissociation and recombination of molecular hydrogen h_2 on atmospheric heat recirculation using a simple energy balance model with eastward winds we demonstrate that h_2 dissociationrecombination can significantly increase the daynight heat transport on ultrahot jupiters uhjs gas giant exoplanets where significant h_2 dissociation occurs the atomic hydrogen from the highly irradiated daysides of uhjs will transport some of the energy deposited on the dayside towards the nightside of the planet where the h atoms recombine into h_2 this mechanism bears similarities to latent heat given a fixed wind speed this will act to increase the heat recirculation efficiency alternatively a measured heat recirculation efficiency will require slower wind speeds after accounting for h_2 dissociationrecombination
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1,802.07726
Exact Bremsstrahlung functions in ABJM theory
In this paper we study the Bremsstrahlung functions for the 1/6 BPS and the 1/2 BPS Wilson lines in ABJM theory. First we use a superconformal defect approach to prove a conjectured relation between the Bremsstrahlung functions associated to the geometric ($B^{\varphi}_{1/6}$) and R-symmetry ($B^{\theta}_{1/6}$) deformations of the 1/6 BPS Wilson line. This result, non-trivially following from a defect supersymmetric Ward identity, provides an exact expression for $B^{\theta}_{1/6}$ based on a known result for $B^{\varphi}_{1/6}$. Subsequently, we explore the consequences of this relation for the 1/2 BPS Wilson line and, using the localization result for the multiply wound Wilson loop, we provide an exact closed form for the corresponding Bremsstrahlung function. Interestingly, for the comparison with integrability, this expression appears particularly natural in terms of the conjectured interpolating function $h(\lambda)$. During the derivation of these results we analyze the protected defect supermultiplets associated to the broken symmetries, including their two- and three-point correlators.
hep-th
in this paper we study the bremsstrahlung functions for the 16 bps and the 12 bps wilson lines in abjm theory first we use a superconformal defect approach to prove a conjectured relation between the bremsstrahlung functions associated to the geometric bvarphi_16 and rsymmetry btheta_16 deformations of the 16 bps wilson line this result nontrivially following from a defect supersymmetric ward identity provides an exact expression for btheta_16 based on a known result for bvarphi_16 subsequently we explore the consequences of this relation for the 12 bps wilson line and using the localization result for the multiply wound wilson loop we provide an exact closed form for the corresponding bremsstrahlung function interestingly for the comparison with integrability this expression appears particularly natural in terms of the conjectured interpolating function hlambda during the derivation of these results we analyze the protected defect supermultiplets associated to the broken symmetries including their two and threepoint correlators
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1,802.07727
The X-shooter GRB afterglow legacy sample (XS-GRB)
In this work we present spectra of all $\gamma$-ray burst (GRB) afterglows that have been promptly observed with the X-shooter spectrograph until 31-03-2017. In total, we obtained spectroscopic observations of 103 individual GRBs observed within 48 hours of the GRB trigger. Redshifts have been measured for 97 per cent of these, covering a redshift range from 0.059 to 7.84. Based on a set of observational selection criteria that minimize biases with regards to intrinsic properties of the GRBs, the follow-up effort has been focused on producing a homogeneous sample of 93 afterglow spectra for GRBs discovered by the Swift satellite. We here provide a public release of all the reduced spectra, including continuum estimates and telluric absorption corrections. For completeness, we also provide reductions for the 18 late-time observations of the underlying host galaxies. We provide an assessment of the degree of completeness with respect to the parent GRB population, in terms of the X-ray properties of the bursts in the sample and find that the sample presented here is representative of the full Swift sample. We constrain the fraction of dark bursts to be < 28 per cent and we confirm previous results that higher optical darkness is correlated with increased X-ray absorption. For the 42 bursts for which it is possible, we provide a measurement of the neutral hydrogen column density, increasing the total number of published HI column density measurements by $\sim$ 33 per cent. This dataset provides a unique resource to study the ISM across cosmic time, from the local progenitor surroundings to the intervening universe.
astro-ph.HE
in this work we present spectra of all gammaray burst grb afterglows that have been promptly observed with the xshooter spectrograph until 31032017 in total we obtained spectroscopic observations of 103 individual grbs observed within 48 hours of the grb trigger redshifts have been measured for 97 per cent of these covering a redshift range from 0059 to 784 based on a set of observational selection criteria that minimize biases with regards to intrinsic properties of the grbs the followup effort has been focused on producing a homogeneous sample of 93 afterglow spectra for grbs discovered by the swift satellite we here provide a public release of all the reduced spectra including continuum estimates and telluric absorption corrections for completeness we also provide reductions for the 18 latetime observations of the underlying host galaxies we provide an assessment of the degree of completeness with respect to the parent grb population in terms of the xray properties of the bursts in the sample and find that the sample presented here is representative of the full swift sample we constrain the fraction of dark bursts to be 28 per cent and we confirm previous results that higher optical darkness is correlated with increased xray absorption for the 42 bursts for which it is possible we provide a measurement of the neutral hydrogen column density increasing the total number of published hi column density measurements by sim 33 per cent this dataset provides a unique resource to study the ism across cosmic time from the local progenitor surroundings to the intervening universe
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1,802.07728
Light Primordial Exotic Compact Objects as All Dark Matter
The radiation emitted by horizonless exotic compact objects (ECOs), such as wormholes, 2-2-holes, fuzzballs, gravastars, boson stars, collapsed polymers, superspinars etc., is expected to be strongly suppressed when compared to the radiation of black holes. If large primordial curvature fluctuations collapse into such objects instead of black holes, they do not evaporate or evaporate much slower than black holes and could thus constitute all of the dark matter with masses below $M < 10^{-16}M_\odot.$ We reevaluate the relevant experimental constraints for light ECOs in this mass range and show that very large new parameter space down to ECO masses $M\sim 10\,{\rm TeV}$ opens up for light primordial dark matter. A new dedicated experimental program is needed to test this mass range of primordial dark matter.
astro-ph.CO gr-qc hep-ph
the radiation emitted by horizonless exotic compact objects ecos such as wormholes 22holes fuzzballs gravastars boson stars collapsed polymers superspinars etc is expected to be strongly suppressed when compared to the radiation of black holes if large primordial curvature fluctuations collapse into such objects instead of black holes they do not evaporate or evaporate much slower than black holes and could thus constitute all of the dark matter with masses below m 1016m_odot we reevaluate the relevant experimental constraints for light ecos in this mass range and show that very large new parameter space down to eco masses msim 10rm tev opens up for light primordial dark matter a new dedicated experimental program is needed to test this mass range of primordial dark matter
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1,802.07729
Facilitated quantum cellular automata as simple models with nonthermal eigenstates and dynamics
We introduce and describe a class of simple facilitated quantum spin models in which the dynamics is due to the repeated application of unitary gates. The gates are applied periodically in time, so their combined action constitutes a Floquet unitary. The dynamics of the models we discuss can be classically simulated, and their eigenstates classically constructed (although they are highly entangled). We consider a variety of models in both one and two dimensions, involving Clifford gates and Toffoli gates. For some of these models, we explicitly construct conserved densities; thus these models are "integrable." The other models do not seem to be integrable; yet, for some system sizes and boundary conditions, their eigenstate entanglement is strongly subthermal. Some of the models have exponentially many eigenstates in which one or more sites are "disentangled" from the rest of the system, as a consequence of reflection symmetry.
cond-mat.stat-mech cond-mat.dis-nn quant-ph
we introduce and describe a class of simple facilitated quantum spin models in which the dynamics is due to the repeated application of unitary gates the gates are applied periodically in time so their combined action constitutes a floquet unitary the dynamics of the models we discuss can be classically simulated and their eigenstates classically constructed although they are highly entangled we consider a variety of models in both one and two dimensions involving clifford gates and toffoli gates for some of these models we explicitly construct conserved densities thus these models are integrable the other models do not seem to be integrable yet for some system sizes and boundary conditions their eigenstate entanglement is strongly subthermal some of the models have exponentially many eigenstates in which one or more sites are disentangled from the rest of the system as a consequence of reflection symmetry
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1,802.0773
The Environments of the Most Energetic Gamma-Ray Bursts
We analyze the properties of a sample of long gamma-ray bursts (LGRBs) detected by the Fermi satellite that have a spectroscopic redshift and good follow-up coverage at both X-ray and optical/nIR wavelengths. The evolution of LGRB afterglows depends on the density profile of the external medium, enabling us to separate wind or ISM-like environments based on the observations. We do this by identifying the environment that provides the best agreement between estimates of $p$, the index of the underlying power-law distribution of electron energies, as determined by the behavior of the afterglow in different spectral/temporal regimes. At 11 rest-frame hours after trigger, we find a roughly even split between ISM-like and wind-like environments. We further find a 2$\sigma$ separation in the prompt emission energy distributions of wind-like and ISM-like bursts. We investigate the underlying physical parameters of the shock, and calculate the (degenerate) product of density and magnetic field energy ($\epsilon_B$). We show that $\epsilon_B$ must be $\ll 10^{-2}$ to avoid implied densities comparable to the intergalactic medium. Finally, we find that the most precisely constrained observations disagree on $p$ by more than would be expected based on observational errors alone. This suggests additional sources of error that are not incorporated in the standard afterglow theory. For the first time, we provide a measurement of this intrinsic error which can be represented as an error in the estimate of $p$ of magnitude $0.25 \pm 0.04$. When this error is included in the fits, the number of LGRBs with an identified environment drops substantially, but the equal division between the two types remains.
astro-ph.HE
we analyze the properties of a sample of long gammaray bursts lgrbs detected by the fermi satellite that have a spectroscopic redshift and good followup coverage at both xray and opticalnir wavelengths the evolution of lgrb afterglows depends on the density profile of the external medium enabling us to separate wind or ismlike environments based on the observations we do this by identifying the environment that provides the best agreement between estimates of p the index of the underlying powerlaw distribution of electron energies as determined by the behavior of the afterglow in different spectraltemporal regimes at 11 restframe hours after trigger we find a roughly even split between ismlike and windlike environments we further find a 2sigma separation in the prompt emission energy distributions of windlike and ismlike bursts we investigate the underlying physical parameters of the shock and calculate the degenerate product of density and magnetic field energy epsilon_b we show that epsilon_b must be ll 102 to avoid implied densities comparable to the intergalactic medium finally we find that the most precisely constrained observations disagree on p by more than would be expected based on observational errors alone this suggests additional sources of error that are not incorporated in the standard afterglow theory for the first time we provide a measurement of this intrinsic error which can be represented as an error in the estimate of p of magnitude 025 pm 004 when this error is included in the fits the number of lgrbs with an identified environment drops substantially but the equal division between the two types remains
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1,802.07731
Modal Decomposition of TTV - Inferring Planet Masses and Eccentricities
Transit timing variations (TTVs) are a powerful tool for characterizing the properties of transiting exoplanets. However, inferring planet properties from the observed timing variations is a challenging task, which is usually addressed by extensive numerical searches. We propose a new, computationally inexpensive method for inverting TTV signals in a planetary system of two transiting planets. To the lowest order in planetary masses and eccentricities, TTVs can be expressed as a linear combination of 3 functions, which we call the \textit{TTV modes}. These functions depend only on the planets' linear ephemerides, and can be either constructed analytically, or by performing 3 orbital integrations of the three-body system. Given a TTV signal, the underlying physical parameters are found by decomposing the data as a sum of the TTV modes. We demonstrate the use of this method by inferring the mass and eccentricity of 6 \textit{Kepler} planets that were previously characterized in other studies. Finally we discuss the implications and future prospects of our new method.
astro-ph.EP
transit timing variations ttvs are a powerful tool for characterizing the properties of transiting exoplanets however inferring planet properties from the observed timing variations is a challenging task which is usually addressed by extensive numerical searches we propose a new computationally inexpensive method for inverting ttv signals in a planetary system of two transiting planets to the lowest order in planetary masses and eccentricities ttvs can be expressed as a linear combination of 3 functions which we call the textitttv modes these functions depend only on the planets linear ephemerides and can be either constructed analytically or by performing 3 orbital integrations of the threebody system given a ttv signal the underlying physical parameters are found by decomposing the data as a sum of the ttv modes we demonstrate the use of this method by inferring the mass and eccentricity of 6 textitkepler planets that were previously characterized in other studies finally we discuss the implications and future prospects of our new method
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1,802.07732
Is the macronova in GW170817 powered by the central engine?
The gravitational wave event GW170817 from a binary neutron star (NS) merger is accompanied by electromagnetic counterparts, and the optical and near-infared emission is called a macronova (or kilonova). Although the radioactivity of synthesized r-process elements is widely discussed as an energy source, its decisive evidence is not clearly shown yet. We discuss a macronova powered by the central engine activities such as jet activities and X-rays from the matter fallback, and show that the engine model allows much broader parameter spaces, in particular smaller ejecta mass ($\sim10^{-4}-0.01\,\Msun$) than the r-process model. The blue and red macronovae are naturally explained by various combinations of the ejecta such as a cocoon and merger ejecta with the energy sources of jets and X-rays. The required energy injection is very similar to the X-ray excess observed in GRB 130603B with the power-law slope of $\sim-1.3$. The required lanthanoid fraction for the opacity can be also consistent with the Galactic one. Early or late multi-wavelength observations are crucial for revealing the central engine of short gamma-ray bursts and the r-process nucleosynthesis.
astro-ph.HE
the gravitational wave event gw170817 from a binary neutron star ns merger is accompanied by electromagnetic counterparts and the optical and nearinfared emission is called a macronova or kilonova although the radioactivity of synthesized rprocess elements is widely discussed as an energy source its decisive evidence is not clearly shown yet we discuss a macronova powered by the central engine activities such as jet activities and xrays from the matter fallback and show that the engine model allows much broader parameter spaces in particular smaller ejecta mass sim104001msun than the rprocess model the blue and red macronovae are naturally explained by various combinations of the ejecta such as a cocoon and merger ejecta with the energy sources of jets and xrays the required energy injection is very similar to the xray excess observed in grb 130603b with the powerlaw slope of sim13 the required lanthanoid fraction for the opacity can be also consistent with the galactic one early or late multiwavelength observations are crucial for revealing the central engine of short gammaray bursts and the rprocess nucleosynthesis
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1,802.07733
Magnetotransport in multi-Weyl semimetals: A kinetic theory approach
We study the longitudinal magnetotransport in three-dimensional multi-Weyl semimetals, constituted by a pair of (anti)-monopole of arbitrary integer charge ($n$), with $n=1,2$ and $3$ in a crystalline environment. For any $n>1$, even though the distribution of the underlying Berry curvature is anisotropic, the corresponding intrinsic component of the longitudinal magnetoconductivity (LMC), bearing the signature of the chiral anomaly, is insensitive to the direction of the external magnetic field ($B$) and increases as $B^2$, at least when it is sufficiently weak (the semi-classical regime). In addition, the LMC scales as $n^3$ with the monopole charge. We demonstrate these outcomes for two distinct scenarios, namely when inter-particle collisions in the Weyl medium are effectively described by (a) a single and (b) two (corresponding to inter- and intra-valley) scattering times. While in the former situation the contribution to LMC from chiral anomaly is inseparable from the non-anomalous ones, these two contributions are characterized by different time scales in the later construction. Specifically for sufficiently large inter-valley scattering time the LMC is dominated by the anomalous contribution, arising from the chiral anomaly. The predicted scaling of LMC and the signature of chiral anomaly can be observed in recently proposed candidate materials, accommodating multi-Weyl semimetals in various solid state compounds.
cond-mat.mes-hall hep-th
we study the longitudinal magnetotransport in threedimensional multiweyl semimetals constituted by a pair of antimonopole of arbitrary integer charge n with n12 and 3 in a crystalline environment for any n1 even though the distribution of the underlying berry curvature is anisotropic the corresponding intrinsic component of the longitudinal magnetoconductivity lmc bearing the signature of the chiral anomaly is insensitive to the direction of the external magnetic field b and increases as b2 at least when it is sufficiently weak the semiclassical regime in addition the lmc scales as n3 with the monopole charge we demonstrate these outcomes for two distinct scenarios namely when interparticle collisions in the weyl medium are effectively described by a a single and b two corresponding to inter and intravalley scattering times while in the former situation the contribution to lmc from chiral anomaly is inseparable from the nonanomalous ones these two contributions are characterized by different time scales in the later construction specifically for sufficiently large intervalley scattering time the lmc is dominated by the anomalous contribution arising from the chiral anomaly the predicted scaling of lmc and the signature of chiral anomaly can be observed in recently proposed candidate materials accommodating multiweyl semimetals in various solid state compounds
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1,802.07734
Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. I. Spatially Resolved Mass Outflow Rates for the Seyfert 2 Galaxy Markarian 573
We present the first spatially resolved mass outflow rate measurements ($\dot M_{out}$) of the optical emission line gas in the narrow line region (NLR) of a Seyfert 2 galaxy, Markarian 573. Using long slit spectra and [O III] imaging from the Hubble Space Telescope and Apache Point Observatory in conjunction with emission line diagnostics and Cloudy photoionization models, we find a peak outflow rate of $\dot M_{out} \approx$ 3.4 $\pm$ 0.5 $M_{\odot}$ yr$^{-1}$ at a distance of 210 pc from the central supermassive black hole (SMBH). The outflow extends to distances of 600 pc from the nucleus with a total mass and kinetic energy of $M \approx 2.2 \times 10^6 M_{\odot}$ and $E \approx 5.1 \times 10^{54}$ erg, revealing the outflows to be more energetic than those in the lower luminosity Seyfert 1 galaxy NGC 4151 (Crenshaw et al. 2015). The peak outflow rate is an order of magnitude larger than the mass accretion and nuclear outflow rates, indicating local in-situ acceleration of the circumnuclear NLR gas. We compare these results to global techniques that quantify an average outflow rate across the NLR, and find the latter are subject to larger uncertainties. These results indicate that spatially resolved observations are critical for probing AGN feedback on scales where circumnuclear star formation occurs.
astro-ph.GA
we present the first spatially resolved mass outflow rate measurements dot m_out of the optical emission line gas in the narrow line region nlr of a seyfert 2 galaxy markarian 573 using long slit spectra and o iii imaging from the hubble space telescope and apache point observatory in conjunction with emission line diagnostics and cloudy photoionization models we find a peak outflow rate of dot m_out approx 34 pm 05 m_odot yr1 at a distance of 210 pc from the central supermassive black hole smbh the outflow extends to distances of 600 pc from the nucleus with a total mass and kinetic energy of m approx 22 times 106 m_odot and e approx 51 times 1054 erg revealing the outflows to be more energetic than those in the lower luminosity seyfert 1 galaxy ngc 4151 crenshaw et al 2015 the peak outflow rate is an order of magnitude larger than the mass accretion and nuclear outflow rates indicating local insitu acceleration of the circumnuclear nlr gas we compare these results to global techniques that quantify an average outflow rate across the nlr and find the latter are subject to larger uncertainties these results indicate that spatially resolved observations are critical for probing agn feedback on scales where circumnuclear star formation occurs
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1,802.07735
Characterization of echoes: A Dyson-series representation of individual pulses
The ability to detect and scrutinize gravitational waves from the merger and coalescence of compact binaries opens up the possibility to perform tests of fundamental physics. One such test concerns the dark, nature of compact objects: are they really black holes? It was recently pointed out that the absence of horizons -- while keeping the external geometry very close to that of General Relativity -- would manifest itself in a series of echoes in gravitational wave signals. The observation of echoes by LIGO/Virgo or upcoming facilities would likely inform us on quantum gravity effects or unseen types of matter. Detection of such signals is in principle feasible with relatively simple tools, but would benefit enormously from accurate templates. Here we analytically individualize each echo waveform and show that it can be written as a Dyson series, for arbitrary effective potential and boundary conditions. We further apply the formalism to explicitly determine the echoes of a simple toy model: the Dirac delta potential. Our results allow to read off a few known features of echoes and may find application in the modelling for data analysis.
gr-qc hep-th
the ability to detect and scrutinize gravitational waves from the merger and coalescence of compact binaries opens up the possibility to perform tests of fundamental physics one such test concerns the dark nature of compact objects are they really black holes it was recently pointed out that the absence of horizons while keeping the external geometry very close to that of general relativity would manifest itself in a series of echoes in gravitational wave signals the observation of echoes by ligovirgo or upcoming facilities would likely inform us on quantum gravity effects or unseen types of matter detection of such signals is in principle feasible with relatively simple tools but would benefit enormously from accurate templates here we analytically individualize each echo waveform and show that it can be written as a dyson series for arbitrary effective potential and boundary conditions we further apply the formalism to explicitly determine the echoes of a simple toy model the dirac delta potential our results allow to read off a few known features of echoes and may find application in the modelling for data analysis
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1,802.07736
Quantum field theory of nematic transitions in spin orbit coupled spin-1 polar bosons
We theoretically study an ultra-cold gas of spin-1 polar bosons in a one dimensional continuum which are subject to linear and quadratic Zeeman fields and a Raman induced spin-orbit coupling. Concentrating on the regime in which the background fields can be treated perturbatively we analytically solve the model in its low-energy sector, i.e. we characterize the relevant phases and the quantum phase transitions between them. Depending on the sign of the effective quadratic Zeeman field $\epsilon$, two superfluid phases with distinct nematic order appear. In addition, we uncover a spin-disordered superfluid phase at strong coupling. We employ a combination of renormalization group calculations and duality transformations to access the nature of the phase transitions. At $\epsilon = 0$, a line of spin-charge separated pairs of Luttinger liquids divides the two nematic phases and the transition to the spin disordered state at strong coupling is of the Berezinskii-Kosterlitz-Thouless type. In contrast, at $\epsilon \neq 0$, the quantum critical theory separating nematic and strong coupling spin disordered phases contains a Luttinger liquid in the charge sector that is coupled to a Majorana fermion in the spin sector (i.e. the critical theory at finite $\epsilon$ maps to a quantum critical Ising model that is coupled to the charge Luttinger liquid). Due to an emergent Lorentz symmetry, both have the same, logarithmically diverging velocity. We discuss the experimental signatures of our findings that are relevant to ongoing experiments in ultra-cold atomic gases of $^{23}$Na.
cond-mat.quant-gas cond-mat.str-el
we theoretically study an ultracold gas of spin1 polar bosons in a one dimensional continuum which are subject to linear and quadratic zeeman fields and a raman induced spinorbit coupling concentrating on the regime in which the background fields can be treated perturbatively we analytically solve the model in its lowenergy sector ie we characterize the relevant phases and the quantum phase transitions between them depending on the sign of the effective quadratic zeeman field epsilon two superfluid phases with distinct nematic order appear in addition we uncover a spindisordered superfluid phase at strong coupling we employ a combination of renormalization group calculations and duality transformations to access the nature of the phase transitions at epsilon 0 a line of spincharge separated pairs of luttinger liquids divides the two nematic phases and the transition to the spin disordered state at strong coupling is of the berezinskiikosterlitzthouless type in contrast at epsilon neq 0 the quantum critical theory separating nematic and strong coupling spin disordered phases contains a luttinger liquid in the charge sector that is coupled to a majorana fermion in the spin sector ie the critical theory at finite epsilon maps to a quantum critical ising model that is coupled to the charge luttinger liquid due to an emergent lorentz symmetry both have the same logarithmically diverging velocity we discuss the experimental signatures of our findings that are relevant to ongoing experiments in ultracold atomic gases of 23na
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1,802.07737
Detection significance of Baryon Acoustic Oscillations peaks in galaxy and quasar clustering
We compare our analysis of the Baryon Acoustic Oscillations (BAO) feature in the correlation functions of SDSS BOSS DR12 LOWZ and CMASS galaxy samples with the findings of arXiv:1509.06371v2. Using subsets of the data we obtain an empirical estimate of the errors on the correlation functions which are in agreement with the simulated errors of arXiv:1509.06371v2. We find that the significance of BAO detection is the quantity most sensitive to the choice of the fitting range with the CMASS value decreasing from $8.0\sigma$ to $5.3\sigma$ as the fitting range is reduced. Although our measurements of $D_V(z)$ are in agreement with those of arXiv:1509.06371v2, we note that their CMASS $8.0\sigma$ (LOWZ $4.0\sigma$) detection significance reduces to $4.7\sigma$ ($2.8\sigma$) in fits with their diagonal covariance terms only. We extend our BAO analysis to higher redshifts by fitting to the weighted mean of 2QDESp, SDSS DR5 UNIFORM, 2QZ and 2SLAQ quasar correlation functions, obtaining a $7.6\%$ measurement compared to $3.9\%$ achieved by eBOSS DR14. Unlike for the LRG surveys, the larger error on quasar correlation functions implies a smaller role for nuisance parameters (accounting for scale-dependent clustering) in providing a good fit to the fiducial $\Lambda$CDM model. Again using only the error bars of arXiv:1705.06373v2 and ignoring any off-diagonal covariance matrix terms, we find that the eBOSS peak significance reduces from 2.8 to $1.4\sigma$. We conclude that for both LRGs and quasars, the reported BAO peak significances from the SDSS surveys depend sensitively on the accuracy of the covariance matrix at large separations.
astro-ph.CO
we compare our analysis of the baryon acoustic oscillations bao feature in the correlation functions of sdss boss dr12 lowz and cmass galaxy samples with the findings of arxiv150906371v2 using subsets of the data we obtain an empirical estimate of the errors on the correlation functions which are in agreement with the simulated errors of arxiv150906371v2 we find that the significance of bao detection is the quantity most sensitive to the choice of the fitting range with the cmass value decreasing from 80sigma to 53sigma as the fitting range is reduced although our measurements of d_vz are in agreement with those of arxiv150906371v2 we note that their cmass 80sigma lowz 40sigma detection significance reduces to 47sigma 28sigma in fits with their diagonal covariance terms only we extend our bao analysis to higher redshifts by fitting to the weighted mean of 2qdesp sdss dr5 uniform 2qz and 2slaq quasar correlation functions obtaining a 76 measurement compared to 39 achieved by eboss dr14 unlike for the lrg surveys the larger error on quasar correlation functions implies a smaller role for nuisance parameters accounting for scaledependent clustering in providing a good fit to the fiducial lambdacdm model again using only the error bars of arxiv170506373v2 and ignoring any offdiagonal covariance matrix terms we find that the eboss peak significance reduces from 28 to 14sigma we conclude that for both lrgs and quasars the reported bao peak significances from the sdss surveys depend sensitively on the accuracy of the covariance matrix at large separations
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1,802.07738
The Impact of Microlensing on the Standardisation of Strongly Lensed Type Ia Supernovae
We investigate the effect of microlensing on the standardisation of strongly lensed Type Ia supernovae (GLSNe Ia). We present predictions for the amount of scatter induced by microlensing across a range of plausible strong lens macromodels. We find that lensed images in regions of low convergence, shear and stellar density are standardisable, where the microlensing scatter is < 0.15 magnitudes, comparable to the intrinsic dispersion of for a typical SN Ia. These standardisable configurations correspond to asymmetric lenses with an image located far outside the Einstein radius of the lens. Symmetric and small Einstein radius lenses (< 0.5 arcsec) are not standardisable. We apply our model to the recently discovered GLSN Ia iPTF16geu and find that the large discrepancy between the observed flux and the macromodel predictions from More et al. (2017) cannot be explained by microlensing alone. Using the mock GLSNe Ia catalogue of Goldstein et al. (2017), we predict that ~ 22% of GLSNe Ia discovered by LSST will be standardisable, with a median Einstein radius of 0.9 arcseconds and a median time-delay of 41 days. By breaking the mass-sheet degeneracy the full LSST GLSNe Ia sample will be able to detect systematics in H0 at the 0.5% level.
astro-ph.CO astro-ph.GA
we investigate the effect of microlensing on the standardisation of strongly lensed type ia supernovae glsne ia we present predictions for the amount of scatter induced by microlensing across a range of plausible strong lens macromodels we find that lensed images in regions of low convergence shear and stellar density are standardisable where the microlensing scatter is 015 magnitudes comparable to the intrinsic dispersion of for a typical sn ia these standardisable configurations correspond to asymmetric lenses with an image located far outside the einstein radius of the lens symmetric and small einstein radius lenses 05 arcsec are not standardisable we apply our model to the recently discovered glsn ia iptf16geu and find that the large discrepancy between the observed flux and the macromodel predictions from more et al 2017 cannot be explained by microlensing alone using the mock glsne ia catalogue of goldstein et al 2017 we predict that 22 of glsne ia discovered by lsst will be standardisable with a median einstein radius of 09 arcseconds and a median timedelay of 41 days by breaking the masssheet degeneracy the full lsst glsne ia sample will be able to detect systematics in h0 at the 05 level
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1,802.07739
Supersymmetric Flaxion
Recently, a new minimal extension of the Standard Model has been proposed, where a spontaneously broken, flavor-dependent global U(1) symmetry is introduced. It not only explains the hierarchical flavor structure in the quark and lepton sector, but also solves the strong CP problem by identifying the Nambu-Goldstone boson as the QCD axion, which we call flaxion. In this work, we consider supersymmetric extensions of the flaxion scenario. We study the CP and flavor violations due to supersymmetric particles, the effects of R-parity violations, the cosmological gravitino and axino problems, and the cosmological evolution of the scalar partner of the flaxion, sflaxion. We also propose an attractor-like inflationary model where the flaxion multiplet contains the inflaton field, and show that a consistent cosmological scenario can be obtained, including inflation, leptogenesis, and dark matter.
hep-ph
recently a new minimal extension of the standard model has been proposed where a spontaneously broken flavordependent global u1 symmetry is introduced it not only explains the hierarchical flavor structure in the quark and lepton sector but also solves the strong cp problem by identifying the nambugoldstone boson as the qcd axion which we call flaxion in this work we consider supersymmetric extensions of the flaxion scenario we study the cp and flavor violations due to supersymmetric particles the effects of rparity violations the cosmological gravitino and axino problems and the cosmological evolution of the scalar partner of the flaxion sflaxion we also propose an attractorlike inflationary model where the flaxion multiplet contains the inflaton field and show that a consistent cosmological scenario can be obtained including inflation leptogenesis and dark matter
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1,802.0774
Machine Theory of Mind
Theory of mind (ToM; Premack & Woodruff, 1978) broadly refers to humans' ability to represent the mental states of others, including their desires, beliefs, and intentions. We propose to train a machine to build such models too. We design a Theory of Mind neural network -- a ToMnet -- which uses meta-learning to build models of the agents it encounters, from observations of their behaviour alone. Through this process, it acquires a strong prior model for agents' behaviour, as well as the ability to bootstrap to richer predictions about agents' characteristics and mental states using only a small number of behavioural observations. We apply the ToMnet to agents behaving in simple gridworld environments, showing that it learns to model random, algorithmic, and deep reinforcement learning agents from varied populations, and that it passes classic ToM tasks such as the "Sally-Anne" test (Wimmer & Perner, 1983; Baron-Cohen et al., 1985) of recognising that others can hold false beliefs about the world. We argue that this system -- which autonomously learns how to model other agents in its world -- is an important step forward for developing multi-agent AI systems, for building intermediating technology for machine-human interaction, and for advancing the progress on interpretable AI.
cs.AI
theory of mind tom premack woodruff 1978 broadly refers to humans ability to represent the mental states of others including their desires beliefs and intentions we propose to train a machine to build such models too we design a theory of mind neural network a tomnet which uses metalearning to build models of the agents it encounters from observations of their behaviour alone through this process it acquires a strong prior model for agents behaviour as well as the ability to bootstrap to richer predictions about agents characteristics and mental states using only a small number of behavioural observations we apply the tomnet to agents behaving in simple gridworld environments showing that it learns to model random algorithmic and deep reinforcement learning agents from varied populations and that it passes classic tom tasks such as the sallyanne test wimmer perner 1983 baroncohen et al 1985 of recognising that others can hold false beliefs about the world we argue that this system which autonomously learns how to model other agents in its world is an important step forward for developing multiagent ai systems for building intermediating technology for machinehuman interaction and for advancing the progress on interpretable ai
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1,802.07741
Extended Reduced-Form Framework for Non-Life Insurance
In this paper we propose a general framework for modeling an insurance liability cash flow in continuous time, by generalizing the reduced-form framework for credit risk and life insurance. In particular, we assume a nontrivial dependence structure between the reference filtration and the insurance internal filtration. We apply these results for pricing and hedging non-life insurance liabilities in hybrid financial and insurance markets, while taking into account the role of inflation under the benchmarked risk-minimization approach. This framework offers at the same time a general and flexible structure, and an explicit and treatable pricing-hedging formula.
q-fin.MF
in this paper we propose a general framework for modeling an insurance liability cash flow in continuous time by generalizing the reducedform framework for credit risk and life insurance in particular we assume a nontrivial dependence structure between the reference filtration and the insurance internal filtration we apply these results for pricing and hedging nonlife insurance liabilities in hybrid financial and insurance markets while taking into account the role of inflation under the benchmarked riskminimization approach this framework offers at the same time a general and flexible structure and an explicit and treatable pricinghedging formula
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1,802.07742
A matrix model for the latitude Wilson loop in ABJM theory
In ABJ(M) theory, we propose a matrix model for the exact evaluation of BPS Wilson loops on a latitude circular contour, so providing a new weak-strong interpolation tool. Intriguingly, the matrix model turns out to be a particular case of that computing torus knot invariants in $U(N_1|N_2)$ Chern-Simons theory. At weak coupling we check our proposal against a three-loop computation, performed for generic framing, winding number and representation. The matrix model is amenable of a Fermi gas formulation, which we use to systematically compute the strong coupling and genus expansions. For the fermionic Wilson loop the leading planar behavior agrees with a previous string theory prediction. For the bosonic operator our result provides a clue for finding the corresponding string dual configuration. Our matrix model is consistent with recent proposals for computing Bremsstrahlung functions exactly in terms of latitude Wilson loops. As a by-product, we extend the conjecture for the exact $B^{\theta}_{1/6}$ Bremsstrahlung function to generic representations and test it with a four-loop perturbative computation. Finally, we propose an exact prediction for $B_{1/2}$ at unequal gauge group ranks.
hep-th
in abjm theory we propose a matrix model for the exact evaluation of bps wilson loops on a latitude circular contour so providing a new weakstrong interpolation tool intriguingly the matrix model turns out to be a particular case of that computing torus knot invariants in un_1n_2 chernsimons theory at weak coupling we check our proposal against a threeloop computation performed for generic framing winding number and representation the matrix model is amenable of a fermi gas formulation which we use to systematically compute the strong coupling and genus expansions for the fermionic wilson loop the leading planar behavior agrees with a previous string theory prediction for the bosonic operator our result provides a clue for finding the corresponding string dual configuration our matrix model is consistent with recent proposals for computing bremsstrahlung functions exactly in terms of latitude wilson loops as a byproduct we extend the conjecture for the exact btheta_16 bremsstrahlung function to generic representations and test it with a fourloop perturbative computation finally we propose an exact prediction for b_12 at unequal gauge group ranks
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1,802.07743
Broad absorption line symbiotic stars: highly ionized species in the fast outflow from MWC 560
In symbiotic binaries, jets and disk winds may be integral to the physics of accretion onto white dwarfs from cool giants. The persistent outflow from symbiotic star MWC 560 (=V694 Mon) is known to manifest as broad absorption lines (BALs), most prominently at the Balmer transitions. We report the detection of high-ionization BALs from C IV, Si IV, N V, and He II in International Ultraviolet Explorer spectra obtained on 1990 April 29-30, when an optical outburst temporarily erased the obscuring 'iron curtain' of absorption troughs from Fe II and similar ions. The C IV and Si IV BALs reached maximum radial velocities at least 1000 km/s higher than contemporaneous Mg II and He II BALs; the same behaviors occur in the winds of quasars and cataclysmic variables. An iron curtain lifts to unveil high-ionization BALs during the P Cygni phase observed in some novae, suggesting by analogy a temporary switch in MWC 560 from persistent outflow to discrete mass ejection. At least three more symbiotic stars exhibit broad absorption with blue edges faster than 1500 km/s; high-ionization BALs have been reported in AS 304 (=V4018 Sgr), while transient Balmer BALs have been reported in Z And and CH Cyg. These BAL-producing fast outflows can have wider opening angles than has been previously supposed. BAL symbiotics are short-timescale laboratories for their giga-scale analogs, broad absorption line quasars (BALQSOs), which display a similarly wide range of ionization states in their winds.
astro-ph.HE astro-ph.GA astro-ph.SR
in symbiotic binaries jets and disk winds may be integral to the physics of accretion onto white dwarfs from cool giants the persistent outflow from symbiotic star mwc 560 v694 mon is known to manifest as broad absorption lines bals most prominently at the balmer transitions we report the detection of highionization bals from c iv si iv n v and he ii in international ultraviolet explorer spectra obtained on 1990 april 2930 when an optical outburst temporarily erased the obscuring iron curtain of absorption troughs from fe ii and similar ions the c iv and si iv bals reached maximum radial velocities at least 1000 kms higher than contemporaneous mg ii and he ii bals the same behaviors occur in the winds of quasars and cataclysmic variables an iron curtain lifts to unveil highionization bals during the p cygni phase observed in some novae suggesting by analogy a temporary switch in mwc 560 from persistent outflow to discrete mass ejection at least three more symbiotic stars exhibit broad absorption with blue edges faster than 1500 kms highionization bals have been reported in as 304 v4018 sgr while transient balmer bals have been reported in z and and ch cyg these balproducing fast outflows can have wider opening angles than has been previously supposed bal symbiotics are shorttimescale laboratories for their gigascale analogs broad absorption line quasars balqsos which display a similarly wide range of ionization states in their winds
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1,802.07744
Contextuality bounds the efficiency of classical simulation of quantum processes
Contextuality has been conjectured to be a super-classical resource for quantum computation, analogous to the role of non-locality as a super-classical resource for communication. We show that the presence of contextuality places a lower bound on the amount of classical memory required to simulate any quantum sub-theory, thereby establishing a quantitative connection between contextuality and classical simulability. We apply our result to the qubit stabilizer sub-theory, where the presence of state-independent contextuality has been an obstacle in establishing contextuality as a quantum computational resource. We find that the presence of contextuality in this sub-theory demands that the minimum number of classical bits of memory required to simulate a multi-qubit system must scale quadratically in the number of qubits; notably, this is the same scaling as the Gottesman-Knill algorithm. We contrast this result with the (non-contextual) qudit case, where linear scaling is possible.
quant-ph
contextuality has been conjectured to be a superclassical resource for quantum computation analogous to the role of nonlocality as a superclassical resource for communication we show that the presence of contextuality places a lower bound on the amount of classical memory required to simulate any quantum subtheory thereby establishing a quantitative connection between contextuality and classical simulability we apply our result to the qubit stabilizer subtheory where the presence of stateindependent contextuality has been an obstacle in establishing contextuality as a quantum computational resource we find that the presence of contextuality in this subtheory demands that the minimum number of classical bits of memory required to simulate a multiqubit system must scale quadratically in the number of qubits notably this is the same scaling as the gottesmanknill algorithm we contrast this result with the noncontextual qudit case where linear scaling is possible
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1,802.07745
Diversity in the stellar velocity dispersion profiles of a large sample of Brightest Cluster Galaxies $z\leq0.3$
We analyse spatially-resolved deep optical spectroscopy of Brightest Cluster Galaxies (BCGs) located in 32 massive clusters with redshifts of 0.05 $\leq z \leq$ 0.30, to investigate their velocity dispersion profiles. We compare these measurements to those of other massive early-type galaxies, as well as central group galaxies, where relevant. This unique, large sample extends to the most extreme of massive galaxies, spanning M$_{K}$ between -25.7 to -27.8 mag, and host cluster halo mass M$_{500}$ up to 1.7 $\times$ 10$^{15}$ M$_{\odot}$. To compare the kinematic properties between brightest group and cluster members, we analyse similar spatially-resolved long-slit spectroscopy for 23 nearby Brightest Group Galaxies (BGGs) from the Complete Local-Volume Groups Sample (CLoGS). We find a surprisingly large variety in velocity dispersion slopes for BCGs, with a significantly larger fraction of positive slopes, unique compared to other (non-central) early-type galaxies as well as the majority of the brightest members of the groups. We find that the velocity dispersion slopes of the BCGs and BGGs correlate with the luminosity of the galaxies, and we quantify this correlation. It is not clear whether the full diversity in velocity dispersion slopes that we see is reproduced in simulations.
astro-ph.GA
we analyse spatiallyresolved deep optical spectroscopy of brightest cluster galaxies bcgs located in 32 massive clusters with redshifts of 005 leq z leq 030 to investigate their velocity dispersion profiles we compare these measurements to those of other massive earlytype galaxies as well as central group galaxies where relevant this unique large sample extends to the most extreme of massive galaxies spanning m_k between 257 to 278 mag and host cluster halo mass m_500 up to 17 times 1015 m_odot to compare the kinematic properties between brightest group and cluster members we analyse similar spatiallyresolved longslit spectroscopy for 23 nearby brightest group galaxies bggs from the complete localvolume groups sample clogs we find a surprisingly large variety in velocity dispersion slopes for bcgs with a significantly larger fraction of positive slopes unique compared to other noncentral earlytype galaxies as well as the majority of the brightest members of the groups we find that the velocity dispersion slopes of the bcgs and bggs correlate with the luminosity of the galaxies and we quantify this correlation it is not clear whether the full diversity in velocity dispersion slopes that we see is reproduced in simulations
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1,802.07746
Holographic dual to charged SYK from 3D Gravity and Chern-Simons
In this paper, we obtain a bulk dual to SYK model, including SYK model with $U(1)$ charge, by Kaluza-Klein (KK) reduction from three dimensions. We show that KK reduction of the 3D Einstein action plus its boundary term gives the Jackiw-Teitelboim (JT) model in 2D with the appropriate 1D boundary term. The size of the KK radius gets identified with the value of the dilaton in the resulting near-AdS$_2$ geometry. In presence of U(1) charge, the 3D model additionally includes a $U(1)$ Chern-Simons (CS) action. In order to describe a boundary theory with non-zero chemical potential, we also introduce a coupling between CS gauge field and bulk gravity. The 3D CS action plus the new coupling term with appropriate boundary terms reduce in two dimensions to a BF-type action plus a source term and boundary terms. The KK reduced 2D theory represents the soft sector of the charged SYK model. The pseudo-Nambu-Goldstone modes of combined $\textit{Diff} /\mathbb{SL}(2,\mathbb{R})$ and $U(1)_{\rm local}/U(1)$ transformations are represented by combined large diffeomorphisms and large gauge transformations. The effective action of the former is reproduced by the action cost of the latter in the bulk dual, after appropriate identification of parameters. We compute chaotic correlators from the bulk and reproduce the result that the contribution from the "boundary photons" corresponds to zero Liapunov exponent.
hep-th cond-mat.stat-mech nlin.CD
in this paper we obtain a bulk dual to syk model including syk model with u1 charge by kaluzaklein kk reduction from three dimensions we show that kk reduction of the 3d einstein action plus its boundary term gives the jackiwteitelboim jt model in 2d with the appropriate 1d boundary term the size of the kk radius gets identified with the value of the dilaton in the resulting nearads_2 geometry in presence of u1 charge the 3d model additionally includes a u1 chernsimons cs action in order to describe a boundary theory with nonzero chemical potential we also introduce a coupling between cs gauge field and bulk gravity the 3d cs action plus the new coupling term with appropriate boundary terms reduce in two dimensions to a bftype action plus a source term and boundary terms the kk reduced 2d theory represents the soft sector of the charged syk model the pseudonambugoldstone modes of combined textitdiff mathbbsl2mathbbr and u1_rm localu1 transformations are represented by combined large diffeomorphisms and large gauge transformations the effective action of the former is reproduced by the action cost of the latter in the bulk dual after appropriate identification of parameters we compute chaotic correlators from the bulk and reproduce the result that the contribution from the boundary photons corresponds to zero liapunov exponent
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1,802.07747
Higher-form symmetries and spontaneous symmetry breaking
We study various aspects of spontaneous symmetry breaking in theories that possess higher-form symmetries, which are symmetries whose charged objects have a dimension $p>0$. We first sketch a proof of a higher version of Goldstone's theorem, and then discuss how boundary conditions and gauge-fixing issues are dealt with in theories with spontaneously broken higher symmetries, focusing in particular on $p$-form $U(1)$ gauge theories. We then elaborate on a generalization of the Coleman-Mermin-Wagner theorem for higher-form symmetries, namely that in spacetime dimension $D$, continuous $p$-form symmetries can never be spontaneously broken if $p\geq D-2$. We also make a few comments on relations between higher symmetries and asymptotic symmetries in Abelian gauge theory.
hep-th cond-mat.str-el
we study various aspects of spontaneous symmetry breaking in theories that possess higherform symmetries which are symmetries whose charged objects have a dimension p0 we first sketch a proof of a higher version of goldstones theorem and then discuss how boundary conditions and gaugefixing issues are dealt with in theories with spontaneously broken higher symmetries focusing in particular on pform u1 gauge theories we then elaborate on a generalization of the colemanmerminwagner theorem for higherform symmetries namely that in spacetime dimension d continuous pform symmetries can never be spontaneously broken if pgeq d2 we also make a few comments on relations between higher symmetries and asymptotic symmetries in abelian gauge theory
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1,802.07748
On the Rates of Steady, Quasi-steady and Impulsive Magnetic Reconnection
Magnetic reconnection (MR) is considered as a major source of particle energization in astrophysical plasma. In the past, analysis of MR often assumes the magnetostatic condition, i.e. $\partial_t = 0$. We show that under the Sweet-Parker-Petschek framework, steady state is an over-constraint and is not achievable. On the other hand, the quasi-steady state defined as $\partial_t \mathbf{E} = 0$ but $\partial_t \mathbf{B} \neq 0$ or equivalently $\partial_t\mathbf{j}\neq 0$ better describes the asymptotic behaviour of MR without turbulence. The upper limit of MR rate for quasi-steady MR is found to be $\sim 1/3\sqrt{3} \sim 0.19$. The limit does not apply to impulsive or turbulent MR of which $\partial_t\mathbf{B} \neq 0$ and $\partial_t\mathbf{E} \neq 0$. In impulsive MR the rate can be higher or lower than 0.19 depending on the state of the turbulence. Our results may explain the apparent discrepancy in observations of solar flare MR rates. The analysis is independent of mass ratio and thus the results are applicable to pair plasma.
physics.space-ph astro-ph.EP astro-ph.HE astro-ph.SR physics.plasm-ph
magnetic reconnection mr is considered as a major source of particle energization in astrophysical plasma in the past analysis of mr often assumes the magnetostatic condition ie partial_t 0 we show that under the sweetparkerpetschek framework steady state is an overconstraint and is not achievable on the other hand the quasisteady state defined as partial_t mathbfe 0 but partial_t mathbfb neq 0 or equivalently partial_tmathbfjneq 0 better describes the asymptotic behaviour of mr without turbulence the upper limit of mr rate for quasisteady mr is found to be sim 13sqrt3 sim 019 the limit does not apply to impulsive or turbulent mr of which partial_tmathbfb neq 0 and partial_tmathbfe neq 0 in impulsive mr the rate can be higher or lower than 019 depending on the state of the turbulence our results may explain the apparent discrepancy in observations of solar flare mr rates the analysis is independent of mass ratio and thus the results are applicable to pair plasma
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1,802.07749
Radiative transfer calculations of the diffuse ionised gas in disc galaxies with cosmic ray feedback
The large vertical scale heights of the diffuse ionised gas (DIG) in disc galaxies are challenging to model, as hydrodynamical models including only thermal feedback seem to be unable to support gas at these heights. In this paper, we use a three dimensional Monte Carlo radiation transfer code to post-process disc simulations of the Simulating the Life-Cycle of Molecular Clouds (SILCC) project that include feedback by cosmic rays. We show that the more extended discs in simulations including cosmic ray feedback naturally lead to larger scale heights for the DIG which are more in line with observed scale heights. We also show that including a fiducial cosmic ray heating term in our model can help to increase the temperature as a function of disc scale height, but fails to reproduce observed DIG nitrogen and sulphur forbidden line intensities. We show that, to reproduce these line emissions, we require a heating mechanism that affects gas over a larger density range than is achieved by cosmic ray heating, which can be achieved by fine tuning the total luminosity of ionising sources to get an appropriate ionising spectrum as a function of scale height. This result sheds a new light on the relation between forbidden line emissions and temperature profiles for realistic DIG gas distributions.
astro-ph.GA
the large vertical scale heights of the diffuse ionised gas dig in disc galaxies are challenging to model as hydrodynamical models including only thermal feedback seem to be unable to support gas at these heights in this paper we use a three dimensional monte carlo radiation transfer code to postprocess disc simulations of the simulating the lifecycle of molecular clouds silcc project that include feedback by cosmic rays we show that the more extended discs in simulations including cosmic ray feedback naturally lead to larger scale heights for the dig which are more in line with observed scale heights we also show that including a fiducial cosmic ray heating term in our model can help to increase the temperature as a function of disc scale height but fails to reproduce observed dig nitrogen and sulphur forbidden line intensities we show that to reproduce these line emissions we require a heating mechanism that affects gas over a larger density range than is achieved by cosmic ray heating which can be achieved by fine tuning the total luminosity of ionising sources to get an appropriate ionising spectrum as a function of scale height this result sheds a new light on the relation between forbidden line emissions and temperature profiles for realistic dig gas distributions
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1,802.0775
Effects of Fall-Back Accretion on Proto-Magnetar Outflows in Gamma-Ray Bursts and Superluminous Supernovae
Rapidly spinning, strongly magnetized proto-neutron stars ("millisecond proto-magnetars") are candidate central engines of long-duration gamma-ray bursts (GRB), superluminous supernovae (SLSNe), and binary neutron star mergers. Magnetar birth may be accompanied by the fall-back of stellar debris, lasting for seconds or longer following the explosion. Accretion alters the magnetar evolution by (1) providing an additional source of rotational energy (or a potential sink, if the propeller mechanism operates); (2) enhancing the spin-down luminosity above the dipole rate by compressing the magnetosphere and expanding the polar cap region of open magnetic field lines; (3) supplying an additional accretion-powered neutrino luminosity that sustains the wind baryon-loading, even after the magnetar's internal neutrino luminosity has subsided. The more complex evolution of the jet power and magnetization of an accreting magnetar more readily accounts for the high 56Ni yields GRB SNe and irregular time evolution of some GRB light curves (e.g.~bursts with precursors followed by a long quiescent interval before the main emission episode). Additional baryon-loading from accretion-powered neutrino irradiation of the magnetar polar cap lengthens the timeframe over which the jet magnetization is in the requisite range sigma ~< 1e3 for efficient gamma-ray emission, thereby accommodating GRBs with ultra-long durations. Though accretion does not significantly raise the maximum energy budget from the limit of <~ few 1e52 ergs for an isolated magnetar, it greatly expands the range of magnetic field strengths and birth spin periods capable of powering GRB jets, reducing the differences between the magnetar properties normally invoked to explain GRBs versus SLSNe.
astro-ph.HE
rapidly spinning strongly magnetized protoneutron stars millisecond protomagnetars are candidate central engines of longduration gammaray bursts grb superluminous supernovae slsne and binary neutron star mergers magnetar birth may be accompanied by the fallback of stellar debris lasting for seconds or longer following the explosion accretion alters the magnetar evolution by 1 providing an additional source of rotational energy or a potential sink if the propeller mechanism operates 2 enhancing the spindown luminosity above the dipole rate by compressing the magnetosphere and expanding the polar cap region of open magnetic field lines 3 supplying an additional accretionpowered neutrino luminosity that sustains the wind baryonloading even after the magnetars internal neutrino luminosity has subsided the more complex evolution of the jet power and magnetization of an accreting magnetar more readily accounts for the high 56ni yields grb sne and irregular time evolution of some grb light curves egbursts with precursors followed by a long quiescent interval before the main emission episode additional baryonloading from accretionpowered neutrino irradiation of the magnetar polar cap lengthens the timeframe over which the jet magnetization is in the requisite range sigma 1e3 for efficient gammaray emission thereby accommodating grbs with ultralong durations though accretion does not significantly raise the maximum energy budget from the limit of few 1e52 ergs for an isolated magnetar it greatly expands the range of magnetic field strengths and birth spin periods capable of powering grb jets reducing the differences between the magnetar properties normally invoked to explain grbs versus slsne
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1,802.07751
Starburst to quiescent from HST/ALMA: Stars and dust unveil minor mergers in submillimeter galaxies at $z \sim 4.5$
Dust-enshrouded, starbursting, submillimeter galaxies (SMGs) at $z \geq 3$ have been proposed as progenitors of $z \geq 2$ compact quiescent galaxies (cQGs). To test this connection, we present a detailed spatially resolved study of the stars, dust and stellar mass in a sample of six submillimeter-bright starburst galaxies at $z \sim 4.5$. The stellar UV emission probed by HST is extended, irregular and shows evidence of multiple components. Informed by HST, we deblend Spitzer/IRAC data at rest-frame optical finding that the systems are undergoing minor mergers, with a typical stellar mass ratio of 1:6.5. The FIR dust continuum emission traced by ALMA locates the bulk of star formation in extremely compact regions (median $r_{\rm{e}} = 0.70 \pm 0.29$ kpc) and it is in all cases associated with the most massive component of the mergers (median $\log (M_{*}/M_{\odot}) = 10.49 \pm 0.32$). We compare spatially resolved UV slope ($\beta$) maps with the FIR dust continuum to study the infrared excess ($\rm{IRX} = L_{\rm{IR}}/L_{\rm{UV}}$)-$\beta$ relation. The SMGs display systematically higher $\rm{IRX}$ values than expected from the nominal trend, demonstrating that the FIR and UV emissions are spatially disconnected. Finally, we show that the SMGs fall on the mass-size plane at smaller stellar masses and sizes than cQGs at $z = 2$. Taking into account the expected evolution in stellar mass and size between $z = 4.5$ and $z = 2$ due to the ongoing starburst and mergers with minor companions, this is in agreement with a direct evolutionary connection between the two populations.
astro-ph.GA
dustenshrouded starbursting submillimeter galaxies smgs at z geq 3 have been proposed as progenitors of z geq 2 compact quiescent galaxies cqgs to test this connection we present a detailed spatially resolved study of the stars dust and stellar mass in a sample of six submillimeterbright starburst galaxies at z sim 45 the stellar uv emission probed by hst is extended irregular and shows evidence of multiple components informed by hst we deblend spitzerirac data at restframe optical finding that the systems are undergoing minor mergers with a typical stellar mass ratio of 165 the fir dust continuum emission traced by alma locates the bulk of star formation in extremely compact regions median r_rme 070 pm 029 kpc and it is in all cases associated with the most massive component of the mergers median log m_m_odot 1049 pm 032 we compare spatially resolved uv slope beta maps with the fir dust continuum to study the infrared excess rmirx l_rmirl_rmuvbeta relation the smgs display systematically higher rmirx values than expected from the nominal trend demonstrating that the fir and uv emissions are spatially disconnected finally we show that the smgs fall on the masssize plane at smaller stellar masses and sizes than cqgs at z 2 taking into account the expected evolution in stellar mass and size between z 45 and z 2 due to the ongoing starburst and mergers with minor companions this is in agreement with a direct evolutionary connection between the two populations
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1,802.07752
Type IIP supernova light curves affected by the acceleration of red supergiant winds
We introduce the first synthetic light-curve model set of Type IIP supernovae exploded within circumstellar media in which the acceleration of the red supergiant winds is taken into account. Because wind acceleration makes the wind velocities near the progenitors low, the density of the immediate vicinity of the red supergiant supernova progenitors can be higher than that extrapolated by using a constant terminal wind velocity. Therefore, even if the mass-loss rate of the progenitor is relatively low, it can have a dense circumstellar medium at the immediate stellar vicinity and the early light curves of Type IIP supernovae are significantly affected by it. We adopt a simple beta velocity law to formulate the wind acceleration. We provide bolometric and multicolor light curves of Type IIP supernovae exploding within such accelerated winds from the combinations of three progenitors, 12 - 16 Msun; five beta, 1-5; seven mass-loss rates, 1e-5 - 1e-2 Msun/yr; and four explosion energies, 0.5e51 - 2e51 erg. All the light curve models are available at https://goo.gl/o5phYb. When the circumstellar density is sufficiently high, our models do not show a classical shock breakout as a consequence of the interaction with the dense and optically-thick circumstellar media. Instead, they show a delayed 'wind breakout', substantially affecting early light curves of Type IIP supernovae. We find that the mass-loss rates of the progenitors need to be 1e-3 - 1e-2 Msun/yr to explain typical rise times of 5 - 10 days in Type IIP supernovae assuming a dense circumstellar radius of 1e15 cm.
astro-ph.HE astro-ph.SR
we introduce the first synthetic lightcurve model set of type iip supernovae exploded within circumstellar media in which the acceleration of the red supergiant winds is taken into account because wind acceleration makes the wind velocities near the progenitors low the density of the immediate vicinity of the red supergiant supernova progenitors can be higher than that extrapolated by using a constant terminal wind velocity therefore even if the massloss rate of the progenitor is relatively low it can have a dense circumstellar medium at the immediate stellar vicinity and the early light curves of type iip supernovae are significantly affected by it we adopt a simple beta velocity law to formulate the wind acceleration we provide bolometric and multicolor light curves of type iip supernovae exploding within such accelerated winds from the combinations of three progenitors 12 16 msun five beta 15 seven massloss rates 1e5 1e2 msunyr and four explosion energies 05e51 2e51 erg all the light curve models are available at httpsgooglo5phyb when the circumstellar density is sufficiently high our models do not show a classical shock breakout as a consequence of the interaction with the dense and opticallythick circumstellar media instead they show a delayed wind breakout substantially affecting early light curves of type iip supernovae we find that the massloss rates of the progenitors need to be 1e3 1e2 msunyr to explain typical rise times of 5 10 days in type iip supernovae assuming a dense circumstellar radius of 1e15 cm
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1,802.07753
Searching for propeller-phase ULXs in the XMM-Newton Serendipitous Source Catalogue
We search for transient sources in a sample of ULXs from the 3XMM-DR4 release of the XMM-Newton Serendipitous Source Catalogue in order to find candidate neutron star ULXs alternating between an accreting state and the propeller regime, in which the luminosity drops dramatically. By examining their fluxes and flux upper limits, we identify five ULXs that demonstrate long-term variability of over an order of magnitude. Using Chandra and Swift data to further characterise their light curves, we find that two of these sources are detected only once and could be X-ray binaries in outburst that only briefly reach ULX luminosities. Two others are consistent with being super-Eddington accreting sources with high levels of inter-observation variability. One source, M51 ULX-4, demonstrates apparent bimodal flux behaviour that could indicate the propeller regime. It has a hard X-ray spectrum, but no significant pulsations in its timing data, although with an upper limit of 10% of the signal pulsed at ~1.5 Hz a pulsating ULX cannot be excluded, particularly if the pulsations are transient. By simulating XMM-Newton observations of a population of pulsating ULXs, we predict that there could be approximately 200 other bimodal ULXs that have not been observed sufficiently well by XMM-Newton to be identified as transient.
astro-ph.HE
we search for transient sources in a sample of ulxs from the 3xmmdr4 release of the xmmnewton serendipitous source catalogue in order to find candidate neutron star ulxs alternating between an accreting state and the propeller regime in which the luminosity drops dramatically by examining their fluxes and flux upper limits we identify five ulxs that demonstrate longterm variability of over an order of magnitude using chandra and swift data to further characterise their light curves we find that two of these sources are detected only once and could be xray binaries in outburst that only briefly reach ulx luminosities two others are consistent with being supereddington accreting sources with high levels of interobservation variability one source m51 ulx4 demonstrates apparent bimodal flux behaviour that could indicate the propeller regime it has a hard xray spectrum but no significant pulsations in its timing data although with an upper limit of 10 of the signal pulsed at 15 hz a pulsating ulx cannot be excluded particularly if the pulsations are transient by simulating xmmnewton observations of a population of pulsating ulxs we predict that there could be approximately 200 other bimodal ulxs that have not been observed sufficiently well by xmmnewton to be identified as transient
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1,802.07754
ALICE Data Release: A revaluation of HST-NICMOS coronagraphic images
The Hubble Space Telescope (HST) NICMOS instrument has been used from 1997 to 2008 to perform coronagraphic observations of about 400 targets. Most of them were part of surveys looking for substellar companions or resolved circumstellar disks to young nearby stars, making the NICMOS coronagraphic archive a valuable database for exoplanets and disks studies. As part of the Archival Legacy Investigations of Circumstellar Environments (ALICE) program, we have consistently re-processed a large fraction of the NICMOS coronagrahic archive using advanced PSF subtraction methods. We present here the high-level science products of these re-analyzed data, which we delivered back to the community through the Mikulski Archive for Space Telescopes (MAST) http://dx.doi.org/10.17909/T9W89V . We also present the second version of the HCI-FITS format (for High-Contrast Imaging FITS format), which we developed as a standard format for data exchange of imaging reduced science products. These re-analyzed products are openly available for population statistics studies, characterization of specific targets, or detected point source identification.
astro-ph.EP astro-ph.IM
the hubble space telescope hst nicmos instrument has been used from 1997 to 2008 to perform coronagraphic observations of about 400 targets most of them were part of surveys looking for substellar companions or resolved circumstellar disks to young nearby stars making the nicmos coronagraphic archive a valuable database for exoplanets and disks studies as part of the archival legacy investigations of circumstellar environments alice program we have consistently reprocessed a large fraction of the nicmos coronagrahic archive using advanced psf subtraction methods we present here the highlevel science products of these reanalyzed data which we delivered back to the community through the mikulski archive for space telescopes mast httpdxdoiorg1017909t9w89v we also present the second version of the hcifits format for highcontrast imaging fits format which we developed as a standard format for data exchange of imaging reduced science products these reanalyzed products are openly available for population statistics studies characterization of specific targets or detected point source identification
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1,802.07755
Emergent light crystal from frustration and pump engineering
We demonstrate how pump engineering drives the emergence of frustration-induced quasi-long-range order in a low-dimensional photonic cavity array. We consider a Lieb chain of nonlinear cavities as described by the Bose-Hubbard model and featuring a photonic flat band in the single-particle spectrum. Incoherent pumping of the Lieb lattice leads to a photonic density-wave which manifests an algebraic decay of correlations with twice the period of the lattice unit cell. This work opens up new directions for the emergence of strongly-correlated phases in quantum optical frustrated systems through pump design.
cond-mat.quant-gas
we demonstrate how pump engineering drives the emergence of frustrationinduced quasilongrange order in a lowdimensional photonic cavity array we consider a lieb chain of nonlinear cavities as described by the bosehubbard model and featuring a photonic flat band in the singleparticle spectrum incoherent pumping of the lieb lattice leads to a photonic densitywave which manifests an algebraic decay of correlations with twice the period of the lattice unit cell this work opens up new directions for the emergence of stronglycorrelated phases in quantum optical frustrated systems through pump design
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1,802.07756
Determining the best classifier for predicting the value of a boolean field on a blood donor database using genetic algorithms
Motivation: Thanks to digitization, we often have access to large databases, consisting of various fields of information, ranging from numbers to texts and even boolean values. Such databases lend themselves especially well to machine learning, classification and big data analysis tasks. We are able to train classifiers, using already existing data and use them for predicting the values of a certain field, given that we have information regarding the other fields. Most specifically, in this study, we look at the Electronic Health Records (EHRs) that are compiled by hospitals. These EHRs are convenient means of accessing data of individual patients, but there processing as a whole still remains a task. However, EHRs that are composed of coherent, well-tabulated structures lend themselves quite well to the application to machine language, via the usage of classifiers. In this study, we look at a Blood Transfusion Service Center Data Set (Data taken from the Blood Transfusion Service Center in Hsin-Chu City in Taiwan). We used scikit-learn machine learning in python. From Support Vector Machines(SVM), we use Support Vector Classification(SVC), from the linear model we import Perceptron. We also used the K.neighborsclassifier and the decision tree classifiers. Furthermore, we use the TPOT library to find an optimized pipeline using genetic algorithms. Using the above classifiers, we score each one of them using k fold cross-validation. Contact: ritabratamaiti@hiretrex.com GitHub Repository: https://github.com/ritabratamaiti/Blooddonorprediction
stat.ML cs.LG
motivation thanks to digitization we often have access to large databases consisting of various fields of information ranging from numbers to texts and even boolean values such databases lend themselves especially well to machine learning classification and big data analysis tasks we are able to train classifiers using already existing data and use them for predicting the values of a certain field given that we have information regarding the other fields most specifically in this study we look at the electronic health records ehrs that are compiled by hospitals these ehrs are convenient means of accessing data of individual patients but there processing as a whole still remains a task however ehrs that are composed of coherent welltabulated structures lend themselves quite well to the application to machine language via the usage of classifiers in this study we look at a blood transfusion service center data set data taken from the blood transfusion service center in hsinchu city in taiwan we used scikitlearn machine learning in python from support vector machinessvm we use support vector classificationsvc from the linear model we import perceptron we also used the kneighborsclassifier and the decision tree classifiers furthermore we use the tpot library to find an optimized pipeline using genetic algorithms using the above classifiers we score each one of them using k fold crossvalidation contact ritabratamaitihiretrexcom github repository httpsgithubcomritabratamaitiblooddonorprediction
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1,802.07757
Pointwise a posteriori error bounds for blow-up in the semilinear heat equation
This work is concerned with the development of a space-time adaptive numerical method, based on a rigorous a posteriori error bound, for the semilinear heat equation with a general local Lipschitz reaction term whose solution may blow-up in finite time. More specifically, conditional a posteriori error bounds are derived in the $L^{\infty}L^{\infty}$ norm for a first order in time, implicit-explicit (IMEX), conforming finite element method in space discretization of the problem. Numerical experiments applied to both blow-up and non blow-up cases highlight the generality of our approach and complement the theoretical results.
math.NA
this work is concerned with the development of a spacetime adaptive numerical method based on a rigorous a posteriori error bound for the semilinear heat equation with a general local lipschitz reaction term whose solution may blowup in finite time more specifically conditional a posteriori error bounds are derived in the linftylinfty norm for a first order in time implicitexplicit imex conforming finite element method in space discretization of the problem numerical experiments applied to both blowup and non blowup cases highlight the generality of our approach and complement the theoretical results
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1,802.07758
Double resummation for Higgs production
We present the first double-resummed prediction of the inclusive cross section for the main Higgs production channel in proton-proton collisions, namely gluon fusion. Our calculation incorporates to all orders in perturbation theory two distinct towers of logarithmic corrections which are enhanced, respectively, at threshold, i.e. large x, and in the high-energy limit, i.e. small x. Large-x logarithms are resummed to next-to-next-to-next-to-leading logarithmic accuracy, while small-x ones to leading logarithmic accuracy. The double-resummed cross section is furthermore matched to the state-of-the-art fixed-order prediction at next-to-next-to-next-to-leading accuracy. We find that double resummation corrects the Higgs production rate by 2% at the currently explored center-of-mass energy of 13 TeV and its impact reaches 10% at future circular colliders at 100 TeV.
hep-ph
we present the first doubleresummed prediction of the inclusive cross section for the main higgs production channel in protonproton collisions namely gluon fusion our calculation incorporates to all orders in perturbation theory two distinct towers of logarithmic corrections which are enhanced respectively at threshold ie large x and in the highenergy limit ie small x largex logarithms are resummed to nexttonexttonexttoleading logarithmic accuracy while smallx ones to leading logarithmic accuracy the doubleresummed cross section is furthermore matched to the stateoftheart fixedorder prediction at nexttonexttonexttoleading accuracy we find that double resummation corrects the higgs production rate by 2 at the currently explored centerofmass energy of 13 tev and its impact reaches 10 at future circular colliders at 100 tev
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1,802.07759
Non-asymptotic Error Bounds For Constant Stepsize Stochastic Approximation For Tracking Mobile Agents
This work revisits the constant stepsize stochastic approximation algorithm for tracking a slowly moving target and obtains a bound for the tracking error that is valid for the entire time axis, using the Alekseev non-linear variation of constants formula. It is the first non-asymptptic bound for the entire time axis in the sense that it is not based on the vanishing stepsize limit and associated limit theorems unlike prior works, and captures clearly the dependence on problem parameters and the dimension.
eess.SP
this work revisits the constant stepsize stochastic approximation algorithm for tracking a slowly moving target and obtains a bound for the tracking error that is valid for the entire time axis using the alekseev nonlinear variation of constants formula it is the first nonasymptptic bound for the entire time axis in the sense that it is not based on the vanishing stepsize limit and associated limit theorems unlike prior works and captures clearly the dependence on problem parameters and the dimension
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