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710.4853
Erratum: Propagation Effects on the Breakdown of a Linear Amplifier Model: Complex-Mass Schrodinger Equation Driven by the Square of a Gaussian Field
The proof of the inequality $\lambda_{q}(x,t)\le (q\mu_{x,t} -0^+)^{-1}$ [p 750, below Eq. (29)] is based on the statement that ${\cal E}(x,t;s)$ is an entire function of $s\in {\mathbb C}^M$ [see below Eq. (30)]. But according to Equation (9) and Lemma 1, all we know is that ${\cal E}(x,t;s)$ is an entire function of $k(s)\in {\mathbb R}^N$. Nevertheless, the above inequality holds, hence the proposition 1.
math-ph math.MP
the proof of the inequality lambda_qxtle qmu_xt 01 p 750 below eq 29 is based on the statement that cal exts is an entire function of sin mathbb cm see below eq 30 but according to equation 9 and lemma 1 all we know is that cal exts is an entire function of ksin mathbb rn nevertheless the above inequality holds hence the proposition 1
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710.4854
Big bang nucleosynthesis as a probe of fundamental "constants"
Big Bang nucleosynthesis (BBN) is the earliest sensitive probe of the values of many fundamental particle physics parameters. We have found the leading linear dependences of primordial abundances on all relevant parameters of the standard BBN code, including binding energies and nuclear reaction rates. This enables us to set limits on possible variations of fundamental parameters. We find that 7Li is expected to be significantly more sensitive than other species to many fundamental parameters, a result which also holds for variations of coupling strengths in grand unified (GUT) models. Our work also indicates which areas of nuclear theory need further development if the values of ``constants'' are to be more accurately probed.
astro-ph gr-qc hep-ph hep-th nucl-th
big bang nucleosynthesis bbn is the earliest sensitive probe of the values of many fundamental particle physics parameters we have found the leading linear dependences of primordial abundances on all relevant parameters of the standard bbn code including binding energies and nuclear reaction rates this enables us to set limits on possible variations of fundamental parameters we find that 7li is expected to be significantly more sensitive than other species to many fundamental parameters a result which also holds for variations of coupling strengths in grand unified gut models our work also indicates which areas of nuclear theory need further development if the values of constants are to be more accurately probed
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710.4855
Radiative Penguin B Decays at the B Factories
In this article, I review the most recent results in radiative penguin decays from the B factories Belle and Babar. Most notably, I will talk about the recent new observations in the decays B -> (rho/omega) gamma, a new analysis technique in b -> s gamma, and first measurements of radiative penguin decays in the B_s meson system. Finally, I will summarize the current status and future prospects of radiative penguin B physics at the B factories.
hep-ex
in this article i review the most recent results in radiative penguin decays from the b factories belle and babar most notably i will talk about the recent new observations in the decays b rhoomega gamma a new analysis technique in b s gamma and first measurements of radiative penguin decays in the b_s meson system finally i will summarize the current status and future prospects of radiative penguin b physics at the b factories
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710.4856
Extending the scope of microscopic solvability: Combination of the Kruskal-Segur method with Zauderer decomposition
Successful applications of the Kruskal-Segur approach to interfacial pattern formation have remained limited due to the necessity of an integral formulation of the problem. This excludes nonlinear bulk equations, rendering convection intractable. Combining the method with Zauderer's asymptotic decomposition scheme, we are able to strongly extend its scope of applicability and solve selection problems based on free boundary formulations in terms of partial differential equations alone. To demonstrate the technique, we give the first analytic solution of the problem of velocity selection for dendritic growth in a forced potential flow.
nlin.PS
successful applications of the kruskalsegur approach to interfacial pattern formation have remained limited due to the necessity of an integral formulation of the problem this excludes nonlinear bulk equations rendering convection intractable combining the method with zauderers asymptotic decomposition scheme we are able to strongly extend its scope of applicability and solve selection problems based on free boundary formulations in terms of partial differential equations alone to demonstrate the technique we give the first analytic solution of the problem of velocity selection for dendritic growth in a forced potential flow
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710.4857
Scintillation light produced by low-energy beams of highly-charged ions
Measurements have been performed of scintillation light intensities emitted from various inorganic scintillators irradiated with low-energy beams of highly-charged ions from an electron beam ion source (EBIS) and an electron cyclotron resonance ion source (ECRIS). Beams of xenon ions Xe$^{q+}$ with various charge states between $q$=2 and $q$=18 have been used at energies between 5 keV and 17.5 keV per charge generated by the ECRIS. The intensity of the beam was typically varied between 1 and 100 nA. Beams of highly charged residual gas ions have been produced by the EBIS at 4.5 keV per charge and with low intensities down to 100 pA. The scintillator materials used are flat screens of P46 YAG and P43 phosphor. In all cases, scintillation light emitted from the screen surface was detected by a CCD camera. The scintillation light intensity has been found to depend linearly on the kinetic ion energy per time deposited into the scintillator, while up to $q$=18 no significant contribution from the ions' potential energy was found. We discuss the results on the background of a possible use as beam diagnostics e.g. for the new HITRAP facility at GSI, Germany.
physics.atom-ph physics.ins-det
measurements have been performed of scintillation light intensities emitted from various inorganic scintillators irradiated with lowenergy beams of highlycharged ions from an electron beam ion source ebis and an electron cyclotron resonance ion source ecris beams of xenon ions xeq with various charge states between q2 and q18 have been used at energies between 5 kev and 175 kev per charge generated by the ecris the intensity of the beam was typically varied between 1 and 100 na beams of highly charged residual gas ions have been produced by the ebis at 45 kev per charge and with low intensities down to 100 pa the scintillator materials used are flat screens of p46 yag and p43 phosphor in all cases scintillation light emitted from the screen surface was detected by a ccd camera the scintillation light intensity has been found to depend linearly on the kinetic ion energy per time deposited into the scintillator while up to q18 no significant contribution from the ions potential energy was found we discuss the results on the background of a possible use as beam diagnostics eg for the new hitrap facility at gsi germany
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710.4858
Experimentally feasible quantum erasure-correcting code for continuous variables
We devise a scheme that protects quantum coherent states of light from probabilistic losses, thus achieving the first continuous-variable quantum erasure-correcting code. If the occurrence of erasures can be probed, then the decoder enables, in principle, a perfect recovery of the original light states. Otherwise, if supplemented with postselection based on homodyne detection, this code can be turned into an efficient erasure-filtration scheme. The experimental feasibility of the proposed protocol is carefully addressed.
quant-ph
we devise a scheme that protects quantum coherent states of light from probabilistic losses thus achieving the first continuousvariable quantum erasurecorrecting code if the occurrence of erasures can be probed then the decoder enables in principle a perfect recovery of the original light states otherwise if supplemented with postselection based on homodyne detection this code can be turned into an efficient erasurefiltration scheme the experimental feasibility of the proposed protocol is carefully addressed
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710.4859
Orbital eccentricities of binary systems with a former AGB star
Many binary stellar systems in which the primary star is beyond the asymptotic giant branch (AGB) evolutionary phase show significant orbital eccentricities whereas current binary interaction models predict their orbits to be circularised. We analyse how the orbital parameters in a system are modified under mass loss and mass exchange among its binary components and propose a model for enhanced mass-loss from the AGB star due to tidal interaction with its companion, which allows a smooth transition between the wind and Roche-lobe overflow mass-loss regimes. We explicitly follow its effect along the orbit on the change of eccentricity and orbital semi-major axis, as well as the effect of accretion by the companion. We calculate timescales for the variation of these orbital parameters and compare them to the tidal circularisation timescale. We find that in many cases, due to the enhanced mass loss of the AGB component at orbital phases closer to the periastron, the net eccentricity growth rate in one orbit is comparable to the rate of tidal circularisation. We show that with this eccentricity enhancing mechanism it is possible to reproduce the orbital period and eccentricity of the Sirius system, which under the standard assumptions of binary interaction is expected to be circularised. We also show that this mechanism may provide an explanation for the eccentricities of most barium star systems, which are expected to be circularised due to tidal dissipation. By proposing a tidally enhanced model of mass loss from AGB stars we find a mechanism which efficiently works against the tidal circularisation of the orbit, which explains the significant eccentricities observed in binary systems containing a white dwarf and a less evolved companion, such as Sirius and systems with barium stars.
astro-ph
many binary stellar systems in which the primary star is beyond the asymptotic giant branch agb evolutionary phase show significant orbital eccentricities whereas current binary interaction models predict their orbits to be circularised we analyse how the orbital parameters in a system are modified under mass loss and mass exchange among its binary components and propose a model for enhanced massloss from the agb star due to tidal interaction with its companion which allows a smooth transition between the wind and rochelobe overflow massloss regimes we explicitly follow its effect along the orbit on the change of eccentricity and orbital semimajor axis as well as the effect of accretion by the companion we calculate timescales for the variation of these orbital parameters and compare them to the tidal circularisation timescale we find that in many cases due to the enhanced mass loss of the agb component at orbital phases closer to the periastron the net eccentricity growth rate in one orbit is comparable to the rate of tidal circularisation we show that with this eccentricity enhancing mechanism it is possible to reproduce the orbital period and eccentricity of the sirius system which under the standard assumptions of binary interaction is expected to be circularised we also show that this mechanism may provide an explanation for the eccentricities of most barium star systems which are expected to be circularised due to tidal dissipation by proposing a tidally enhanced model of mass loss from agb stars we find a mechanism which efficiently works against the tidal circularisation of the orbit which explains the significant eccentricities observed in binary systems containing a white dwarf and a less evolved companion such as sirius and systems with barium stars
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710.486
Loschmidt cooling by time reversal of atomic matter waves
We propose an experimental scheme which allows to realize approximate time reversal of matter waves for ultracold atoms in the regime of quantum chaos. We show that a significant fraction of the atoms return back to their original state, being at the same time cooled down by several orders of magnitude. We give a theoretical description of this effect supported by extensive numerical simulations. The proposed scheme can be implemented with existing experimental setups.
cond-mat.stat-mech nlin.CD quant-ph
we propose an experimental scheme which allows to realize approximate time reversal of matter waves for ultracold atoms in the regime of quantum chaos we show that a significant fraction of the atoms return back to their original state being at the same time cooled down by several orders of magnitude we give a theoretical description of this effect supported by extensive numerical simulations the proposed scheme can be implemented with existing experimental setups
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710.4861
Van der Corput sets in Z^d
In this partly expository paper we study van der Corput sets in $\Z^d$, with a focus on connections with harmonic analysis and recurrence properties of measure preserving dynamical systems. We prove multidimensional versions of some classical results obtained for $d=1$ in \cite{K-MF} and \cite{R}, establish new characterizations, introduce and discuss some modifications of van der Corput sets which correspond to various notions of recurrence, provide numerous examples and formulate some natural open questions.
math.DS math.NT
in this partly expository paper we study van der corput sets in zd with a focus on connections with harmonic analysis and recurrence properties of measure preserving dynamical systems we prove multidimensional versions of some classical results obtained for d1 in citekmf and citer establish new characterizations introduce and discuss some modifications of van der corput sets which correspond to various notions of recurrence provide numerous examples and formulate some natural open questions
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710.4862
Intersective polynomials and polynomial Szemeredi theorem
Let $P=\{p_{1},\ld,p_{r}\}\subset\Q[n_{1},\ld,n_{m}]$ be a family of polynomials such that $p_{i}(\Z^{m})\sle\Z$, $i=1,\ld,r$. We say that the family $P$ has {\it PSZ property} if for any set $E\sle\Z$ with $d^{*}(E)=\limsup_{N-M\ras\infty}\frac{|E\cap[M,N-1]|}{N-M}>0$ there exist infinitely many $n\in\Z^{m}$ such that $E$ contains a polynomial progression of the form \hbox{$\{a,a+p_{1}(n),\ld,a+p_{r}(n)\}$}. We prove that a polynomial family $P=\{p_{1},\ld,p_{r}\}$ has PSZ property if and only if the polynomials $p_{1},\ld,p_{r}$ are {\it jointly intersective}, meaning that for any $k\in\N$ there exists $n\in\Z^{m}$ such that the integers $p_{1}(n),\ld,p_{r}(n)$ are all divisible by $k$. To obtain this result we give a new ergodic proof of the polynomial Szemer\'{e}di theorem, based on the fact that the key to the phenomenon of polynomial multiple recurrence lies with the dynamical systems defined by translations on nilmanifolds. We also obtain, as a corollary, the following generalization of the polynomial van der Waerden theorem: If $p_{1},\ld,p_{r}\in\Q[n]$ are jointly intersective integral polynomials, then for any finite partition of $\Z$, $\Z=\bigcup_{i=1}^{k}E_{i}$, there exist $i\in\{1,\ld,k\}$ and $a,n\in E_{i}$ such that $\{a,a+p_{1}(n),\ld,a+p_{r}(n)\}\sln E_{i}$.
math.DS math.CO
let pp_1ldp_rsubsetqn_1ldn_m be a family of polynomials such that p_izmslez i1ldr we say that the family p has it psz property if for any set eslez with delimsup_nmrasinftyfracecapmn1nm0 there exist infinitely many ninzm such that e contains a polynomial progression of the form hboxaap_1nldap_rn we prove that a polynomial family pp_1ldp_r has psz property if and only if the polynomials p_1ldp_r are it jointly intersective meaning that for any kinn there exists ninzm such that the integers p_1nldp_rn are all divisible by k to obtain this result we give a new ergodic proof of the polynomial szemeredi theorem based on the fact that the key to the phenomenon of polynomial multiple recurrence lies with the dynamical systems defined by translations on nilmanifolds we also obtain as a corollary the following generalization of the polynomial van der waerden theorem if p_1ldp_rinqn are jointly intersective integral polynomials then for any finite partition of z zbigcup_i1ke_i there exist iin1ldk and anin e_i such that aap_1nldap_rnsln e_i
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710.4863
Near-infrared adaptive optics imaging of high redshift quasars
The properties of high redshift quasar host galaxies are studied, in order to investigate the connection between galaxy evolution, nuclear activity, and the formation of supermassive black holes. We combine new near-infrared observations of three high redshift quasars (2 < z < 3), obtained at the ESO Very Large Telescope equipped with adaptive optics, with selected data from the literature. For the three new objects we were able to detect and characterize the properties of the host galaxy, found to be consistent with those of massive elliptical galaxies of M(R) ~ -24.7 for the one radio loud quasar, and M(R) ~ -23.8 for the two radio quiet quasars. When combined with existing data at lower redshift, these new observations depict a scenario where the host galaxies of radio loud quasars are seen to follow the expected trend of luminous (~5L*) elliptical galaxies undergoing passive evolution. This trend is remarkably similar to that followed by radio galaxies at z > 1.5. Radio quiet quasars hosts also follow a similar trend but at a lower average luminosity (~0.5 mag dimmer). The data indicate that quasar host galaxies are already fully formed at epochs as early as ~2 Gyr after the Big Bang and then passively fade in luminosity to the present epoch.
astro-ph
the properties of high redshift quasar host galaxies are studied in order to investigate the connection between galaxy evolution nuclear activity and the formation of supermassive black holes we combine new nearinfrared observations of three high redshift quasars 2 z 3 obtained at the eso very large telescope equipped with adaptive optics with selected data from the literature for the three new objects we were able to detect and characterize the properties of the host galaxy found to be consistent with those of massive elliptical galaxies of mr 247 for the one radio loud quasar and mr 238 for the two radio quiet quasars when combined with existing data at lower redshift these new observations depict a scenario where the host galaxies of radio loud quasars are seen to follow the expected trend of luminous 5l elliptical galaxies undergoing passive evolution this trend is remarkably similar to that followed by radio galaxies at z 15 radio quiet quasars hosts also follow a similar trend but at a lower average luminosity 05 mag dimmer the data indicate that quasar host galaxies are already fully formed at epochs as early as 2 gyr after the big bang and then passively fade in luminosity to the present epoch
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710.4864
Conformal invariance and finiteness theorems for non-planar beta-deformed N=4 SYM theory
We study the conformal invariance of non-planar beta-deformed N=4 SYM theory using the coupling constant reduction (CCR) formalism. We show that up to order g^10, differently from the planar case, we can remove the scheme dependence in the definition of the theory without reducing to the real beta case. We also compute the gauge beta function up to four loops and see that the generalized finiteness theorems proposed in [hep-th: 0705.1483] still hold.
hep-th
we study the conformal invariance of nonplanar betadeformed n4 sym theory using the coupling constant reduction ccr formalism we show that up to order g10 differently from the planar case we can remove the scheme dependence in the definition of the theory without reducing to the real beta case we also compute the gauge beta function up to four loops and see that the generalized finiteness theorems proposed in hepth 07051483 still hold
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710.4865
Exact mesoscopic correlation functions of the pairing model
We study the static correlation functions of the Richardson pairing model (also known as the reduced or discrete-state BCS model) in the canonical ensemble. Making use of the Algebraic Bethe Ansatz formalism, we obtain exact expressions which are easily evaluated numerically for any value of the pairing strength up to large numbers of particles. We provide explicit results at half-filling and extensively discuss their finite-size scaling behavior.
cond-mat.mes-hall cond-mat.supr-con nucl-th
we study the static correlation functions of the richardson pairing model also known as the reduced or discretestate bcs model in the canonical ensemble making use of the algebraic bethe ansatz formalism we obtain exact expressions which are easily evaluated numerically for any value of the pairing strength up to large numbers of particles we provide explicit results at halffilling and extensively discuss their finitesize scaling behavior
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710.4866
Mixed action simulations: approaching physical quark masses
Some algorithmic details of our $N_f=2+1$ QCD mixed action simulations with overlap valence and improved Wilson sea quarks are presented.
hep-lat
some algorithmic details of our n_f21 qcd mixed action simulations with overlap valence and improved wilson sea quarks are presented
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710.4867
Bi-clique Communities
We present a novel method for detecting communities in bipartite networks. Based on an extension of the $k$-clique community detection algorithm, we demonstrate how modular structure in bipartite networks presents itself as overlapping bicliques. If bipartite information is available, the bi-clique community detection algorithm retains all of the advantages of the $k$-clique algorithm, but avoids discarding important structural information when performing a one-mode projection of the network. Further, the bi-clique community detection algorithm provides a new level of flexibility by incorporating independent clique thresholds for each of the non-overlapping node sets in the bipartite network.
physics.data-an physics.soc-ph
we present a novel method for detecting communities in bipartite networks based on an extension of the kclique community detection algorithm we demonstrate how modular structure in bipartite networks presents itself as overlapping bicliques if bipartite information is available the biclique community detection algorithm retains all of the advantages of the kclique algorithm but avoids discarding important structural information when performing a onemode projection of the network further the biclique community detection algorithm provides a new level of flexibility by incorporating independent clique thresholds for each of the nonoverlapping node sets in the bipartite network
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710.4868
SO(10)-like Superstring Standard Model with R-parity from the Heterotic String
We construct a supersymmetric standard model in the context of the Z_{12-I} orbifold compactification of the E_8 x E_8' heterotic string theory. The gauge group is SU(3)_c x SU(2)_L x U(1)_Y x U(1)^4 x [SO(10) x U(1)^3]' with sin^2\theta_W = 3/8. We obtain three families of SO(10) spinor-like chiral matter states, and Higgs doublets. All other extra states are exactly vector-like under the standard model gauge symmetry. There are numerous standard model singlets, many of which get VEVs such that only the standard model gauge symmetry survives and desired Yukawa couplings can be generated at lower energies. In particular, all vector-like exotic states achieve superheavy masses and the R-parity can be preserved.
hep-th hep-ph
we construct a supersymmetric standard model in the context of the z_12i orbifold compactification of the e_8 x e_8 heterotic string theory the gauge group is su3_c x su2_l x u1_y x u14 x so10 x u13 with sin2theta_w 38 we obtain three families of so10 spinorlike chiral matter states and higgs doublets all other extra states are exactly vectorlike under the standard model gauge symmetry there are numerous standard model singlets many of which get vevs such that only the standard model gauge symmetry survives and desired yukawa couplings can be generated at lower energies in particular all vectorlike exotic states achieve superheavy masses and the rparity can be preserved
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710.4869
Elementary aspects of the geometry of metric spaces
The setting of metric spaces is very natural for numerous questions concerning manifolds, norms, and fractal sets, and a few of the main ingredients are surveyed here.
math.MG
the setting of metric spaces is very natural for numerous questions concerning manifolds norms and fractal sets and a few of the main ingredients are surveyed here
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710.487
The Lonely Vertex Problem
In a locally finite tiling of n-dim Euclidean space by convex polytopes, each point of the space is either a vertex of at least two tiles, or no vertex at all.
math.MG
in a locally finite tiling of ndim euclidean space by convex polytopes each point of the space is either a vertex of at least two tiles or no vertex at all
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710.4871
Light curve analysis of the hybrid sdB pulsators HS0702+6043 and HS2201+2610
We present the detection of low-amplitude, long-period g-modes in two individual sdBV stars which are known to be p-mode pulsators. Only few of these hybrid objects, showing both p- and g-modes, are known today. We resolve the g-mode domain in HS0702+6043 and add HS2201+2610 to the list of hybrid pulsators. To discover the low-amplitude g-modes, a filtering algorithm based on wavelet transformations was applied to denoise observational data.
astro-ph
we present the detection of lowamplitude longperiod gmodes in two individual sdbv stars which are known to be pmode pulsators only few of these hybrid objects showing both p and gmodes are known today we resolve the gmode domain in hs07026043 and add hs22012610 to the list of hybrid pulsators to discover the lowamplitude gmodes a filtering algorithm based on wavelet transformations was applied to denoise observational data
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710.4872
Mapping Observations of 6.7 GHz Methanol Masers with Japanese VLBI Network
We have observed 13 methanol maser sources associated with massive star-forming regions; W3(OH), Mon R2, S 255, W 33A, IRAS 18151-1208, G 24.78+0.08, G 29.95-0.02, IRAS 18556+0136, W 48, OH 43.8-0.1, ON 1, Cep A and NGC 7538 at 6.7 GHz using the Japanese VLBI Network (JVN). Twelve of the thirteen sources were detected at our longest baseline of $\sim$50 M$\lambda$, and their images are presented. Seven of them are the first VLBI images at 6.7 GHz. This high detection rate and the small fringe spacing of $\sim$4 milli-arcsecond suggest that most of the methanol maser sources have compact structure. Given this compactness as well as the known properties of long-life and small internal-motion, this methanol maser line is suitable for astrometry with VLBI.
astro-ph
we have observed 13 methanol maser sources associated with massive starforming regions w3oh mon r2 s 255 w 33a iras 181511208 g 2478008 g 2995002 iras 185560136 w 48 oh 43801 on 1 cep a and ngc 7538 at 67 ghz using the japanese vlbi network jvn twelve of the thirteen sources were detected at our longest baseline of sim50 mlambda and their images are presented seven of them are the first vlbi images at 67 ghz this high detection rate and the small fringe spacing of sim4 milliarcsecond suggest that most of the methanol maser sources have compact structure given this compactness as well as the known properties of longlife and small internalmotion this methanol maser line is suitable for astrometry with vlbi
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710.4873
The shadow of light: evidences of photon behaviour contradicting known electrodynamics
We report the results of a double-slit-like experiment in the infrared range, which evidence an anomalous behaviour of photon systems under particular (energy and space) constraints. The statistical analysis of these outcomes (independently confirmed by crossing photon beam experiments in both the optical and the microwave range) shows a significant departure from the predictions of both classical and quantum electrodynamics.
physics.gen-ph
we report the results of a doubleslitlike experiment in the infrared range which evidence an anomalous behaviour of photon systems under particular energy and space constraints the statistical analysis of these outcomes independently confirmed by crossing photon beam experiments in both the optical and the microwave range shows a significant departure from the predictions of both classical and quantum electrodynamics
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710.4874
Decays of the Littlest Higgs Z_H and the Onset of Strong Dynamics
The Little Higgs mechanism, as realized in various models, requires a set of new massive gauge bosons, some of which mix with gauge bosons of the Standard Model. For a range of mixing angles the coupling of gauge bosons to scalars can become strong, ultimately resulting in a breakdown of perturbative calculation. This phenomenon is studied in the Littlest Higgs model, where the approach to strong dynamics is characterized by increasing tree-level decay widths of the neutral Z_H boson to lighter gauge bosons plus multiple scalars. These increasing widths suggest a distinctive qualitative collider signature for the approach to the strong coupling regime of large Higgs and other scalar multiplicities. In this work we catalog the kinematically allowed three-body decays of the Z_H, and calculate the partial width of the process Z_H to Z_L H H. This partial width is found to be larger than the comparable two-body decay Z_H to Z_L H for values of the SU(2) mixing angle cosine(theta) less than 0.13, indicating divergence of the littlest Higgs sigma field expansion at values of cosine(theta) larger than a simple parametric calculation would suggest. Additionally, we present analytical expressions for all two-body decays of the Littlest Higgs Z_H gauge boson, including the effects of all final-state masses.
hep-ph
the little higgs mechanism as realized in various models requires a set of new massive gauge bosons some of which mix with gauge bosons of the standard model for a range of mixing angles the coupling of gauge bosons to scalars can become strong ultimately resulting in a breakdown of perturbative calculation this phenomenon is studied in the littlest higgs model where the approach to strong dynamics is characterized by increasing treelevel decay widths of the neutral z_h boson to lighter gauge bosons plus multiple scalars these increasing widths suggest a distinctive qualitative collider signature for the approach to the strong coupling regime of large higgs and other scalar multiplicities in this work we catalog the kinematically allowed threebody decays of the z_h and calculate the partial width of the process z_h to z_l h h this partial width is found to be larger than the comparable twobody decay z_h to z_l h for values of the su2 mixing angle cosinetheta less than 013 indicating divergence of the littlest higgs sigma field expansion at values of cosinetheta larger than a simple parametric calculation would suggest additionally we present analytical expressions for all twobody decays of the littlest higgs z_h gauge boson including the effects of all finalstate masses
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710.4875
A discrete version and stability of Brunn Minkowski inequality
In the first part of the paper, we define an approximated Brunn-Minkowski inequality which generalizes the classical one for length spaces. Our new definition based only on distance properties allows us also to deal with discrete spaces. Then we show the stability of our new inequality under a convergence of metric measure spaces. This result gives as a corollary the stability of the classical Brunn-Minkowski inequality for geodesic spaces. The proof of this stability was done for different inequalities (curvature dimension inequality, metric contraction property) but as far as we know not for the Brunn-Minkowski one. In the second part of the paper, we show that every metric measure space satisfying classical Brunn-Minkowski inequality can be approximated by discrete spaces with some approximated Brunn-Minkowski inequalities.
math.MG
in the first part of the paper we define an approximated brunnminkowski inequality which generalizes the classical one for length spaces our new definition based only on distance properties allows us also to deal with discrete spaces then we show the stability of our new inequality under a convergence of metric measure spaces this result gives as a corollary the stability of the classical brunnminkowski inequality for geodesic spaces the proof of this stability was done for different inequalities curvature dimension inequality metric contraction property but as far as we know not for the brunnminkowski one in the second part of the paper we show that every metric measure space satisfying classical brunnminkowski inequality can be approximated by discrete spaces with some approximated brunnminkowski inequalities
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710.4876
D-term Uplifted Racetrack Inflation
It is shown that racetrack inflation can be implemented in a moduli stabilisation scenario with a supersymmetric uplifting D-term. The resulting model is completely described by an effective supergravity theory, in contrast to the original racetrack models. We study the inflationary dynamics and show that the gaugino condensates vary during inflation. The resulting spectral index is n_s = 0.95 as in the original racetrack inflation model. Hence extra fields do not appear to alter the predictions of the model. An equivalent, simplified model with just a single field is presented.
hep-th hep-ph
it is shown that racetrack inflation can be implemented in a moduli stabilisation scenario with a supersymmetric uplifting dterm the resulting model is completely described by an effective supergravity theory in contrast to the original racetrack models we study the inflationary dynamics and show that the gaugino condensates vary during inflation the resulting spectral index is n_s 095 as in the original racetrack inflation model hence extra fields do not appear to alter the predictions of the model an equivalent simplified model with just a single field is presented
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710.4877
Moduli stabilization in (string) model building: gauge fluxes and loops
We discuss the moduli stabilization arising in the presence of gauge fluxes, R-symmetry twists and non-perturbative effects in the context of 6-dimensional supergravity models. We show how the presence of D-terms, due to the gauge fluxes, is compatible with gaugino condensation, and that the two effects, combined with the R-symmetry twist, do stabilize all the Kaehler moduli present in the model, in the spirit of KKLT. We also calculate the flux-induced one-loop correction to the scalar potential coming from charged hypermultiplets, and find that it does not destabilize the minimum.
hep-th
we discuss the moduli stabilization arising in the presence of gauge fluxes rsymmetry twists and nonperturbative effects in the context of 6dimensional supergravity models we show how the presence of dterms due to the gauge fluxes is compatible with gaugino condensation and that the two effects combined with the rsymmetry twist do stabilize all the kaehler moduli present in the model in the spirit of kklt we also calculate the fluxinduced oneloop correction to the scalar potential coming from charged hypermultiplets and find that it does not destabilize the minimum
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710.4878
Discovery Potential for the SM Higgs Boson in the Inclusive Search Channels
This paper gives an overview of the potential to discover a Standard Model Higgs Boson in the inclusive search channels at the ATLAS and CMS experiments at the LHC. The most important decay modes, $H \to \gamma \gamma$, $H \to WW \to ll\nu\nu$ and $H \to ZZ \to 4l$ are described and a summary of recently published analyses using realistic detector simulations is presented.
hep-ex
this paper gives an overview of the potential to discover a standard model higgs boson in the inclusive search channels at the atlas and cms experiments at the lhc the most important decay modes h to gamma gamma h to ww to llnunu and h to zz to 4l are described and a summary of recently published analyses using realistic detector simulations is presented
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710.4879
QT-Symmetry and Weak Pseudo-Hermiticity
For an invertible (bounded) linear operator Q acting in a Hilbert space ${\cal H}$, we consider the consequences of the QT-symmetry of a non-Hermitian Hamiltonian $H:{\cal H}\to{\cal H}$ where T is the time-reversal operator. If H is symmetric in the sense that ${\cal T} H^\dagger {\cal T}=H$, then QT-symmetry is equivalent to Q^{-1}-weak-pseudo-Hermiticity. But in general this equivalence does not hold. We show this using some specific examples. Among these is a large class of non-PT-symmetric Hamiltonians that share the spectral properties of PT-symmetric Hamiltonians.
quant-ph hep-th math-ph math.MP
for an invertible bounded linear operator q acting in a hilbert space cal h we consider the consequences of the qtsymmetry of a nonhermitian hamiltonian hcal htocal h where t is the timereversal operator if h is symmetric in the sense that cal t hdagger cal th then qtsymmetry is equivalent to q1weakpseudohermiticity but in general this equivalence does not hold we show this using some specific examples among these is a large class of nonptsymmetric hamiltonians that share the spectral properties of ptsymmetric hamiltonians
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710.488
Perturbative and non-perturbative aspects of QED_{3}
In this work we review various findings in the planar quantum physics with the special emphasis on the two-component quantum electrodynamics in three-dimensional spacetime (QED_{3}) with the Chern-Simons (CS) term. First the classical electrodynamics is briefly outlined. Then we construct and classify the unitary irreducible representations of the Poincare group and connect them to various covariant fields. Subtleties with discrete symmetries arising in QED_{3} are also discussed. Quantization of the free gauge field with and without the CS term is performed in Coulomb gauge. Subsequently we discuss the ultraviolet behavior of the theory in perturbative regime and perform some one-loop calculations. The induced CS term is examined using the effective action formalism. The non-relativistic electron-electron interactions are considered in the Maxwell-Chern-Simons theory and the possibility of bound states is briefly discussed. We also examine the non-relativistic scattering of two anyons in the pure CS theory to one-loop order.
hep-ph cond-mat.other
in this work we review various findings in the planar quantum physics with the special emphasis on the twocomponent quantum electrodynamics in threedimensional spacetime qed_3 with the chernsimons cs term first the classical electrodynamics is briefly outlined then we construct and classify the unitary irreducible representations of the poincare group and connect them to various covariant fields subtleties with discrete symmetries arising in qed_3 are also discussed quantization of the free gauge field with and without the cs term is performed in coulomb gauge subsequently we discuss the ultraviolet behavior of the theory in perturbative regime and perform some oneloop calculations the induced cs term is examined using the effective action formalism the nonrelativistic electronelectron interactions are considered in the maxwellchernsimons theory and the possibility of bound states is briefly discussed we also examine the nonrelativistic scattering of two anyons in the pure cs theory to oneloop order
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710.4881
Inclusive charged-current neutrino-nucleus reactions calculated with the relativistic quasiparticle random phase approximation
Inclusive neutrino-nucleus cross sections are calculated using a consistent relativistic mean-field theoretical framework. The weak lepton-hadron interaction is expressed in the standard current-current form, the nuclear ground state is described with the relativistic Hartree-Bogoliubov model, and the relevant transitions to excited nuclear states are calculated in the relativistic quasiparticle random phase approximation. Illustrative test calculations are performed for charged-current neutrino reactions on $^{12}$C, $^{16}$O, $^{56}$Fe, and $^{208}$Pb, and results compared with previous studies and available data. Using the experimental neutrino fluxes, the averaged cross sections are evaluated for nuclei of interest for neutrino detectors. We analyze the total neutrino-nucleus cross sections, and the evolution of the contribution of the different multipole excitations as a function of neutrino energy. The cross sections for reactions of supernova neutrinos on $^{16}$O and $^{208}$Pb target nuclei are analyzed as functions of the temperature and chemical potential.
nucl-th astro-ph.SR physics.ins-det
inclusive neutrinonucleus cross sections are calculated using a consistent relativistic meanfield theoretical framework the weak leptonhadron interaction is expressed in the standard currentcurrent form the nuclear ground state is described with the relativistic hartreebogoliubov model and the relevant transitions to excited nuclear states are calculated in the relativistic quasiparticle random phase approximation illustrative test calculations are performed for chargedcurrent neutrino reactions on 12c 16o 56fe and 208pb and results compared with previous studies and available data using the experimental neutrino fluxes the averaged cross sections are evaluated for nuclei of interest for neutrino detectors we analyze the total neutrinonucleus cross sections and the evolution of the contribution of the different multipole excitations as a function of neutrino energy the cross sections for reactions of supernova neutrinos on 16o and 208pb target nuclei are analyzed as functions of the temperature and chemical potential
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710.4882
Analytical and Numerical Demonstration of How the Drude Dispersive Model Satisfies Nernst's Theorem for the Casimir Entropy
In view of the current discussion on the subject, an effort is made to show very accurately both analytically and numerically how the Drude dispersive model, assuming the relaxation is nonzero at zero temperature (which is the case when impurities are present), gives consistent results for the Casimir free energy at low temperatures. Specifically, we find that the free energy consists essentially of two terms, one leading term proportional to T^2, and a next term proportional to T^{5/2}. Both these terms give rise to zero Casimir entropy as T -> 0, thus in accordance with Nernst's theorem.
quant-ph hep-th
in view of the current discussion on the subject an effort is made to show very accurately both analytically and numerically how the drude dispersive model assuming the relaxation is nonzero at zero temperature which is the case when impurities are present gives consistent results for the casimir free energy at low temperatures specifically we find that the free energy consists essentially of two terms one leading term proportional to t2 and a next term proportional to t52 both these terms give rise to zero casimir entropy as t 0 thus in accordance with nernsts theorem
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710.4883
The transiting exoplanet host star GJ 436: a test of stellar evolution models in the lower main sequence, and revised planetary parameters
Knowledge of the stellar parameters for the parent stars of transiting exoplanets is pre-requisite for establishing the planet properties themselves, and often relies on stellar evolution models. GJ 436, which is orbited by a transiting Neptune-mass object, presents a difficult case because it is an M dwarf. Stellar models in this mass regime are not as reliable as for higher mass stars, and tend to underestimate the radius. Here we use constraints from published transit light curve solutions for GJ 436 along with other spectroscopic quantities to show how the models can still be used to infer the mass and radius accurately, and at the same time allow the radius discrepancy to be estimated. Similar systems should be found during the upcoming Kepler mission, and could provide in this way valuable constraints to stellar evolution models in the lower main sequence. The stellar mass and radius of GJ 436 are M = 0.452 [-0.012,+0.014] M(Sun) and R = 0.464 [-0.011,+0.009] R(Sun), and the radius is 10% larger than predicted by the standard models, in agreement with previous results from well studied double-lined eclipsing binaries. We obtain an improved planet mass and radius of M = 23.17 +/- 0.79 M(Earth) and R = 4.22 [-0.10,+0.09] R(Earth), a density of rho = 1.69 [-0.12,+0.14] g/cm3, and an orbital semimajor axis of a = 0.02872 +/- 0.00027 AU.
astro-ph
knowledge of the stellar parameters for the parent stars of transiting exoplanets is prerequisite for establishing the planet properties themselves and often relies on stellar evolution models gj 436 which is orbited by a transiting neptunemass object presents a difficult case because it is an m dwarf stellar models in this mass regime are not as reliable as for higher mass stars and tend to underestimate the radius here we use constraints from published transit light curve solutions for gj 436 along with other spectroscopic quantities to show how the models can still be used to infer the mass and radius accurately and at the same time allow the radius discrepancy to be estimated similar systems should be found during the upcoming kepler mission and could provide in this way valuable constraints to stellar evolution models in the lower main sequence the stellar mass and radius of gj 436 are m 0452 00120014 msun and r 0464 00110009 rsun and the radius is 10 larger than predicted by the standard models in agreement with previous results from well studied doublelined eclipsing binaries we obtain an improved planet mass and radius of m 2317 079 mearth and r 422 010009 rearth a density of rho 169 012014 gcm3 and an orbital semimajor axis of a 002872 000027 au
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710.4884
Upper Bounds for the Security of two Distributed-Phase Reference Protocols of Quantum Cryptography (Coherent-One-Way and Differential-Phase-Shift)
The Differential-Phase-Shift (DPS) and the Coherent-One-Way (COW) are among the most practical protocols for quantum cryptography, and are therefore the object of fast-paced experimental developments. The assessment of their security is also a challenge for theorists: the existing tools, that allow to prove security against the most general attacks, do not apply to these two protocols in any straightforward way. We present new upper bounds for their security in the limit of large distances ($d \gtrsim 50$km with typical values in optical fibers) by considering a large class of collective attacks, namely those in which the adversary attaches ancillary quantum systems to each pulse or to each pair of pulses. We introduce also two modified versions of the COW protocol, which may prove more robust than the original one.
quant-ph
the differentialphaseshift dps and the coherentoneway cow are among the most practical protocols for quantum cryptography and are therefore the object of fastpaced experimental developments the assessment of their security is also a challenge for theorists the existing tools that allow to prove security against the most general attacks do not apply to these two protocols in any straightforward way we present new upper bounds for their security in the limit of large distances d gtrsim 50km with typical values in optical fibers by considering a large class of collective attacks namely those in which the adversary attaches ancillary quantum systems to each pulse or to each pair of pulses we introduce also two modified versions of the cow protocol which may prove more robust than the original one
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710.4885
The Weight System of the Multivariable Alexander Polynomial
We derive a formula for the weight system of the multivariable Alexander polynomial using determinants, show that it obeys known relations, and satisfies some of the same relations as the single variable polynomial.
math.GT
we derive a formula for the weight system of the multivariable alexander polynomial using determinants show that it obeys known relations and satisfies some of the same relations as the single variable polynomial
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710.4886
Network synchronization: Optimal and Pessimal Scale-Free Topologies
By employing a recently introduced optimization algorithm we explicitely design optimally synchronizable (unweighted) networks for any given scale-free degree distribution. We explore how the optimization process affects degree-degree correlations and observe a generic tendency towards disassortativity. Still, we show that there is not a one-to-one correspondence between synchronizability and disassortativity. On the other hand, we study the nature of optimally un-synchronizable networks, that is, networks whose topology minimizes the range of stability of the synchronous state. The resulting ``pessimal networks'' turn out to have a highly assortative string-like structure. We also derive a rigorous lower bound for the Laplacian eigenvalue ratio controlling synchronizability, which helps understanding the impact of degree correlations on network synchronizability.
cond-mat.dis-nn cond-mat.stat-mech
by employing a recently introduced optimization algorithm we explicitely design optimally synchronizable unweighted networks for any given scalefree degree distribution we explore how the optimization process affects degreedegree correlations and observe a generic tendency towards disassortativity still we show that there is not a onetoone correspondence between synchronizability and disassortativity on the other hand we study the nature of optimally unsynchronizable networks that is networks whose topology minimizes the range of stability of the synchronous state the resulting pessimal networks turn out to have a highly assortative stringlike structure we also derive a rigorous lower bound for the laplacian eigenvalue ratio controlling synchronizability which helps understanding the impact of degree correlations on network synchronizability
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710.4887
Sensitivity of the LHC Experiments to Extra Dimensions
This conference report briefly reviews the potential of the ATLAS and CMS experiments to discover evidence of extra dimensions.
hep-ex
this conference report briefly reviews the potential of the atlas and cms experiments to discover evidence of extra dimensions
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710.4888
Hypernuclear production by ($\gamma, K^+$) reaction within a relativistic model
Within a fully covariant model based on an effective Lagrangian picture, we investigate the hypernuclear production in photon-nucleus interaction on $ ^{16}$O target. The explicit kaon production vertex is described via creation, propagation and decay into relevant channel of $N^*$(1650), $N^*$(1710), and $N^*$(1720) intermediate baryonic resonance states in the initial interaction of the incident photon with one of the target protons. Bound state nucleon and hyperon wave functions are obtained by solving the Dirac equation. Using vertex parameters determined in the previous studies, contributions of the $N^*$(1710) baryonic resonance dominate the total production cross sections which are found to peak at photon energies below 1 GeV. The results show that photoproduction is the most appropriate means for studying the unnatural parity hypernuclear states, thus accessing the spin dependence of the hyperon-nucleon interaction.
nucl-th hep-ph nucl-ex
within a fully covariant model based on an effective lagrangian picture we investigate the hypernuclear production in photonnucleus interaction on 16o target the explicit kaon production vertex is described via creation propagation and decay into relevant channel of n1650 n1710 and n1720 intermediate baryonic resonance states in the initial interaction of the incident photon with one of the target protons bound state nucleon and hyperon wave functions are obtained by solving the dirac equation using vertex parameters determined in the previous studies contributions of the n1710 baryonic resonance dominate the total production cross sections which are found to peak at photon energies below 1 gev the results show that photoproduction is the most appropriate means for studying the unnatural parity hypernuclear states thus accessing the spin dependence of the hyperonnucleon interaction
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710.4889
Phenomenology of the 1/N$_f$ Expansion for Field Theories in Extra Dimensions
In this paper we review the properties of the 1/$N_f$ expansion in multidimensional theories. Contrary to the usual perturbative expansion it is renormalizable and contains only logarithmic divergencies. The price for it is the presence of ghost states which, however, in certain cases do not contribute to physical amplitudes. In this case the theory is unitary and one can calculate the cross-sections. As an example we consider the differential cross section of elastic $eq \to eq$ scattering in $D=7,11,...$-dimensional world. We look also for the unification of the gauge couplings in multidimensional Standard Model and its SUSY extension which takes place at energies lower than in 4 dimensions.
hep-ph
in this paper we review the properties of the 1n_f expansion in multidimensional theories contrary to the usual perturbative expansion it is renormalizable and contains only logarithmic divergencies the price for it is the presence of ghost states which however in certain cases do not contribute to physical amplitudes in this case the theory is unitary and one can calculate the crosssections as an example we consider the differential cross section of elastic eq to eq scattering in d711dimensional world we look also for the unification of the gauge couplings in multidimensional standard model and its susy extension which takes place at energies lower than in 4 dimensions
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710.489
The role of Starbursts in the Star Formation History of the Universe
This review presents a personal view of the role that starbursts play in the star formation history of the universe. It is mainly focused on the properties of nearby starburst galaxies selected for their strong UV and/or FIR emission. The similarities between local starbursts and star-forming galaxies at high redshift are also presented. I discuss too the role that LIRGs and ULIRGs and merging systems play in the formation and evolution of galaxies.
astro-ph
this review presents a personal view of the role that starbursts play in the star formation history of the universe it is mainly focused on the properties of nearby starburst galaxies selected for their strong uv andor fir emission the similarities between local starbursts and starforming galaxies at high redshift are also presented i discuss too the role that lirgs and ulirgs and merging systems play in the formation and evolution of galaxies
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710.4891
Higgs Masses and More in the Complex MSSM with FeynHiggs
We present the latest version 2.6 of FeynHiggs, a program for computing MSSM Higgs-boson masses and related observables, such as mixing angles, branching ratios, and couplings, including state-of-the-art higher-order contributions. The most important new feature is the inclusion of the fully complex O(\alpha_t\alpha_s) two-loop corrections, which enables FeynHiggs to give the most precise Higgs-mass evaluation in the complex MSSM in the Feynman-diagrammatic approach to date.
hep-ph
we present the latest version 26 of feynhiggs a program for computing mssm higgsboson masses and related observables such as mixing angles branching ratios and couplings including stateoftheart higherorder contributions the most important new feature is the inclusion of the fully complex oalpha_talpha_s twoloop corrections which enables feynhiggs to give the most precise higgsmass evaluation in the complex mssm in the feynmandiagrammatic approach to date
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710.4892
Collisional Quenching at Ultralow Energies: Controlling Efficiency with Internal State Selection
Calculations have been carried out for the vibrational quenching of excited H$_2$ molecules which collide with Li$^+$ ions at ultralow energies. The dynamics has been treated exactly using the well known quantum coupled-channel expansions over different initial vibrational levels. The overall interaction potential has been obtained from the calculations carried out earlier in our group using highly correlated ab initio methods. The results indicate that specific features of the scattering observables, e.g. the appearance of Ramsauer-Townsend minima in elastic channel cross sections and the marked increase of the cooling rates from specific initial states, can be linked to potential properties at vanishing energies (sign and size of scattering lengths) and to the presence of either virtual states or bound states. The suggestion is made that by selecting the initial state preparation of the molecular partners, the ionic interactions would be amenable to controlling quenching efficiency at ultralow energies.
physics.chem-ph
calculations have been carried out for the vibrational quenching of excited h_2 molecules which collide with li ions at ultralow energies the dynamics has been treated exactly using the well known quantum coupledchannel expansions over different initial vibrational levels the overall interaction potential has been obtained from the calculations carried out earlier in our group using highly correlated ab initio methods the results indicate that specific features of the scattering observables eg the appearance of ramsauertownsend minima in elastic channel cross sections and the marked increase of the cooling rates from specific initial states can be linked to potential properties at vanishing energies sign and size of scattering lengths and to the presence of either virtual states or bound states the suggestion is made that by selecting the initial state preparation of the molecular partners the ionic interactions would be amenable to controlling quenching efficiency at ultralow energies
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710.4893
A Multi-coloured survey of NGC 253 with XMM-Newton
There is a large body of work that has used the excellent Chandra observations of nearby galaxies with neglible low mass X-ray binary (LMXB) populations. This has culminated in a ``Universal'' X-ray luminosity function (XLF) for high mass X-ray binaries (HMXBs). However, a number of methods have been used to convert from source intensities to luminosities when creating these XLFs. We have taken advantage of the XMM-Newton observations of the nearby starbursting spiral galaxy NGC 253 to test some of these methods. We find the luminosities derived from these various methods to vary by a factor of $\sim$3. We also find the most influential factor in the conversion from intensity to luminosity to be the absorption. We therefore conclude that a more consistent approach is required for determining the true Universal XLF for HMXBs. Ideally, this would involve individual spectral fitting of each X-ray source. Certainly, the line-of-sight absorption should be determined from the observations rather than assuming Galactic absorption. We find the best approach for obtaining an XLF from low-count data to be the splitting of the X-ray sources into two or more intensity intervals, and obtaining a conversion from intensity to flux for each group from spectral modelling of the summed spectrum of that group.
astro-ph
there is a large body of work that has used the excellent chandra observations of nearby galaxies with neglible low mass xray binary lmxb populations this has culminated in a universal xray luminosity function xlf for high mass xray binaries hmxbs however a number of methods have been used to convert from source intensities to luminosities when creating these xlfs we have taken advantage of the xmmnewton observations of the nearby starbursting spiral galaxy ngc 253 to test some of these methods we find the luminosities derived from these various methods to vary by a factor of sim3 we also find the most influential factor in the conversion from intensity to luminosity to be the absorption we therefore conclude that a more consistent approach is required for determining the true universal xlf for hmxbs ideally this would involve individual spectral fitting of each xray source certainly the lineofsight absorption should be determined from the observations rather than assuming galactic absorption we find the best approach for obtaining an xlf from lowcount data to be the splitting of the xray sources into two or more intensity intervals and obtaining a conversion from intensity to flux for each group from spectral modelling of the summed spectrum of that group
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710.4894
The EPR experiment in the energy-based stochastic reduction framework
We consider the EPR experiment in the energy-based stochastic reduction framework. A gedanken set up is constructed to model the interaction of the particles with the measurement devices. The evolution of particles' density matrix is analytically derived. We compute the dependence of the disentanglement rate on the parameters of the model, and study the dependence of the outcome probabilities on the noise trajectories. Finally, we argue that these trajectories can be regarded as non-local hidden variables.
quant-ph
we consider the epr experiment in the energybased stochastic reduction framework a gedanken set up is constructed to model the interaction of the particles with the measurement devices the evolution of particles density matrix is analytically derived we compute the dependence of the disentanglement rate on the parameters of the model and study the dependence of the outcome probabilities on the noise trajectories finally we argue that these trajectories can be regarded as nonlocal hidden variables
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710.4895
Plasmonic Resonant Optical Nanoswitch
We examine here the anomalous optical response of a nanosphere composed of two conjoined hemispheres of different materials, one of them being plasmonic. At the internal resonance, we show how the light interaction becomes dramatically dependent on the polarization of the local electric field exciting the particle. In particular, its response may be varied from the one of an ideal perfect electric to a perfect magnetic homogeneous sphere through all the possible intermediate stages, by a simple 90 deg rotation. Applications as optical switch and as a novel nanocircuit element are envisioned.
cond-mat.mtrl-sci
we examine here the anomalous optical response of a nanosphere composed of two conjoined hemispheres of different materials one of them being plasmonic at the internal resonance we show how the light interaction becomes dramatically dependent on the polarization of the local electric field exciting the particle in particular its response may be varied from the one of an ideal perfect electric to a perfect magnetic homogeneous sphere through all the possible intermediate stages by a simple 90 deg rotation applications as optical switch and as a novel nanocircuit element are envisioned
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710.4896
LAW: A Tool for Improved Productivity with High-Performance Linear Algebra Codes. Design and Applications
LAPACK and ScaLAPACK are arguably the defacto standard libraries among the scientific community for solving linear algebra problems on sequential, shared-memory and distributed-memory architectures. While ease of use was a major design goal for the ScaLAPACK project; with respect to its predecessor LAPACK; it is still a non-trivial exercise to develop a new code or modify an existing LAPACK code to exploit processor grids, distributed-array descriptors and the associated distributed-memory ScaLAPACK/PBLAS routines. In this paper, we introduce what we believe will be an invaluable development tool for the scientific code developer, which exploits ad-hoc polymorphism, derived-types, optional arguments, overloaded operators and conditional compilation in Fortran 95, to provide wrappers to a subset of common linear algebra kernels. These wrappers are introduced to facilitate the abstraction of low-level details which are irrelevant to the science being performed, such as target platform and execution model. By exploiting this high-level library interface, only a single code source is required with mapping onto a diverse range of execution models performed at link-time with no user modification. We conclude with a case study whereby we describe application of the LAW library in the implementation of the well-known Chebyshev Matrix Exponentiation algorithm for Hermitian matrices.
physics.comp-ph
lapack and scalapack are arguably the defacto standard libraries among the scientific community for solving linear algebra problems on sequential sharedmemory and distributedmemory architectures while ease of use was a major design goal for the scalapack project with respect to its predecessor lapack it is still a nontrivial exercise to develop a new code or modify an existing lapack code to exploit processor grids distributedarray descriptors and the associated distributedmemory scalapackpblas routines in this paper we introduce what we believe will be an invaluable development tool for the scientific code developer which exploits adhoc polymorphism derivedtypes optional arguments overloaded operators and conditional compilation in fortran 95 to provide wrappers to a subset of common linear algebra kernels these wrappers are introduced to facilitate the abstraction of lowlevel details which are irrelevant to the science being performed such as target platform and execution model by exploiting this highlevel library interface only a single code source is required with mapping onto a diverse range of execution models performed at linktime with no user modification we conclude with a case study whereby we describe application of the law library in the implementation of the wellknown chebyshev matrix exponentiation algorithm for hermitian matrices
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710.4897
Nuclear PDFs from neutrino deep inelastic scattering
We study nuclear effects in charged current deep inelastic neutrino-iron scattering in the frame-work of a chi^2 analysis of parton distribution functions. We extract a set of iron PDFs and show that under reasonable assumptions it is possible to constrain the valence, light sea and strange quark distributions. Our iron PDFs are used to compute x_{Bj}-dependent and Q^2-dependent nuclear correction factors for iron structure functions which are required in global analyses of free nucleon PDFs. We compare our results with nuclear correction factors from neutrino-nucleus scattering models and correction factors for charged lepton-iron scattering. We find that, except for very high x_{Bj}, our correction factors differ in both shape and magnitude from the correction factors of the models and charged-lepton scattering.
hep-ph
we study nuclear effects in charged current deep inelastic neutrinoiron scattering in the framework of a chi2 analysis of parton distribution functions we extract a set of iron pdfs and show that under reasonable assumptions it is possible to constrain the valence light sea and strange quark distributions our iron pdfs are used to compute x_bjdependent and q2dependent nuclear correction factors for iron structure functions which are required in global analyses of free nucleon pdfs we compare our results with nuclear correction factors from neutrinonucleus scattering models and correction factors for charged leptoniron scattering we find that except for very high x_bj our correction factors differ in both shape and magnitude from the correction factors of the models and chargedlepton scattering
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710.4898
Report on an all-sky LIGO search for periodic gravitational waves in the S4 data
We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50-1000 Hz and having a negative frequency time derivative with magnitude between zero and $10^{-8}$ Hz/s. Data from the fourth LIGO science run have been used in this search. Three different semi-coherent methods of summing strain power were applied. Observing no evidence for periodic gravitational radiation, we report upper limits on strain amplitude and interpret these limits to constrain radiation from rotating neutron stars.
gr-qc
we report on an allsky search with the ligo detectors for periodic gravitational waves in the frequency range 501000 hz and having a negative frequency time derivative with magnitude between zero and 108 hzs data from the fourth ligo science run have been used in this search three different semicoherent methods of summing strain power were applied observing no evidence for periodic gravitational radiation we report upper limits on strain amplitude and interpret these limits to constrain radiation from rotating neutron stars
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710.4899
Derivation via free energy conservation constraints of gyrofluid equations with finite-gyroradius electromagnetic nonlinearities
The derivation of electromagnetic gyrofluid equations is made systematic by using the Hermite polynomial form of the underlying delta-f gyrokinetic distribution function. The gyrokinetic free-energy functional is explicitly used to set up the model. The gyrofluid free energy follows directly. The interaction term in the gyrokinetic Lagrangian is used to obtain the gyrofluid counterpart, from which the polarisation equation follows. One closure rule is decided for taking moments over the kinetic gyroaveraging operator. These steps fix the rest of the derivation of the conservative part of the gyrofluid equations. Dissipation is then added in a form to obtain positive definite dissipation and to obtain the collisional fluid equations in their appropriate limit. Existing results are recovered, with the addition of a completely consistent model for finite gyroradius effects in the nonlinearities responsible for magnetic reconnection.
physics.plasm-ph
the derivation of electromagnetic gyrofluid equations is made systematic by using the hermite polynomial form of the underlying deltaf gyrokinetic distribution function the gyrokinetic freeenergy functional is explicitly used to set up the model the gyrofluid free energy follows directly the interaction term in the gyrokinetic lagrangian is used to obtain the gyrofluid counterpart from which the polarisation equation follows one closure rule is decided for taking moments over the kinetic gyroaveraging operator these steps fix the rest of the derivation of the conservative part of the gyrofluid equations dissipation is then added in a form to obtain positive definite dissipation and to obtain the collisional fluid equations in their appropriate limit existing results are recovered with the addition of a completely consistent model for finite gyroradius effects in the nonlinearities responsible for magnetic reconnection
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710.49
Chiral Symmetry Breaking in Brane Models
We discuss the chiral symmetry breaking in general intersecting Dq/Dp brane models consisting of N_c Dq-branes and a single Dp-brane with an s-dimensional intersection. There exists a QCD-like theory localized at the intersection and the Dq/Dp model gives a holographic description of it. The rotational symmetry of directions transverse to both of the Dq and Dp-branes can be identified with a chiral symmetry, which is non-Abelian for certain cases. The asymptotic distance between the Dq-branes and the Dp-brane corresponds to a quark mass. By studying the probe Dp-brane dynamics in a Dq-brane background in the near horizon and large N_c limit we find that the chiral symmetry is spontaneously broken and there appear (pseudo-)Nambu-Goldstone bosons. We also discuss the models at finite temperature.
hep-th
we discuss the chiral symmetry breaking in general intersecting dqdp brane models consisting of n_c dqbranes and a single dpbrane with an sdimensional intersection there exists a qcdlike theory localized at the intersection and the dqdp model gives a holographic description of it the rotational symmetry of directions transverse to both of the dq and dpbranes can be identified with a chiral symmetry which is nonabelian for certain cases the asymptotic distance between the dqbranes and the dpbrane corresponds to a quark mass by studying the probe dpbrane dynamics in a dqbrane background in the near horizon and large n_c limit we find that the chiral symmetry is spontaneously broken and there appear pseudonambugoldstone bosons we also discuss the models at finite temperature
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710.4901
Optical detection of single electron spin resonance in a quantum dot
We demonstrate optically detected spin resonance of a single electron confined to a self-assembled quantum dot. The dot is rendered dark by resonant optical pumping of the spin with a coherent laser. Contrast is restored by applying a radio frequency (rf) magnetic field at the spin resonance. The scheme is sensitive even to rf fields of just a few micro-T. In one case, the spin resonance behaves exactly as a driven 3-level quantum system (a lambda-system) with weak damping. In another, the dot exhibits remarkably strong (67% signal recovery) and narrow (0.34 MHz) spin resonances with fluctuating resonant positions, evidence of unusual dynamic processes of non-Markovian character.
cond-mat.other
we demonstrate optically detected spin resonance of a single electron confined to a selfassembled quantum dot the dot is rendered dark by resonant optical pumping of the spin with a coherent laser contrast is restored by applying a radio frequency rf magnetic field at the spin resonance the scheme is sensitive even to rf fields of just a few microt in one case the spin resonance behaves exactly as a driven 3level quantum system a lambdasystem with weak damping in another the dot exhibits remarkably strong 67 signal recovery and narrow 034 mhz spin resonances with fluctuating resonant positions evidence of unusual dynamic processes of nonmarkovian character
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710.4902
The Lifshitz-Khalatnikov Kasner index parametrization and the Weyl Tensor
The scale invariant Petrov classification of the Weyl tensor is linked to the scale invariant combination of the Kasner index constraints, and the Lifshitz-Khalatnikov Kasner index parametrization scheme turns out to be a natural way of adapting to this symmetry, while hiding the permutation symmetry that is instead made manifest by the Misner parametrization scheme. While not so interesting for the Kasner spacetime by itself, it gives a geometrical meaning to the famous Kasner map transitioning between Kasner epochs and Kasner eras, equivalently bouncing between curvature walls, in the BLK-Mixmaster dynamics exhibited by spatially homogeneous cosmologies approaching the initial cosmological singularity and the inhomogeneous generalization of this dynamics.
gr-qc
the scale invariant petrov classification of the weyl tensor is linked to the scale invariant combination of the kasner index constraints and the lifshitzkhalatnikov kasner index parametrization scheme turns out to be a natural way of adapting to this symmetry while hiding the permutation symmetry that is instead made manifest by the misner parametrization scheme while not so interesting for the kasner spacetime by itself it gives a geometrical meaning to the famous kasner map transitioning between kasner epochs and kasner eras equivalently bouncing between curvature walls in the blkmixmaster dynamics exhibited by spatially homogeneous cosmologies approaching the initial cosmological singularity and the inhomogeneous generalization of this dynamics
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710.4903
Anonymous Networking amidst Eavesdroppers
The problem of security against timing based traffic analysis in wireless networks is considered in this work. An analytical measure of anonymity in eavesdropped networks is proposed using the information theoretic concept of equivocation. For a physical layer with orthogonal transmitter directed signaling, scheduling and relaying techniques are designed to maximize achievable network performance for any given level of anonymity. The network performance is measured by the achievable relay rates from the sources to destinations under latency and medium access constraints. In particular, analytical results are presented for two scenarios: For a two-hop network with maximum anonymity, achievable rate regions for a general m x 1 relay are characterized when nodes generate independent Poisson transmission schedules. The rate regions are presented for both strict and average delay constraints on traffic flow through the relay. For a multihop network with an arbitrary anonymity requirement, the problem of maximizing the sum-rate of flows (network throughput) is considered. A selective independent scheduling strategy is designed for this purpose, and using the analytical results for the two-hop network, the achievable throughput is characterized as a function of the anonymity level. The throughput-anonymity relation for the proposed strategy is shown to be equivalent to an information theoretic rate-distortion function.
cs.IT math.IT
the problem of security against timing based traffic analysis in wireless networks is considered in this work an analytical measure of anonymity in eavesdropped networks is proposed using the information theoretic concept of equivocation for a physical layer with orthogonal transmitter directed signaling scheduling and relaying techniques are designed to maximize achievable network performance for any given level of anonymity the network performance is measured by the achievable relay rates from the sources to destinations under latency and medium access constraints in particular analytical results are presented for two scenarios for a twohop network with maximum anonymity achievable rate regions for a general m x 1 relay are characterized when nodes generate independent poisson transmission schedules the rate regions are presented for both strict and average delay constraints on traffic flow through the relay for a multihop network with an arbitrary anonymity requirement the problem of maximizing the sumrate of flows network throughput is considered a selective independent scheduling strategy is designed for this purpose and using the analytical results for the twohop network the achievable throughput is characterized as a function of the anonymity level the throughputanonymity relation for the proposed strategy is shown to be equivalent to an information theoretic ratedistortion function
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710.4904
Density Functional Theory for the Photoionization Dynamics of Uracil
Photoionization dynamics of the RNA base Uracil is studied in the framework of Density Functional Theory (DFT). The photoionization calculations take advantage of a newly developed parallel version of a multicentric approach to the calculation of the electronic continuum spectrum which uses a set of B-spline radial basis functions and a Kohn-Sham density functional hamiltonian. Both valence and core ionizations are considered. Scattering resonances in selected single-particle ionization channels are classified by the symmetry of the resonant state and the peak energy position in the photoelectron kinetic energy scale; the present results highlight once more the site specificity of core ionization processes. We further suggest that the resonant structures previously characterized in low-energy electron collision experiments are partly shifted below threshold by the photoionization processes. A critical evaluation of the theoretical results providing a guide for future experimental work on similar biosystems.
physics.chem-ph
photoionization dynamics of the rna base uracil is studied in the framework of density functional theory dft the photoionization calculations take advantage of a newly developed parallel version of a multicentric approach to the calculation of the electronic continuum spectrum which uses a set of bspline radial basis functions and a kohnsham density functional hamiltonian both valence and core ionizations are considered scattering resonances in selected singleparticle ionization channels are classified by the symmetry of the resonant state and the peak energy position in the photoelectron kinetic energy scale the present results highlight once more the site specificity of core ionization processes we further suggest that the resonant structures previously characterized in lowenergy electron collision experiments are partly shifted below threshold by the photoionization processes a critical evaluation of the theoretical results providing a guide for future experimental work on similar biosystems
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710.4905
Distributed Source Coding in the Presence of Byzantine Sensors
The distributed source coding problem is considered when the sensors, or encoders, are under Byzantine attack; that is, an unknown group of sensors have been reprogrammed by a malicious intruder to undermine the reconstruction at the fusion center. Three different forms of the problem are considered. The first is a variable-rate setup, in which the decoder adaptively chooses the rates at which the sensors transmit. An explicit characterization of the variable-rate achievable sum rates is given for any number of sensors and any groups of traitors. The converse is proved constructively by letting the traitors simulate a fake distribution and report the generated values as the true ones. This fake distribution is chosen so that the decoder cannot determine which sensors are traitors while maximizing the required rate to decode every value. Achievability is proved using a scheme in which the decoder receives small packets of information from a sensor until its message can be decoded, before moving on to the next sensor. The sensors use randomization to choose from a set of coding functions, which makes it probabilistically impossible for the traitors to cause the decoder to make an error. Two forms of the fixed-rate problem are considered, one with deterministic coding and one with randomized coding. The achievable rate regions are given for both these problems, and it is shown that lower rates can be achieved with randomized coding.
cs.IT math.IT
the distributed source coding problem is considered when the sensors or encoders are under byzantine attack that is an unknown group of sensors have been reprogrammed by a malicious intruder to undermine the reconstruction at the fusion center three different forms of the problem are considered the first is a variablerate setup in which the decoder adaptively chooses the rates at which the sensors transmit an explicit characterization of the variablerate achievable sum rates is given for any number of sensors and any groups of traitors the converse is proved constructively by letting the traitors simulate a fake distribution and report the generated values as the true ones this fake distribution is chosen so that the decoder cannot determine which sensors are traitors while maximizing the required rate to decode every value achievability is proved using a scheme in which the decoder receives small packets of information from a sensor until its message can be decoded before moving on to the next sensor the sensors use randomization to choose from a set of coding functions which makes it probabilistically impossible for the traitors to cause the decoder to make an error two forms of the fixedrate problem are considered one with deterministic coding and one with randomized coding the achievable rate regions are given for both these problems and it is shown that lower rates can be achieved with randomized coding
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710.4906
Systematics and background suppression in the KATRIN experiment
Recent neutrino mass experiments at Mainz and Troitsk using tritium beta-decay have reached their sensitivity potential, yielding upper limits of about 2 eV/c^2 for the electron antineutrino mass. The KArlsruhe TRItium Neutrino experiment (KATRIN), designed to reach a sensitivity of 0.2 eV/c^2 (90% C.L.), will improve the signal rate by a factor of about 100 with respect to previous experiments while maintaining the same low background level at an enhanced energy resolution of 0.93 eV of the spectrometer which is scaled up by a factor of 10 in linear dimensions. This low background rate can only be achieved by active and passive reduction of the background components induced by the spectrometer itself and in the detector region. Furthermore, sources of systematic errors such as energy losses inside the tritium source or fluctuations of the energy scale of the spectrometer need to be carefully controlled and analysed. An overview of KATRIN's method to reduce the background rate and to determine the systematics as well as the sensitivity on the neutrino mass will be presented.
hep-ex
recent neutrino mass experiments at mainz and troitsk using tritium betadecay have reached their sensitivity potential yielding upper limits of about 2 evc2 for the electron antineutrino mass the karlsruhe tritium neutrino experiment katrin designed to reach a sensitivity of 02 evc2 90 cl will improve the signal rate by a factor of about 100 with respect to previous experiments while maintaining the same low background level at an enhanced energy resolution of 093 ev of the spectrometer which is scaled up by a factor of 10 in linear dimensions this low background rate can only be achieved by active and passive reduction of the background components induced by the spectrometer itself and in the detector region furthermore sources of systematic errors such as energy losses inside the tritium source or fluctuations of the energy scale of the spectrometer need to be carefully controlled and analysed an overview of katrins method to reduce the background rate and to determine the systematics as well as the sensitivity on the neutrino mass will be presented
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710.4907
U-Duality and the Compactified Gauss-Bonnet Term
We present the complete toroidal compactification of the Gauss-Bonnet Lagrangian from D dimensions to (D-n) dimensions. Our goal is to investigate the resulting action from the point of view of the "U-duality" symmetry SL(n+1,R) which is present in the tree-level Lagrangian when D-n=3. The analysis builds upon and extends the investigation of the paper [arXiv:0706.1183], by computing in detail the full structure of the compactified Gauss-Bonnet term, including the contribution from the dilaton exponents. We analyze these exponents using the representation theory of the Lie algebra sl(n+1,R) and determine which representation seems to be the relevant one for quadratic curvature corrections. By interpreting the result of the compactification as a leading term in a large volume expansion of an SL(n+1,Z)-invariant action, we conclude that the overall exponential dilaton factor should not be included in the representation structure. As a consequence, all dilaton exponents correspond to weights of sl(n+1,R), which, nevertheless, remain on the positive side of the root lattice.
hep-th
we present the complete toroidal compactification of the gaussbonnet lagrangian from d dimensions to dn dimensions our goal is to investigate the resulting action from the point of view of the uduality symmetry sln1r which is present in the treelevel lagrangian when dn3 the analysis builds upon and extends the investigation of the paper arxiv07061183 by computing in detail the full structure of the compactified gaussbonnet term including the contribution from the dilaton exponents we analyze these exponents using the representation theory of the lie algebra sln1r and determine which representation seems to be the relevant one for quadratic curvature corrections by interpreting the result of the compactification as a leading term in a large volume expansion of an sln1zinvariant action we conclude that the overall exponential dilaton factor should not be included in the representation structure as a consequence all dilaton exponents correspond to weights of sln1r which nevertheless remain on the positive side of the root lattice
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710.4908
Physics at SuperB
Flavour will play a crucial role in understanding physics beyond the Standard Model. Progress in developing a future programme to investigate this central area of particle physics has recently passed a milestone, with the completion of the conceptual design report for SuperB, a very high luminosity, asymmetric e+e- collider. This article summarizes the important role of SuperB in understanding new physics in the LHC era.
hep-ex
flavour will play a crucial role in understanding physics beyond the standard model progress in developing a future programme to investigate this central area of particle physics has recently passed a milestone with the completion of the conceptual design report for superb a very high luminosity asymmetric ee collider this article summarizes the important role of superb in understanding new physics in the lhc era
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710.4909
The origin of galactic cosmic rays
The origin of galactic cosmic rays is one of the most interesting unsolved problems in astroparticle physics. Experimentally, the problem is attacked by a multi-disciplinary effort, namely by direct measurements of cosmic rays above the atmosphere, by air shower observations, and by the detection of TeV $\gamma$ rays. Recent experimental results are presented and their implications on the contemporary understanding of the origin of galactic cosmic rays are discussed.
astro-ph
the origin of galactic cosmic rays is one of the most interesting unsolved problems in astroparticle physics experimentally the problem is attacked by a multidisciplinary effort namely by direct measurements of cosmic rays above the atmosphere by air shower observations and by the detection of tev gamma rays recent experimental results are presented and their implications on the contemporary understanding of the origin of galactic cosmic rays are discussed
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710.491
Generic Absorbing Transition in Coevolution Dynamics
We study a coevolution voter model on a network that evolves according to the state of the nodes. In a single update, a link between opposite-state nodes is rewired with probability $p$, while with probability $1-p$ one of the nodes takes its neighbor's state. A mean-field approximation reveals an absorbing transition from an active to a frozen phase at a critical value $p_c=\frac{\mu-2}{\mu-1}$ that only depends on the average degree $\mu$ of the network. The approach to the final state is characterized by a time scale that diverges at the critical point as $\tau \sim |p_c-p|^{-1}$. We find that the active and frozen phases correspond to a connected and a fragmented network respectively. We show that the transition in finite-size systems can be seen as the sudden change in the trajectory of an equivalent random walk at the critical rewiring rate $p_c$, highlighting the fact that the mechanism behind the transition is a competition between the rates at which the network and the state of the nodes evolve.
physics.soc-ph cond-mat.stat-mech
we study a coevolution voter model on a network that evolves according to the state of the nodes in a single update a link between oppositestate nodes is rewired with probability p while with probability 1p one of the nodes takes its neighbors state a meanfield approximation reveals an absorbing transition from an active to a frozen phase at a critical value p_cfracmu2mu1 that only depends on the average degree mu of the network the approach to the final state is characterized by a time scale that diverges at the critical point as tau sim p_cp1 we find that the active and frozen phases correspond to a connected and a fragmented network respectively we show that the transition in finitesize systems can be seen as the sudden change in the trajectory of an equivalent random walk at the critical rewiring rate p_c highlighting the fact that the mechanism behind the transition is a competition between the rates at which the network and the state of the nodes evolve
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710.4911
Social Media as Windows on the Social Life of the Mind
This is a programmatic paper, marking out two directions in which the study of social media can contribute to broader problems of social science: understanding cultural evolution and understanding collective cognition. Under the first heading, I discuss some difficulties with the usual, adaptationist explanations of cultural phenomena, alternative explanations involving network diffusion effects, and some ways these could be tested using social-media data. Under the second I describe some of the ways in which social media could be used to study how the social organization of an epistemic community supports its collective cognitive performance.
cs.CY physics.soc-ph
this is a programmatic paper marking out two directions in which the study of social media can contribute to broader problems of social science understanding cultural evolution and understanding collective cognition under the first heading i discuss some difficulties with the usual adaptationist explanations of cultural phenomena alternative explanations involving network diffusion effects and some ways these could be tested using socialmedia data under the second i describe some of the ways in which social media could be used to study how the social organization of an epistemic community supports its collective cognitive performance
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710.4912
Near-horizon microstates of the D1-D5-P black hole
We construct probe solutions in the attractor background of the five-dimensional D1-D5-P black hole which represent near-horizon microstates in the limit of large D1-charge. These generalize the corresponding solutions considered by Gaiotto, Strominger and Yin for the 4-dimensional D0-D4 black hole. Using U-duality and a 4D-5D connection, we argue that the relevant configurations are bound states of D1-branes that have expanded through the Myers effect to form a Kaluza-Klein monopole wrapping the black hole horizon. We show that these branes experience a magnetic field on their moduli space, and that the degeneracy of lowest Landau levels reproduces the Bekenstein-Hawking entropy.
hep-th
we construct probe solutions in the attractor background of the fivedimensional d1d5p black hole which represent nearhorizon microstates in the limit of large d1charge these generalize the corresponding solutions considered by gaiotto strominger and yin for the 4dimensional d0d4 black hole using uduality and a 4d5d connection we argue that the relevant configurations are bound states of d1branes that have expanded through the myers effect to form a kaluzaklein monopole wrapping the black hole horizon we show that these branes experience a magnetic field on their moduli space and that the degeneracy of lowest landau levels reproduces the bekensteinhawking entropy
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710.4913
Tackling master equations with a flux loop transform
A procedure is introduced which allows to represent the dynamics of a non-equilibrium system violating detailed balance by its steady state loop fluxes. It is shown that detailed balance is restored in this representation, such that the non-equilibrium steady state follows a simple Boltzmann distribution. A novel algorithm for the construction of the steady state densities naturally emerges, as well as an expression for a 'free energy' functional which attains a minimum in the steady state.
cond-mat.stat-mech
a procedure is introduced which allows to represent the dynamics of a nonequilibrium system violating detailed balance by its steady state loop fluxes it is shown that detailed balance is restored in this representation such that the nonequilibrium steady state follows a simple boltzmann distribution a novel algorithm for the construction of the steady state densities naturally emerges as well as an expression for a free energy functional which attains a minimum in the steady state
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710.4914
Joule heating in the cooling of magnetized neutron stars
We present 2D simulations of the cooling of neutron stars with strong magnetic fields (B \geq 10^{13} G). We solve the diffusion equation in axial symmetry including the state of the art microphysics that controls the cooling such as slow/fast neutrino processes, superfluidity, as well as possible heating mechanisms. We study how the cooling curves depend on the the magnetic field strength and geometry. Special attention is given to discuss the influence of magnetic field decay. We show that Joule heating effects are very large and in some cases control the thermal evolution. We characterize the temperature anisotropy induced by the magnetic field for the early and late stages of the evolution of isolated neutron stars.
astro-ph hep-ph nucl-th
we present 2d simulations of the cooling of neutron stars with strong magnetic fields b geq 1013 g we solve the diffusion equation in axial symmetry including the state of the art microphysics that controls the cooling such as slowfast neutrino processes superfluidity as well as possible heating mechanisms we study how the cooling curves depend on the the magnetic field strength and geometry special attention is given to discuss the influence of magnetic field decay we show that joule heating effects are very large and in some cases control the thermal evolution we characterize the temperature anisotropy induced by the magnetic field for the early and late stages of the evolution of isolated neutron stars
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710.4915
Casimir energy and entropy between dissipative mirrors
We discuss the Casimir effect between two identical, parallel slabs, emphasizing the role of dissipation and temperature. Starting from quite general assumptions, we analyze the behavior of the Casimir entropy in the limit T->0 and link it to the behavior of the slab's reflection coefficients at low frequencies. We also derive a formula in terms of a sum over modes, valid for dissipative slabs that can be interpreted in terms of a damped quantum oscillator.
quant-ph
we discuss the casimir effect between two identical parallel slabs emphasizing the role of dissipation and temperature starting from quite general assumptions we analyze the behavior of the casimir entropy in the limit t0 and link it to the behavior of the slabs reflection coefficients at low frequencies we also derive a formula in terms of a sum over modes valid for dissipative slabs that can be interpreted in terms of a damped quantum oscillator
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710.4916
Impact of interactions on human dynamics
Queueing theory has been recently proposed as a framework to model the heavy tailed statistics of human activity patterns. The main predictions are the existence of a power-law distribution for the interevent time of human actions and two decay exponents $\alpha=1$ and $\alpha=3/2$. Current models lack, however, a key aspect of human dynamics, i.e. several tasks require, or are determined by, interactions between individuals. Here we introduce a minimal queueing model of human dynamics that already takes into account human-human interactions. To achieve large scale simulations we obtain a coarse-grained version of the model, allowing us to reach large interevent times and reliable scaling exponents estimations. Using this we show that the interevent distribution of interacting tasks exhibit the scaling exponents $\alpha=2$, 3/2 and a series of numerable values between 3/2 and 1. This work demonstrates that, within the context of queueing models of human dynamics, interactions change the exponent of the power-law distributed interevent times. Beyond the study of human dynamics, these results are relevant to systems where the event of interest consists of the simultaneous occurrence of two (or more) events.
physics.soc-ph cond-mat.stat-mech
queueing theory has been recently proposed as a framework to model the heavy tailed statistics of human activity patterns the main predictions are the existence of a powerlaw distribution for the interevent time of human actions and two decay exponents alpha1 and alpha32 current models lack however a key aspect of human dynamics ie several tasks require or are determined by interactions between individuals here we introduce a minimal queueing model of human dynamics that already takes into account humanhuman interactions to achieve large scale simulations we obtain a coarsegrained version of the model allowing us to reach large interevent times and reliable scaling exponents estimations using this we show that the interevent distribution of interacting tasks exhibit the scaling exponents alpha2 32 and a series of numerable values between 32 and 1 this work demonstrates that within the context of queueing models of human dynamics interactions change the exponent of the powerlaw distributed interevent times beyond the study of human dynamics these results are relevant to systems where the event of interest consists of the simultaneous occurrence of two or more events
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710.4917
Drip Paintings and Fractal Analysis
It has been claimed [1-6] that fractal analysis can be applied to unambiguously characterize works of art such as the drip paintings of Jackson Pollock. This academic issue has become of more general interest following the recent discovery of a cache of disputed Pollock paintings. We definitively demonstrate here, by analyzing paintings by Pollock and others, that fractal criteria provide no information about artistic authenticity. This work has also led to two new results in fractal analysis of more general scientific significance. First, the composite of two fractals is not generally scale invariant and exhibits complex multifractal scaling in the small distance asymptotic limit. Second the statistics of box-counting and related staircases provide a new way to characterize geometry and distinguish fractals from Euclidean objects.
cond-mat.stat-mech physics.soc-ph
it has been claimed 16 that fractal analysis can be applied to unambiguously characterize works of art such as the drip paintings of jackson pollock this academic issue has become of more general interest following the recent discovery of a cache of disputed pollock paintings we definitively demonstrate here by analyzing paintings by pollock and others that fractal criteria provide no information about artistic authenticity this work has also led to two new results in fractal analysis of more general scientific significance first the composite of two fractals is not generally scale invariant and exhibits complex multifractal scaling in the small distance asymptotic limit second the statistics of boxcounting and related staircases provide a new way to characterize geometry and distinguish fractals from euclidean objects
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710.4918
A precise formulation of the third law of thermodynamics
The third law of thermodynamics is formulated precisely: all points of the state space of zero temperature $\Gamma_0$ are physically adiabatically inaccessible from the state space of a simple system. In addition to implying the unattainability of absolute zero in finite time (or "by a finite number of operations"), it admits as corollary, under a continuity assumption, that all points of $\Gamma_0$ are adiabatically equivalent. We argue that the third law is universally valid for all macroscopic systems which obey the laws of quantum mechanics and/or quantum field theory. We also briefly discuss why a precise formulation of the third law for black holes remains an open problem.
math-ph gr-qc math.MP
the third law of thermodynamics is formulated precisely all points of the state space of zero temperature gamma_0 are physically adiabatically inaccessible from the state space of a simple system in addition to implying the unattainability of absolute zero in finite time or by a finite number of operations it admits as corollary under a continuity assumption that all points of gamma_0 are adiabatically equivalent we argue that the third law is universally valid for all macroscopic systems which obey the laws of quantum mechanics andor quantum field theory we also briefly discuss why a precise formulation of the third law for black holes remains an open problem
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710.4919
Harmonic cosmology: How much can we know about a universe before the big bang?
Quantum gravity may remove classical space-time singularities and thus reveal what a universe at and before the big bang could be like. In loop quantum cosmology, an exactly solvable model is available which allows one to address precise dynamical coherent states and their evolution in such a setting. It is shown here that quantum fluctuations before the big bang are generically unrelated to those after the big bang. A reliable determination of pre-big bang quantum fluctuations would require exceedingly precise observations.
gr-qc astro-ph hep-th
quantum gravity may remove classical spacetime singularities and thus reveal what a universe at and before the big bang could be like in loop quantum cosmology an exactly solvable model is available which allows one to address precise dynamical coherent states and their evolution in such a setting it is shown here that quantum fluctuations before the big bang are generically unrelated to those after the big bang a reliable determination of prebig bang quantum fluctuations would require exceedingly precise observations
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710.492
On the quasi-derivation relation for multiple zeta values
Recently, Masanobu Kaneko introduced a conjecture on an extension of the derivation relation for multiple zeta values. The goal of the present paper is to present a proof of this conjecture by reducing it to a class of relations for multiple zeta values studied by Kawashima. In addition, some algebraic aspects of the quasi-derivation operator $\partial_n^{(c)}$ on $\mathbb{Q}< x,y>$, which was defined by modeling a Hopf algebra developed by Connes and Moscovici, will be presented.
math.NT
recently masanobu kaneko introduced a conjecture on an extension of the derivation relation for multiple zeta values the goal of the present paper is to present a proof of this conjecture by reducing it to a class of relations for multiple zeta values studied by kawashima in addition some algebraic aspects of the quasiderivation operator partial_nc on mathbbq xy which was defined by modeling a hopf algebra developed by connes and moscovici will be presented
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710.4921
Weinberg like sum rules revisited
The generalized Weinberg sum rules containing the difference of isovector vector and axial-vector spectral functions saturated by both finite and infinite number of narrow resonances are considered. We summarize the status of these sum rules and analyze their overall agreement with phenomenological Lagrangians, low-energy relations, parity doubling, hadron string models, and experimental data.
hep-ph
the generalized weinberg sum rules containing the difference of isovector vector and axialvector spectral functions saturated by both finite and infinite number of narrow resonances are considered we summarize the status of these sum rules and analyze their overall agreement with phenomenological lagrangians lowenergy relations parity doubling hadron string models and experimental data
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710.4922
Constraining DM properties with SPI
Using the high-resolution spectrometer SPI on board the International Gamma-Ray Astrophysics Laboratory (INTEGRAL), we search for a spectral line produced by a dark matter(DM) particle with a mass in the range 40keV < M_DM < 14MeV, decaying in the DM halo of the Milky Way. To distinguish the DM decay line from numerous instrumental lines found in the SPI background spectrum, we study the dependence of the intensity of the line signal on the offset of the SPI pointing from the direction toward the Galactic Centre. After a critical analysis of the uncertainties of the DM density profile in the inner Galaxy, we find that the intensity of the DM decay line should decrease by at least a factor of 3 when the offset from the Galactic Centre increases from 0 to 180 degrees. We find that such a pronounced variation of the line flux across the sky is not observed for any line, detected with a significance higher than 3 sigma in the SPI background spectrum. Possible DM decay origin is not ruled out only for the unidentified spectral lines, having low (~3 sigma) significance or coinciding in position with the instrumental ones. In the energy interval from 20 keV to 7 MeV, we derive restrictions on the DM decay line flux, implied by the (non-)detection of the DM decay line. For a particular DM candidate, the sterile neutrino of mass MDM, we derive a bound on the mixing angle.
astro-ph hep-ph
using the highresolution spectrometer spi on board the international gammaray astrophysics laboratory integral we search for a spectral line produced by a dark matterdm particle with a mass in the range 40kev m_dm 14mev decaying in the dm halo of the milky way to distinguish the dm decay line from numerous instrumental lines found in the spi background spectrum we study the dependence of the intensity of the line signal on the offset of the spi pointing from the direction toward the galactic centre after a critical analysis of the uncertainties of the dm density profile in the inner galaxy we find that the intensity of the dm decay line should decrease by at least a factor of 3 when the offset from the galactic centre increases from 0 to 180 degrees we find that such a pronounced variation of the line flux across the sky is not observed for any line detected with a significance higher than 3 sigma in the spi background spectrum possible dm decay origin is not ruled out only for the unidentified spectral lines having low 3 sigma significance or coinciding in position with the instrumental ones in the energy interval from 20 kev to 7 mev we derive restrictions on the dm decay line flux implied by the nondetection of the dm decay line for a particular dm candidate the sterile neutrino of mass mdm we derive a bound on the mixing angle
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710.4923
Di-photon Higgs Decay in SUSY with CP Violation
Physical Higgs particles in the Minimal Supersymmetric Standard Model (MSSM) with explicit CP violation are CP mixed states. The decay of these Higgs particles can be analysed to study the CP properties of the MSSM. In the present work we consider the di-photon channel of the lightest neutral Higgs boson for this purpose. Compared to earlier studies on effects of scalar/pseudo-scalar mixing, our analysis also investigates the effect due to Higgs-sfermion-sfermion couplings along with that of mixing. We find that a light stop may have a strong impact on the width and Branching Ratio (BR) of the decay process H1 --> gamma.gamma, whereas other light sparticles have only little influence. In some regions of the MSSM parameter space with large CP-violating phase phi-mu ~ 90 deg a light (~ 200 GeV) stop can change the di-photon BR by more than 50 % compared to the case with heavy (~ 1 TeV) stop and otherwise same MSSM parameters.
hep-ph
physical higgs particles in the minimal supersymmetric standard model mssm with explicit cp violation are cp mixed states the decay of these higgs particles can be analysed to study the cp properties of the mssm in the present work we consider the diphoton channel of the lightest neutral higgs boson for this purpose compared to earlier studies on effects of scalarpseudoscalar mixing our analysis also investigates the effect due to higgssfermionsfermion couplings along with that of mixing we find that a light stop may have a strong impact on the width and branching ratio br of the decay process h1 gammagamma whereas other light sparticles have only little influence in some regions of the mssm parameter space with large cpviolating phase phimu 90 deg a light 200 gev stop can change the diphoton br by more than 50 compared to the case with heavy 1 tev stop and otherwise same mssm parameters
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710.4924
Do Incomplete GUT Multiplets Always Spoil Unification?
We consider a new class of light vectorlike exotics with fractional electric charge which do not come in complete representations of a grand unified gauge group, and are nevertheless compatible with gauge coupling unification and other predictions from Grand Unified Theories. Such states naturally arise in orbifold constructions of the heterotic string. Some aspects of their phenomenology and the consequences for the LHC are explored.
hep-ph
we consider a new class of light vectorlike exotics with fractional electric charge which do not come in complete representations of a grand unified gauge group and are nevertheless compatible with gauge coupling unification and other predictions from grand unified theories such states naturally arise in orbifold constructions of the heterotic string some aspects of their phenomenology and the consequences for the lhc are explored
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710.4925
Differences in Solution Behavior among Four Semiconductor-Binding Peptides
Recent experiments have identified peptides with adhesion affinity for GaAs and Si surfaces. Here we use all-atom Monte Carlo (MC) simulations with implicit solvent to investigate the behavior in aqueous solution of four such peptides, all with 12 residues. At room temperature, we find that all the four peptides are largely unstructured, which is consistent with experimental data. At the same time, we find that one of the peptides is structurally different and more flexible, compared to the others. This finding points at structural differences as a possible explanation for differences in adhesion properties between these peptides. By also analyzing designed mutants of two of the peptides, an experimental test of this hypothesis is proposed.
cond-mat.soft
recent experiments have identified peptides with adhesion affinity for gaas and si surfaces here we use allatom monte carlo mc simulations with implicit solvent to investigate the behavior in aqueous solution of four such peptides all with 12 residues at room temperature we find that all the four peptides are largely unstructured which is consistent with experimental data at the same time we find that one of the peptides is structurally different and more flexible compared to the others this finding points at structural differences as a possible explanation for differences in adhesion properties between these peptides by also analyzing designed mutants of two of the peptides an experimental test of this hypothesis is proposed
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710.4926
Time-resolved investigation of magnetization dynamics of arrays of non-ellipsoidal nanomagnets with a non-uniform ground state
We have performed time-resolved scanning Kerr microscopy (TRSKM) measurements upon arrays of square ferromagnetic nano-elements of different size and for a range of bias fields. The experimental results were compared to micromagnetic simulations of model arrays in order to understand the non-uniform precessional dynamics within the elements. In the experimental spectra two branches of excited modes were observed to co-exist above a particular bias field. Below the so-called crossover field, the higher frequency branch was observed to vanish. Micromagnetic simulations and Fourier imaging revealed that modes from the higher frequency branch had large amplitude at the center of the element where the effective field was parallel to the bias field and the static magnetization. Modes from the lower frequency branch had large amplitude near the edges of the element perpendicular to the bias field. The simulations revealed significant canting of the static magnetization and the effective field away from the direction of the bias field in the edge regions. For the smallest element sizes and/or at low bias field values the effective field was found to become anti-parallel to the static magnetization. The simulations revealed that the majority of the modes were de-localized with finite amplitude throughout the element, while the spatial character of a mode was found to be correlated with the spatial variation of the total effective field and the static magnetization state. The simulations also revealed that the frequencies of the edge modes are strongly affected by the spatial distribution of the static magnetization state both within an element and within its nearest neighbors.
cond-mat.mtrl-sci
we have performed timeresolved scanning kerr microscopy trskm measurements upon arrays of square ferromagnetic nanoelements of different size and for a range of bias fields the experimental results were compared to micromagnetic simulations of model arrays in order to understand the nonuniform precessional dynamics within the elements in the experimental spectra two branches of excited modes were observed to coexist above a particular bias field below the socalled crossover field the higher frequency branch was observed to vanish micromagnetic simulations and fourier imaging revealed that modes from the higher frequency branch had large amplitude at the center of the element where the effective field was parallel to the bias field and the static magnetization modes from the lower frequency branch had large amplitude near the edges of the element perpendicular to the bias field the simulations revealed significant canting of the static magnetization and the effective field away from the direction of the bias field in the edge regions for the smallest element sizes andor at low bias field values the effective field was found to become antiparallel to the static magnetization the simulations revealed that the majority of the modes were delocalized with finite amplitude throughout the element while the spatial character of a mode was found to be correlated with the spatial variation of the total effective field and the static magnetization state the simulations also revealed that the frequencies of the edge modes are strongly affected by the spatial distribution of the static magnetization state both within an element and within its nearest neighbors
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710.4927
Identification of Characteristic Protein Folding Channels in a Coarse-Grained Hydrophobic-Polar Peptide Model
Folding channels and free-energy landscapes of hydrophobic-polar heteropolymers are discussed on the basis of a minimalistic off-lattice coarse-grained model. We investigate how rearrangements of hydrophobic and polar monomers in a heteropolymer sequence lead to completely different folding behaviors. Studying three exemplified sequences with the same content of hydrophobic and polar residues, we can reproduce within this simple model two-state folding, folding through intermediates, as well as metastability.
cond-mat.soft
folding channels and freeenergy landscapes of hydrophobicpolar heteropolymers are discussed on the basis of a minimalistic offlattice coarsegrained model we investigate how rearrangements of hydrophobic and polar monomers in a heteropolymer sequence lead to completely different folding behaviors studying three exemplified sequences with the same content of hydrophobic and polar residues we can reproduce within this simple model twostate folding folding through intermediates as well as metastability
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710.4928
Quantum Hall effect in graphene: A functional determinant approach
We start the paper with a brief presentation of the main characteristics of graphene, and of the Dirac theory of massless fermions in 2+1 dimensions obtained as the associated low-momentum effective theory, in the absence of external fields. We then summarize the main steps needed to obtain the Hall conductivity in the effective theory at finite temperature and density, with emphasis on its dependence on the phase of the Dirac determinant selected during the evaluation of the effective action. Finally, we discuss the behavior, under gauge transformations, of the contribution due to the lowest Landau level, and interpret gauge transformations as rotations of the corresponding spinors around the magnetic field.
hep-th cond-mat.mes-hall math-ph math.MP
we start the paper with a brief presentation of the main characteristics of graphene and of the dirac theory of massless fermions in 21 dimensions obtained as the associated lowmomentum effective theory in the absence of external fields we then summarize the main steps needed to obtain the hall conductivity in the effective theory at finite temperature and density with emphasis on its dependence on the phase of the dirac determinant selected during the evaluation of the effective action finally we discuss the behavior under gauge transformations of the contribution due to the lowest landau level and interpret gauge transformations as rotations of the corresponding spinors around the magnetic field
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710.4929
Phase Separation in Peptide Aggregation Processes - Multicanonical Study of a Mesoscopic Model
We have performed multicanonical computer simulations of a small system of short protein-like heteropolymers and found that their aggregation transition possesses similarities to first-order phase separation processes. Not being a phase transition in the thermodynamic sense, the observed folding-binding behavior exhibits fascinating features leading to the conclusion that the temperature is no suitable control parameter in the transition region. More formally, for such small systems the microcanonical interpretation is more favorable than the typically used canonical picture.
cond-mat.soft
we have performed multicanonical computer simulations of a small system of short proteinlike heteropolymers and found that their aggregation transition possesses similarities to firstorder phase separation processes not being a phase transition in the thermodynamic sense the observed foldingbinding behavior exhibits fascinating features leading to the conclusion that the temperature is no suitable control parameter in the transition region more formally for such small systems the microcanonical interpretation is more favorable than the typically used canonical picture
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710.493
Extensions of discrete classical orthogonal polynomials beyond the orthogonality
It is well known that the family of Hahn polynomials $\{h_n^{\alpha,\beta}(x;N)\}_{n\ge 0}$ is orthogonal with respect to a certain weight function up to $N$. In this paper we present a factorization for Hahn polynomials for a degree higher than $N$ and we prove that these polynomials can be characterized by a $\Delta$-Sobolev orthogonality. We also present an analogous result for dual-Hahn, Krawtchouk, and Racah polynomials and give the limit relations between them for all $n\in \XX N_0$. Furthermore, in order to get this results for the Krawtchouk polynomials we will get a more general property of orthogonality for Meixner polynomials.
math.CA
it is well known that the family of hahn polynomials h_nalphabetaxn_nge 0 is orthogonal with respect to a certain weight function up to n in this paper we present a factorization for hahn polynomials for a degree higher than n and we prove that these polynomials can be characterized by a deltasobolev orthogonality we also present an analogous result for dualhahn krawtchouk and racah polynomials and give the limit relations between them for all nin xx n_0 furthermore in order to get this results for the krawtchouk polynomials we will get a more general property of orthogonality for meixner polynomials
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710.4931
Recent results in four-dimensional non-perturbative string theory
We review recent progress in understanding non-perturbative instanton corrections to the hypermultiplet moduli space in type II string compactifications on Calabi-Yau threefolds.
hep-th
we review recent progress in understanding nonperturbative instanton corrections to the hypermultiplet moduli space in type ii string compactifications on calabiyau threefolds
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710.4932
The concentration index of subharmonic functions of infinite order
The purpose of this paper is to introduce into consideration an analogue of the concentration index in the class of subharmonic functions of infinite order. The one in the case of finite order is used in the interpolation theory.
math.CV
the purpose of this paper is to introduce into consideration an analogue of the concentration index in the class of subharmonic functions of infinite order the one in the case of finite order is used in the interpolation theory
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710.4933
Superlens imaging theory for anisotropic nanostructured metamaterials with broadband all-angle negative refraction
We show that a metamaterial consisting of aligned metallic nanowires in a dielectric matrix has strongly anisotropic optical properties. For filling ratio f<1/2, the composite medium shows two surface plasmon resonances (SPRs): the transverse and longitudinal SPR with wavelengths lambda_t<lambda_l. For lambda>lambda_l, the longitudinal SPR, the material exhibits Re epsilon_l<0, Re epsilon_t>0, relative to the nanowires axis, enabling the achievement of broadband all-angle negative refraction and superlens imaging. An imaging theory of superlens made of these media is established. High performance systems made with Au, Ag or Al nanowires in nanoporous templates are designed and predicted to work from the infrared up to ultraviolet frequencies.
cond-mat.mtrl-sci
we show that a metamaterial consisting of aligned metallic nanowires in a dielectric matrix has strongly anisotropic optical properties for filling ratio f12 the composite medium shows two surface plasmon resonances sprs the transverse and longitudinal spr with wavelengths lambda_tlambda_l for lambdalambda_l the longitudinal spr the material exhibits re epsilon_l0 re epsilon_t0 relative to the nanowires axis enabling the achievement of broadband allangle negative refraction and superlens imaging an imaging theory of superlens made of these media is established high performance systems made with au ag or al nanowires in nanoporous templates are designed and predicted to work from the infrared up to ultraviolet frequencies
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710.4934
Spectral analysis of LMC X-2 with XMM/Newton: unveiling the emission process in the extragalactic Z-source
We present the results of the analysis of an archival observation of LMC X-2 performed with XMM/Newton. The spectra taken by high-precision instruments have never been analyzed before. We find an X-ray position for the source that is inconsistent with the one obtained by ROSAT, but in agreement with the Einstein position and that of the optical counterpart. The correlated spectral and timing behaviour of the source suggests that the source is probably in the normal branch of its X-ray color-color diagram. The spectrum of the source can be fitted with a blackbody with a temperature 1.5 keV plus a disk blackbody at 0.8 keV. Photoelectric absorption from neutral matter has an equivalent hydrogen column of 4 x 10^{20} cm^{-2}. An emission line, which we identify as the O VIII Lyman alpha line, is detected, while no feature due to iron is detected in the spectrum. We argue that the emission of this source can be straightforwardly interpreted as a sum of the emission from a boundary layer between the NS and the disc and a blackbody component coming from the disc itself. Other canonical models that are used to fit Z-sources do not give a satisfactory fit to the data. The detection of the O VIII emission line (and the lack of detection of lines in the iron region) can be due to the fact that the source lies in the Large Magellanic Cloud.
astro-ph
we present the results of the analysis of an archival observation of lmc x2 performed with xmmnewton the spectra taken by highprecision instruments have never been analyzed before we find an xray position for the source that is inconsistent with the one obtained by rosat but in agreement with the einstein position and that of the optical counterpart the correlated spectral and timing behaviour of the source suggests that the source is probably in the normal branch of its xray colorcolor diagram the spectrum of the source can be fitted with a blackbody with a temperature 15 kev plus a disk blackbody at 08 kev photoelectric absorption from neutral matter has an equivalent hydrogen column of 4 x 1020 cm2 an emission line which we identify as the o viii lyman alpha line is detected while no feature due to iron is detected in the spectrum we argue that the emission of this source can be straightforwardly interpreted as a sum of the emission from a boundary layer between the ns and the disc and a blackbody component coming from the disc itself other canonical models that are used to fit zsources do not give a satisfactory fit to the data the detection of the o viii emission line and the lack of detection of lines in the iron region can be due to the fact that the source lies in the large magellanic cloud
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710.4935
Is Gravitational Lensing by Intercluster Filaments Always Negligible?
Intercluster filaments negligibly contribute to the weak lensing signal in general relativity (GR), $\gamma_{N}\sim 10^{-4}-10^{-3}$. In the context of relativistic modified Newtonian dynamics (MOND) introduced by Bekenstein, however, a single filament inclined by $\approx 45^\circ$ from the line of sight can cause substantial distortion of background sources pointing towards the filament's axis ($\kappa=\gamma=(1-A^{-1})/2\sim 0.01$); this is rigorous for infinitely long uniform filaments, but also qualitatively true for short filaments ($\sim 30$Mpc), and even in regions where the projected matter density of the filament is equal to zero. Since galaxies and galaxy clusters are generally embedded in filaments or are projected on such structures, this contribution complicates the interpretation of the weak lensing shear map in the context of MOND. While our analysis is of mainly theoretical interest providing order-of-magnitude estimates only, it seems safe to conclude that when modeling systems with anomalous weak lensing signals, e.g. the "bullet cluster" of Clowe et al., the "cosmic train wreck" of Abell 520 from Mahdavi et al., and the "dark clusters" of Erben et al., filamentary structures might contribute in a significant and likely complex fashion. On the other hand, our predictions of a (conceptual) difference in the weak lensing signal could, in principle, be used to falsify MOND/TeVeS and its variations.
astro-ph
intercluster filaments negligibly contribute to the weak lensing signal in general relativity gr gamma_nsim 104103 in the context of relativistic modified newtonian dynamics mond introduced by bekenstein however a single filament inclined by approx 45circ from the line of sight can cause substantial distortion of background sources pointing towards the filaments axis kappagamma1a12sim 001 this is rigorous for infinitely long uniform filaments but also qualitatively true for short filaments sim 30mpc and even in regions where the projected matter density of the filament is equal to zero since galaxies and galaxy clusters are generally embedded in filaments or are projected on such structures this contribution complicates the interpretation of the weak lensing shear map in the context of mond while our analysis is of mainly theoretical interest providing orderofmagnitude estimates only it seems safe to conclude that when modeling systems with anomalous weak lensing signals eg the bullet cluster of clowe et al the cosmic train wreck of abell 520 from mahdavi et al and the dark clusters of erben et al filamentary structures might contribute in a significant and likely complex fashion on the other hand our predictions of a conceptual difference in the weak lensing signal could in principle be used to falsify mondteves and its variations
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710.4936
Dark Matter Caustics in Galaxy Clusters
We interpret the recent gravitational lensing observations of Jee et al. \cite{Jee} as first evidence for a {\it caustic} ring of dark matter in a galaxy cluster. A caustic ring unavoidably forms when a cold collisionless flow falls with net overall rotation in and out of a gravitational potential well. Evidence for caustic rings of dark matter was previously found in the Milky Way and other isolated spiral galaxies. We argue that galaxy clusters have at least one and possibly two or three caustic rings. We calculate the column density profile of a caustic ring in a cluster and show that it is consistent with the observations of Jee et al.
astro-ph
we interpret the recent gravitational lensing observations of jee et al citejee as first evidence for a it caustic ring of dark matter in a galaxy cluster a caustic ring unavoidably forms when a cold collisionless flow falls with net overall rotation in and out of a gravitational potential well evidence for caustic rings of dark matter was previously found in the milky way and other isolated spiral galaxies we argue that galaxy clusters have at least one and possibly two or three caustic rings we calculate the column density profile of a caustic ring in a cluster and show that it is consistent with the observations of jee et al
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710.4937
Heavy sfermions in SUSY analysis at LHC and ILC
The physics potential of the Large Hadron Collider in combination with the planned International Linear Collider is discussed for a difficult region of supersymmetry that is characterized by scalar SUSY particles with masses around 2 TeV. Precision measurements of masses, cross sections and forward-backward asymmetries allow to determine the fundamental supersymmetric parameters even if only a small part of the spectrum is accessible. No assumptions on a specific SUSY-breaking mechanism are imposed. Mass contraints for the kinematically inaccessible particles can be derived.
hep-ph
the physics potential of the large hadron collider in combination with the planned international linear collider is discussed for a difficult region of supersymmetry that is characterized by scalar susy particles with masses around 2 tev precision measurements of masses cross sections and forwardbackward asymmetries allow to determine the fundamental supersymmetric parameters even if only a small part of the spectrum is accessible no assumptions on a specific susybreaking mechanism are imposed mass contraints for the kinematically inaccessible particles can be derived
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710.4938
Breakdown of the Fermi-liquid regime in the 2D Hubbard model from a two-loop field-theoretical renormalization group approach
We analyze the particle-hole symmetric two-dimensional Hubbard model on a square lattice starting from weak-to-moderate couplings by means of the field-theoretical renormalization group (RG) approach up to two-loop order. This method is essential in order to evaluate the effect of the momentum-resolved anomalous dimension $\eta(\textbf{p})$ which arises in the normal phase of this model on the corresponding low-energy single-particle excitations. As a result, we find important indications pointing to the existence of a non-Fermi liquid (NFL) regime at temperature $T\to 0$ displaying a truncated Fermi surface (FS) for a doping range exactly in between the well-known antiferromagnetic insulating and the $d_{x^2-y^2}$-wave singlet superconducting phases. This NFL evolves as a function of doping into a correlated metal with a large FS before the $d_{x^2-y^2}$-wave pairing susceptibility finally produces the dominant instability in the low-energy limit.
cond-mat.str-el cond-mat.supr-con
we analyze the particlehole symmetric twodimensional hubbard model on a square lattice starting from weaktomoderate couplings by means of the fieldtheoretical renormalization group rg approach up to twoloop order this method is essential in order to evaluate the effect of the momentumresolved anomalous dimension etatextbfp which arises in the normal phase of this model on the corresponding lowenergy singleparticle excitations as a result we find important indications pointing to the existence of a nonfermi liquid nfl regime at temperature tto 0 displaying a truncated fermi surface fs for a doping range exactly in between the wellknown antiferromagnetic insulating and the d_x2y2wave singlet superconducting phases this nfl evolves as a function of doping into a correlated metal with a large fs before the d_x2y2wave pairing susceptibility finally produces the dominant instability in the lowenergy limit
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710.4939
Lifetime difference in D^0 - \bar{D^0} mixing within R-parity-violating SUSY
We re-examine constraints from the recent evidence for observation of the lifetime difference in D^0 - \bar{D}^0 mixing on the parameters of supersymmetric models with R-parity violation (RPV). We find that RPV SUSY can give large negative contribution to the lifetime difference. We also discuss the importance of the choice of weak or mass basis when placing the constraints on RPV-violating couplings from flavor mixing experiments.
hep-ph
we reexamine constraints from the recent evidence for observation of the lifetime difference in d0 bard0 mixing on the parameters of supersymmetric models with rparity violation rpv we find that rpv susy can give large negative contribution to the lifetime difference we also discuss the importance of the choice of weak or mass basis when placing the constraints on rpvviolating couplings from flavor mixing experiments
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710.494
Pore-blockade Times for Field-Driven Polymer Translocation
We study pore blockade times for a translocating polymer of length $N$, driven by a field $E$ across the pore in three dimensions. The polymer performs Rouse dynamics, i.e., we consider polymer dynamics in the absence of hydrodynamical interactions. We find that the typical time the pore remains blocked during a translocation event scales as $\sim N^{(1+2\nu)/(1+\nu)}/E$, where $\nu\simeq0.588$ is the Flory exponent for the polymer. In line with our previous work, we show that this scaling behaviour stems from the polymer dynamics at the immediate vicinity of the pore -- in particular, the memory effects in the polymer chain tension imbalance across the pore. This result, along with the numerical results by several other groups, violates the lower bound $\sim N^{1+\nu}/E$ suggested earlier in the literature. We discuss why this lower bound is incorrect and show, based on conservation of energy, that the correct lower bound for the pore-blockade time for field-driven translocation is given by $\eta N^{2\nu}/E$, where $\eta$ is the viscosity of the medium surrounding the polymer.
cond-mat.soft cond-mat.stat-mech physics.bio-ph q-bio.BM
we study pore blockade times for a translocating polymer of length n driven by a field e across the pore in three dimensions the polymer performs rouse dynamics ie we consider polymer dynamics in the absence of hydrodynamical interactions we find that the typical time the pore remains blocked during a translocation event scales as sim n12nu1nue where nusimeq0588 is the flory exponent for the polymer in line with our previous work we show that this scaling behaviour stems from the polymer dynamics at the immediate vicinity of the pore in particular the memory effects in the polymer chain tension imbalance across the pore this result along with the numerical results by several other groups violates the lower bound sim n1nue suggested earlier in the literature we discuss why this lower bound is incorrect and show based on conservation of energy that the correct lower bound for the poreblockade time for fielddriven translocation is given by eta n2nue where eta is the viscosity of the medium surrounding the polymer
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710.4941
Ocean Planet or Thick Atmosphere: On the Mass-Radius Relationship for Solid Exoplanets with Massive Atmospheres
The bulk composition of an exoplanet is commonly inferred from its average density. For small planets, however, the average density is not unique within the range of compositions. Variations of a number of important planetary parameters--which are difficult or impossible to constrain from measurements alone--produce planets with the same average densities but widely varying bulk compositions. We find that adding a gas envelope equivalent to 0.1%-10% of the mass of a solid planet causes the radius to increase 5-60% above its gas-free value. A planet with a given mass and radius might have substantial water ice content (a so-called ocean planet) or alternatively a large rocky-iron core and some H and/or He. For example, a wide variety of compositions can explain the observed radius of GJ 436b, although all models require some H/He. We conclude that the identification of water worlds based on the mass-radius relationship alone is impossible unless a significant gas layer can be ruled out by other means.
astro-ph
the bulk composition of an exoplanet is commonly inferred from its average density for small planets however the average density is not unique within the range of compositions variations of a number of important planetary parameterswhich are difficult or impossible to constrain from measurements aloneproduce planets with the same average densities but widely varying bulk compositions we find that adding a gas envelope equivalent to 0110 of the mass of a solid planet causes the radius to increase 560 above its gasfree value a planet with a given mass and radius might have substantial water ice content a socalled ocean planet or alternatively a large rockyiron core and some h andor he for example a wide variety of compositions can explain the observed radius of gj 436b although all models require some hhe we conclude that the identification of water worlds based on the massradius relationship alone is impossible unless a significant gas layer can be ruled out by other means
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710.4942
Topology of the Spin-polarized Charge Density in bcc and fcc Iron
We investigate the topology of the spin-polarized charge density in bcc and fcc iron. While the total spin-density is found to possess the topology of the non-magnetic prototypical structures, in some cases the spin-polarized densities are characterized by unique topologies; for example, the spin-polarized charge densities of bcc and high-spin fcc iron are atypical of any known for non-magnetic materials. In these cases, the two spin-densities are correlated: the spin-minority electrons have directional bond paths with deep minima in the minority density, while the spin-majority electrons fill these holes, reducing bond directionality. The presence of two distinct spin topologies suggests that a well-known magnetic phase transition in iron can be fruitfully reexamined in light of these topological changes. We show that the two phase changes seen in fcc iron (paramagnetic to low-spin and low-spin to high-spin) are different. The former follows the Landau symmetry-breaking paradigm and proceeds without a topological transformation, while the latter also involves a topological catastrophe.
cond-mat.mtrl-sci
we investigate the topology of the spinpolarized charge density in bcc and fcc iron while the total spindensity is found to possess the topology of the nonmagnetic prototypical structures in some cases the spinpolarized densities are characterized by unique topologies for example the spinpolarized charge densities of bcc and highspin fcc iron are atypical of any known for nonmagnetic materials in these cases the two spindensities are correlated the spinminority electrons have directional bond paths with deep minima in the minority density while the spinmajority electrons fill these holes reducing bond directionality the presence of two distinct spin topologies suggests that a wellknown magnetic phase transition in iron can be fruitfully reexamined in light of these topological changes we show that the two phase changes seen in fcc iron paramagnetic to lowspin and lowspin to highspin are different the former follows the landau symmetrybreaking paradigm and proceeds without a topological transformation while the latter also involves a topological catastrophe
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710.4943
Radiative Mechanism to Light Fermion Masses in the MSSM
In a previous work we have showed that the ${\cal Z}_{2}^{\prime}$ Symmetry, imply that the light fermions, the electron and the quarks, $u,d$ and $s$, get their masses only at one loop level. Here, we considere the more general hypothesis for flavour mixing in the sfermion sector in the MSSM. Then, we present our results to the masses of these light fermions and as a final result we can explain why the $s$ quark is heavier than the $u,d$ quarks. This mechanism is in agrement with the experimental constraint on the sfermion's masses values.
hep-ph
in a previous work we have showed that the cal z_2prime symmetry imply that the light fermions the electron and the quarks ud and s get their masses only at one loop level here we considere the more general hypothesis for flavour mixing in the sfermion sector in the mssm then we present our results to the masses of these light fermions and as a final result we can explain why the s quark is heavier than the ud quarks this mechanism is in agrement with the experimental constraint on the sfermions masses values
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710.4944
Evidence for higher order QED in e+ e- pair production at RHIC
A new lowest order QED calculation for RHIC e+ e- pair production has been carried out with a phenomenological treatment of the Coulomb dissociation of the heavy ion nuclei observed in the STAR ZDC triggers. The lowest order QED result for the experimental acceptance is nearly two standard deviations larger than the STAR data. A corresponding higher order QED calculation is consistent with the data.
nucl-th nucl-ex
a new lowest order qed calculation for rhic e e pair production has been carried out with a phenomenological treatment of the coulomb dissociation of the heavy ion nuclei observed in the star zdc triggers the lowest order qed result for the experimental acceptance is nearly two standard deviations larger than the star data a corresponding higher order qed calculation is consistent with the data
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710.4945
Degree Bounds for Gr\"obner Bases in Algebras of Solvable Type
We establish doubly-exponential degree bounds for Gr\"obner bases in certain algebras of solvable type over a field (as introduced by Kandri-Rody and Weispfenning). The class of algebras considered here includes commutative polynomial rings, Weyl algebras, and universal enveloping algebras of finite-dimensional Lie algebras. For the computation of these bounds, we adapt a method due to Dub\'e based on a generalization of Stanley decompositions. Our bounds yield doubly-exponential degree bounds for ideal membership and syzygies, generalizing the classical results of Hermann and Seidenberg (in the commutative case) and Grigoriev (in the case of Weyl algebras).
math.AC math.RA
we establish doublyexponential degree bounds for grobner bases in certain algebras of solvable type over a field as introduced by kandrirody and weispfenning the class of algebras considered here includes commutative polynomial rings weyl algebras and universal enveloping algebras of finitedimensional lie algebras for the computation of these bounds we adapt a method due to dube based on a generalization of stanley decompositions our bounds yield doublyexponential degree bounds for ideal membership and syzygies generalizing the classical results of hermann and seidenberg in the commutative case and grigoriev in the case of weyl algebras
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710.4946
Small Structures via Thermal Instability of Partially Ionized Plasma. I. Condensation Mode
(Shortened) Thermal instability of partially ionized plasma is investigated by linear perturbation analysis. According to the previous studies under the one fluid approach, the thermal instability is suppressed due to the magnetic pressure. However, the previous studies did not precisely consider the effect of the ion-neutral friction, since they did not treat the flow as two fluid which is composed of ions and neutrals. Then, we revisit the effect of the ion-neutral friction of the two fluid to the growth of the thermal instability. According to our study, (1) The instability which is characterized by the mean molecular weight of neutrals is suppressed via the ion-neutral friction only when the magnetic field and the friction are sufficiently strong. The suppression owing to the friction occurs even along the field line. If the magnetic field and the friction are not so strong, the instability is not stabilized. (2) The effect of the friction and the magnetic field is mainly reduction of the growth rate of the thermal instability of weakly ionized plasma. (3) The effect of friction does not affect the critical wavelength lambdaF for the thermal instability. This yields that lambdaF of the weakly ionized plasma is not enlarged even when the magnetic field exists. We insist that the thermal instability of the weakly ionized plasma in the magnetic field can grow up even at the small length scale where the instability under the assumption of the one fluid plasma can not grow owing to the stabilization by the magnetic field. (4) The wavelength of the maximum growth rate of the instability shifts shortward according to the decrement of the growth rate, because the friction is effective at rather larger scale. Therefore, smaller structures are expected to appear than those without the ion-neutral friction.
astro-ph
shortened thermal instability of partially ionized plasma is investigated by linear perturbation analysis according to the previous studies under the one fluid approach the thermal instability is suppressed due to the magnetic pressure however the previous studies did not precisely consider the effect of the ionneutral friction since they did not treat the flow as two fluid which is composed of ions and neutrals then we revisit the effect of the ionneutral friction of the two fluid to the growth of the thermal instability according to our study 1 the instability which is characterized by the mean molecular weight of neutrals is suppressed via the ionneutral friction only when the magnetic field and the friction are sufficiently strong the suppression owing to the friction occurs even along the field line if the magnetic field and the friction are not so strong the instability is not stabilized 2 the effect of the friction and the magnetic field is mainly reduction of the growth rate of the thermal instability of weakly ionized plasma 3 the effect of friction does not affect the critical wavelength lambdaf for the thermal instability this yields that lambdaf of the weakly ionized plasma is not enlarged even when the magnetic field exists we insist that the thermal instability of the weakly ionized plasma in the magnetic field can grow up even at the small length scale where the instability under the assumption of the one fluid plasma can not grow owing to the stabilization by the magnetic field 4 the wavelength of the maximum growth rate of the instability shifts shortward according to the decrement of the growth rate because the friction is effective at rather larger scale therefore smaller structures are expected to appear than those without the ionneutral friction
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710.4947
Physics at a future Neutrino Factory and super-beam facility
The conclusions of the Physics Working Group of the international scoping study of a future Neutrino Factory and super-beam facility (the ISS) are presented. The ISS was carried by the international community between NuFact05, (the 7th International Workshop on Neutrino Factories and Superbeams, Laboratori Nazionali di Frascati, Rome, June 21-26, 2005) and NuFact06 (Ivine, California, 24{30 August 2006). The physics case for an extensive experimental programme to understand the properties of the neutrino is presented and the role of high-precision measurements of neutrino oscillations within this programme is discussed in detail. The performance of second generation super-beam experiments, beta-beam facilities, and the Neutrino Factory are evaluated and a quantitative comparison of the discovery potential of the three classes of facility is presented. High-precision studies of the properties of the muon are complementary to the study of neutrino oscillations. The Neutrino Factory has the potential to provide extremely intense muon beams and the physics potential of such beams is discussed in the final section of the report.
hep-ph
the conclusions of the physics working group of the international scoping study of a future neutrino factory and superbeam facility the iss are presented the iss was carried by the international community between nufact05 the 7th international workshop on neutrino factories and superbeams laboratori nazionali di frascati rome june 2126 2005 and nufact06 ivine california 2430 august 2006 the physics case for an extensive experimental programme to understand the properties of the neutrino is presented and the role of highprecision measurements of neutrino oscillations within this programme is discussed in detail the performance of second generation superbeam experiments betabeam facilities and the neutrino factory are evaluated and a quantitative comparison of the discovery potential of the three classes of facility is presented highprecision studies of the properties of the muon are complementary to the study of neutrino oscillations the neutrino factory has the potential to provide extremely intense muon beams and the physics potential of such beams is discussed in the final section of the report
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710.4948
A New Algorithm in Geometry of Numbers
A lattice Delaunay polytope P is called perfect if its Delaunay sphere is the only ellipsoid circumscribed about P. We present a new algorithm for finding perfect Delaunay polytopes. Our method overcomes the major shortcomings of the previously used method. We have implemented and used our algorithm for finding perfect Delaunay polytopes in dimensions 6, 7, 8. Our findings lead to a new conjecture that sheds light on the structure of lattice Delaunay tilings.
math.NT math.MG
a lattice delaunay polytope p is called perfect if its delaunay sphere is the only ellipsoid circumscribed about p we present a new algorithm for finding perfect delaunay polytopes our method overcomes the major shortcomings of the previously used method we have implemented and used our algorithm for finding perfect delaunay polytopes in dimensions 6 7 8 our findings lead to a new conjecture that sheds light on the structure of lattice delaunay tilings
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710.4949
Detection of quantum light in the presence of noise
Detection of quantum light in the presence of dark counts and background radiation noise is considered. The corresponding positive operator-valued measure is obtained and photocounts statistics of quantum light in the presence of noise is studied.
quant-ph
detection of quantum light in the presence of dark counts and background radiation noise is considered the corresponding positive operatorvalued measure is obtained and photocounts statistics of quantum light in the presence of noise is studied
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710.495
Titan's rotation: A 3-dimensional theory
We study the forced rotation of Titan seen as a rigid body at the equilibrium Cassini state, involving the spin-orbit synchronization. We used both the analytical and the numerical ways. We analytically determined the equilibrium positions and the frequencies of the 3 free librations around it, while a numerical integration associated to frequency analysis gave us a more synthetic, complete theory, where the free solution split from the forced one. We find a mean obliquity of 2.2 arcmin and the fundamental frequencies of the free librations of about 2.0977, 167.4883, and 306.3360 years. Moreover, we bring out the main role played by Titan's inclination on its rotation, and we suspect a likely resonance involving Titan's wobble.
astro-ph
we study the forced rotation of titan seen as a rigid body at the equilibrium cassini state involving the spinorbit synchronization we used both the analytical and the numerical ways we analytically determined the equilibrium positions and the frequencies of the 3 free librations around it while a numerical integration associated to frequency analysis gave us a more synthetic complete theory where the free solution split from the forced one we find a mean obliquity of 22 arcmin and the fundamental frequencies of the free librations of about 20977 1674883 and 3063360 years moreover we bring out the main role played by titans inclination on its rotation and we suspect a likely resonance involving titans wobble
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710.4951
A Symbolic Finite-state approach for Automated Proving of Theorems in Combinatorial Game Theory
We develop a finite-state automata approach, implemented in a Maple package {\tt ToadsAndFrogs} available from our websites, for conjecturing, and then rigorously proving, values for large families of positions in Richard Guy's combinatorial game ``Toads and Frogs''. In particular, we prove a conjecture of Jeff Erickson.
math.DS math.CO
we develop a finitestate automata approach implemented in a maple package tt toadsandfrogs available from our websites for conjecturing and then rigorously proving values for large families of positions in richard guys combinatorial game toads and frogs in particular we prove a conjecture of jeff erickson
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710.4952
On descent theory and main conjectures in non-commutative Iwasawa theory
We prove a `Weierstrass Preparation Theorem' and develop an explicit descent formalism in the context of Whitehead groups of non-commutative Iwasawa algebras. We use these results to describe the precise connection between the main conjecture of non-commutative Iwasawa theory (in the sense of Coates, Fukaya, Kato, Sujatha and Venjakob) and the equivariant Tamagawa number conjecture. The latter result is both a converse to a theorem of Fukaya and Kato and also provides an important means of deriving explicit consequences of the main conjecture.
math.NT
we prove a weierstrass preparation theorem and develop an explicit descent formalism in the context of whitehead groups of noncommutative iwasawa algebras we use these results to describe the precise connection between the main conjecture of noncommutative iwasawa theory in the sense of coates fukaya kato sujatha and venjakob and the equivariant tamagawa number conjecture the latter result is both a converse to a theorem of fukaya and kato and also provides an important means of deriving explicit consequences of the main conjecture
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