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710.3853
Hopf modules for autonomous pseudomonoids and the monoidal centre
In this work we develop some aspects of the theory of Hopf algebras to the context of autonomous map pseudomonoids. We concentrate in the Hopf modules and the Centre or Drinfel'd double. If $A$ is a map pseudomonoid in a monoidal bicategory \M, the analogue of the category of Hopf modules for $A$ is an Eilenberg-Moore construction for a certain monad in $\mathbf{Hom}(\M^{\mathrm{op}},\mathbf{Cat})$. We study the existence of the internalisation of this notion, called the Hopf module construction, by extending the completion under Eilenberg-Moore objects of a 2-category to a endo-homomorphism of tricategories on $\mathbf{Bicat}$. Our main result is the equivalence between the existence of a left dualization for $A$ ({\em i.e.}, $A$ is left autonomous) and the validity of an analogue of the structure theorem of Hopf modules. In this case the Hopf module construction for $A$ always exists. We use these results to study the lax centre of a left autonomous map pseudomonoid. We show that the lax centre is the Eilenberg-Moore construction for a certain monad on $A$ (one existing if the other does). If $A$ is also right autonomous, then the lax centre equals the centre. We look at the examples of the bicategories of \V-modules and of comodules in \V, and obtain the Drinfel'd double of a coquasi-Hopf algebra $H$ as the centre of $H$.
math.CT math.QA
in this work we develop some aspects of the theory of hopf algebras to the context of autonomous map pseudomonoids we concentrate in the hopf modules and the centre or drinfeld double if a is a map pseudomonoid in a monoidal bicategory m the analogue of the category of hopf modules for a is an eilenbergmoore construction for a certain monad in mathbfhommmathrmopmathbfcat we study the existence of the internalisation of this notion called the hopf module construction by extending the completion under eilenbergmoore objects of a 2category to a endohomomorphism of tricategories on mathbfbicat our main result is the equivalence between the existence of a left dualization for a em ie a is left autonomous and the validity of an analogue of the structure theorem of hopf modules in this case the hopf module construction for a always exists we use these results to study the lax centre of a left autonomous map pseudomonoid we show that the lax centre is the eilenbergmoore construction for a certain monad on a one existing if the other does if a is also right autonomous then the lax centre equals the centre we look at the examples of the bicategories of vmodules and of comodules in v and obtain the drinfeld double of a coquasihopf algebra h as the centre of h
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710.3854
Models for the Observable System Parameters of Ultraluminous X-ray Sources
We investigate the evolution of the properties of model populations of ultraluminous X-ray sources (ULXs) consisting of a black-hole accretor in a binary with a donor star. We have computed models corresponding to three different populations of black-hole binaries; two invoke stellar-mass (~10 Msun) black hole accretors, and the third utilizes intermediate-mass (~1000 Msun) black holes (IMBHs). For each of the three populations, we computed 30,000 binary evolution sequences using a full Henyey stellar evolution code. The optical flux from the model ULXs includes contributions from the accretion disk, due to x-ray irradiation as well as intrinsic viscous heating, and that due to the donor star. We present "probability images" for the ULX systems in planes of color-magnitude, orbital period vs. X-ray luminosity, and luminosity vs. evolution time. Estimates of the numbers of ULXs in a typical galaxy as functions of time and of X-ray luminosity are also presented. Our model CMDs are compared with six ULX counterparts that have been discussed in the literature. Overall, the observed systems seem more closely related to model systems with very high-mass donors (> ~25 Msun) in binaries with IMBH accretors. However, significant difficulties remain with both the IMBH and stellar-mass black hole models.
astro-ph
we investigate the evolution of the properties of model populations of ultraluminous xray sources ulxs consisting of a blackhole accretor in a binary with a donor star we have computed models corresponding to three different populations of blackhole binaries two invoke stellarmass 10 msun black hole accretors and the third utilizes intermediatemass 1000 msun black holes imbhs for each of the three populations we computed 30000 binary evolution sequences using a full henyey stellar evolution code the optical flux from the model ulxs includes contributions from the accretion disk due to xray irradiation as well as intrinsic viscous heating and that due to the donor star we present probability images for the ulx systems in planes of colormagnitude orbital period vs xray luminosity and luminosity vs evolution time estimates of the numbers of ulxs in a typical galaxy as functions of time and of xray luminosity are also presented our model cmds are compared with six ulx counterparts that have been discussed in the literature overall the observed systems seem more closely related to model systems with very highmass donors 25 msun in binaries with imbh accretors however significant difficulties remain with both the imbh and stellarmass black hole models
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710.3855
Extraction of Singlet States from Noninteracting High-Dimensional Spins
We present a scheme for the extraction of singlet states of two remote particles of arbitrary quantum spin number. The goal is achieved through post-selection of the state of interaction mediators sent in succession. A small number of iterations is sufficient to make the scheme effective. We propose two suitable experimental setups where the protocol can be implemented.
quant-ph
we present a scheme for the extraction of singlet states of two remote particles of arbitrary quantum spin number the goal is achieved through postselection of the state of interaction mediators sent in succession a small number of iterations is sufficient to make the scheme effective we propose two suitable experimental setups where the protocol can be implemented
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710.3856
The Lattice Free Energy of QCD with Clover Fermions, up to Three-Loops
We calculate the perturbative value of the free energy in Lattice QCD, up to three loops. Our calculation is performed using Wilson gluons and the Sheikholeslami - Wolhert (clover) improved action for fermions. The free energy is directly related to the average plaquette. To carry out the calculation, we compute all relevant Feynman diagrams up to 3 loops, using a set of automated procedures in Mathematica; numerical evaluation of the resulting loop integrals is performed on finite lattice, with subsequent extrapolation to infinite size. The results are presented as a function of the fermion mass m, for any SU(N_c) gauge group, and for an arbitrary number of fermion flavors. In order to enable independent comparisons, we also provide the results on a per diagram basis, for a specific mass value.
hep-lat
we calculate the perturbative value of the free energy in lattice qcd up to three loops our calculation is performed using wilson gluons and the sheikholeslami wolhert clover improved action for fermions the free energy is directly related to the average plaquette to carry out the calculation we compute all relevant feynman diagrams up to 3 loops using a set of automated procedures in mathematica numerical evaluation of the resulting loop integrals is performed on finite lattice with subsequent extrapolation to infinite size the results are presented as a function of the fermion mass m for any sun_c gauge group and for an arbitrary number of fermion flavors in order to enable independent comparisons we also provide the results on a per diagram basis for a specific mass value
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710.3857
Generalizations of Sch\"{o}bi's Tetrahedral Dissection
Let v_1, ..., v_n be unit vectors in R^n such that v_i . v_j = -w for i != j, where -1 <w < 1/(n-1). The points Sum_{i=1..n} lambda_i v_i, where 1 >= lambda_1 >= ... >= lambda_n >= 0, form a ``Hill-simplex of the first type'', denoted by Q_n(w). It was shown by Hadwiger in 1951 that Q_n(w) is equidissectable with a cube. In 1985, Sch\"{o}bi gave a three-piece dissection of Q_3(w) into a triangular prism c Q_2(1/2) X I, where I denotes an interval and c = sqrt{2(w+1)/3}. The present paper generalizes Sch\"{o}bi's dissection to an n-piece dissection of Q_n(w) into a prism c Q_{n-1}(1/(n-1)) X I, where c = sqrt{(n-1)(w+1)/n}. Iterating this process leads to a dissection of Q_n(w) into an n-dimensional rectangular parallelepiped (or ``brick'') using at most n! pieces. The complexity of computing the map from Q_n(w) to the brick is O(n^2). A second generalization of Sch\"{o}bi's dissection is given which applies specifically in R^4. The results have applications to source coding and to constant-weight binary codes.
math.MG math.CO
let v_1 v_n be unit vectors in rn such that v_i v_j w for i j where 1 w 1n1 the points sum_i1n lambda_i v_i where 1 lambda_1 lambda_n 0 form a hillsimplex of the first type denoted by q_nw it was shown by hadwiger in 1951 that q_nw is equidissectable with a cube in 1985 schobi gave a threepiece dissection of q_3w into a triangular prism c q_212 x i where i denotes an interval and c sqrt2w13 the present paper generalizes schobis dissection to an npiece dissection of q_nw into a prism c q_n11n1 x i where c sqrtn1w1n iterating this process leads to a dissection of q_nw into an ndimensional rectangular parallelepiped or brick using at most n pieces the complexity of computing the map from q_nw to the brick is on2 a second generalization of schobis dissection is given which applies specifically in r4 the results have applications to source coding and to constantweight binary codes
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710.3858
Tamagawa defect of Euler systems
As remarked in [Kolyvagin systems, by Barry Mazur and Karl Rubin] Proposition 6.2.6 and Buyukboduk[ arXiv:0706.0377v1 ] Remark 3.25 one does not expect the Kolyvagin system obtained from an Euler system for a p-adic Galois representation T to be primitive (in the sense of [Kolyvagin systems, by Barry Mazur and Karl Rubin] Definition 4.5.5) if p divides a Tamagawa number at a prime \ell different from p; thus fails to compute the correct size of the relevant Selmer module. In this paper we obtain a lower bound for the size of the cokernel of the Euler system to Kolyvagin system map (see Theorem 3.2.4 of [Kolyvagin systems, by Barry Mazur and Karl Rubin] for a definition of this map) in terms of the Tamagawa numbers of T, refining [Kolyvagin systems, by Barry Mazur and Karl Rubin] Propostion 6.2.6. We show how this partially accounts for the missing Tamagawa factors in Kato's calculations with his Euler system.
math.NT
as remarked in kolyvagin systems by barry mazur and karl rubin proposition 626 and buyukboduk arxiv07060377v1 remark 325 one does not expect the kolyvagin system obtained from an euler system for a padic galois representation t to be primitive in the sense of kolyvagin systems by barry mazur and karl rubin definition 455 if p divides a tamagawa number at a prime ell different from p thus fails to compute the correct size of the relevant selmer module in this paper we obtain a lower bound for the size of the cokernel of the euler system to kolyvagin system map see theorem 324 of kolyvagin systems by barry mazur and karl rubin for a definition of this map in terms of the tamagawa numbers of t refining kolyvagin systems by barry mazur and karl rubin propostion 626 we show how this partially accounts for the missing tamagawa factors in katos calculations with his euler system
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710.3859
Endogenous versus Exogenous Origins of Diseases
Many illnesses are associated with an alteration of the immune system homeostasis due to any combination of factors, including exogenous bacterial insult, endogenous breakdown (e.g., development of a disease that results in immuno suppression), or an exogenous hit like surgery that simultaneously alters immune responsiveness and provides access to bacteria, or genetic disorder. We conjecture that, as a consequence of the co-evolution of the immune system of individuals with the ecology of pathogens, the homeostasis of the immune system requires the influx of pathogens. This allows the immune system to keep the ever present pathogens under control and to react and adjust fast to bursts of infections. We construct the simplest and most general system of rate equations which describes the dynamics of five compartments: healthy cells, altered cells, adaptive and innate immune cells, and pathogens. We study four regimes obtained with or without auto-immune disorder and with or without spontaneous proliferation of infected cells. Over all regimes, we find that seven different states are naturally described by the model: (i) strong healthy immune system, (ii) healthy organism with evanescent immune cells, (iii) chronic infections, (iv) strong infections, (v) cancer, (vi) critically ill state and (vii) death. The analysis of stability conditions demonstrates that these seven states depend on the balance between the robustness of the immune system and the influx of pathogens.
physics.bio-ph physics.med-ph q-bio.CB
many illnesses are associated with an alteration of the immune system homeostasis due to any combination of factors including exogenous bacterial insult endogenous breakdown eg development of a disease that results in immuno suppression or an exogenous hit like surgery that simultaneously alters immune responsiveness and provides access to bacteria or genetic disorder we conjecture that as a consequence of the coevolution of the immune system of individuals with the ecology of pathogens the homeostasis of the immune system requires the influx of pathogens this allows the immune system to keep the ever present pathogens under control and to react and adjust fast to bursts of infections we construct the simplest and most general system of rate equations which describes the dynamics of five compartments healthy cells altered cells adaptive and innate immune cells and pathogens we study four regimes obtained with or without autoimmune disorder and with or without spontaneous proliferation of infected cells over all regimes we find that seven different states are naturally described by the model i strong healthy immune system ii healthy organism with evanescent immune cells iii chronic infections iv strong infections v cancer vi critically ill state and vii death the analysis of stability conditions demonstrates that these seven states depend on the balance between the robustness of the immune system and the influx of pathogens
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710.386
Prime and composite Laurent polynomials
In 1922 Ritt constructed the theory of functional decompositions of polynomials with complex coefficients. In particular, he described explicitly indecomposable polynomial solutions of the functional equation f(p(z))=g(q(z)). In this paper we study the equation above in the case when f,g,p,q are holomorphic functions on compact Riemann surfaces. We also construct a self-contained theory of functional decompositions of rational functions with at most two poles generalizing the Ritt theory. In particular, we give new proofs of the theorems of Ritt and of the theorem of Bilu and Tichy.
math.CV math.AG
in 1922 ritt constructed the theory of functional decompositions of polynomials with complex coefficients in particular he described explicitly indecomposable polynomial solutions of the functional equation fpzgqz in this paper we study the equation above in the case when fgpq are holomorphic functions on compact riemann surfaces we also construct a selfcontained theory of functional decompositions of rational functions with at most two poles generalizing the ritt theory in particular we give new proofs of the theorems of ritt and of the theorem of bilu and tichy
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710.3861
Optimal encoding on discrete lattice with translational invariant constrains using statistical algorithms
In this paper will be presented methodology of encoding information in valuations of discrete lattice with some translational invariant constrains in asymptotically optimal way. The method is based on finding statistical description of such valuations and changing it into statistical algorithm, which allows to construct deterministically valuation with given statistics. Optimal statistics allow to generate valuations with uniform distribution - we get maximum information capacity this way. It will be shown that we can reach the optimum for one-dimensional models using maximal entropy random walk and that for the general case we can practically get as close to the capacity of the model as we want (found numerically: lost 10^{-10} bit/node for Hard Square). There will be also presented simpler alternative to arithmetic coding method which can be used as cryptosystem and data correction method too.
cs.IT math.IT
in this paper will be presented methodology of encoding information in valuations of discrete lattice with some translational invariant constrains in asymptotically optimal way the method is based on finding statistical description of such valuations and changing it into statistical algorithm which allows to construct deterministically valuation with given statistics optimal statistics allow to generate valuations with uniform distribution we get maximum information capacity this way it will be shown that we can reach the optimum for onedimensional models using maximal entropy random walk and that for the general case we can practically get as close to the capacity of the model as we want found numerically lost 1010 bitnode for hard square there will be also presented simpler alternative to arithmetic coding method which can be used as cryptosystem and data correction method too
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710.3862
Large-scale instability in a sheared nonhelical turbulence: formation of vortical structures
We study a large-scale instability in a sheared nonhelical turbulence that causes generation of large-scale vorticity. Three types of the background large-scale flows are considered, i.e., the Couette and Poiseuille flows in a small-scale homogeneous turbulence, and the "log-linear" velocity shear in an inhomogeneous turbulence. It is known that laminar plane Couette flow and antisymmetric mode of laminar plane Poiseuille flow are stable with respect to small perturbations for any Reynolds numbers. We demonstrate that in a small-scale turbulence under certain conditions the large-scale Couette and Poiseuille flows are unstable due to the large-scale instability. This instability causes formation of large-scale vortical structures stretched along the mean sheared velocity. The growth rate of the large-scale instability for the "log-linear" velocity shear is much larger than that for the Couette and Poiseuille background flows. We have found a turbulent analogue of the Tollmien-Schlichting waves in a small-scale sheared turbulence. A mechanism of excitation of turbulent Tollmien-Schlichting waves is associated with a combined effect of the turbulent Reynolds stress-induced generation of perturbations of the mean vorticity and the background sheared motions. These waves can be excited even in a plane Couette flow imposed on a small-scale turbulence when perturbations of mean velocity depend on three spatial coordinates. The energy of these waves is supplied by the small-scale sheared turbulence.
physics.flu-dyn astro-ph physics.geo-ph
we study a largescale instability in a sheared nonhelical turbulence that causes generation of largescale vorticity three types of the background largescale flows are considered ie the couette and poiseuille flows in a smallscale homogeneous turbulence and the loglinear velocity shear in an inhomogeneous turbulence it is known that laminar plane couette flow and antisymmetric mode of laminar plane poiseuille flow are stable with respect to small perturbations for any reynolds numbers we demonstrate that in a smallscale turbulence under certain conditions the largescale couette and poiseuille flows are unstable due to the largescale instability this instability causes formation of largescale vortical structures stretched along the mean sheared velocity the growth rate of the largescale instability for the loglinear velocity shear is much larger than that for the couette and poiseuille background flows we have found a turbulent analogue of the tollmienschlichting waves in a smallscale sheared turbulence a mechanism of excitation of turbulent tollmienschlichting waves is associated with a combined effect of the turbulent reynolds stressinduced generation of perturbations of the mean vorticity and the background sheared motions these waves can be excited even in a plane couette flow imposed on a smallscale turbulence when perturbations of mean velocity depend on three spatial coordinates the energy of these waves is supplied by the smallscale sheared turbulence
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710.3863
Analysis of the convex hull of the attractor of an IFS
In this paper we will introduce the methodology of analysis of the convex hull of the attractors of iterated functional systems (IFS) - compact fixed sets of self-similarity mapping. The method is based on a function which for a direction, gives width in that direction. We can write the self similarity equation in terms of this function, solve and analyze them. Using this function we can quickly check if the distance from K of a given x is smaller than a given distance or even compute analytically convex hull area and the length of its boundary
math.CA
in this paper we will introduce the methodology of analysis of the convex hull of the attractors of iterated functional systems ifs compact fixed sets of selfsimilarity mapping the method is based on a function which for a direction gives width in that direction we can write the self similarity equation in terms of this function solve and analyze them using this function we can quickly check if the distance from k of a given x is smaller than a given distance or even compute analytically convex hull area and the length of its boundary
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710.3864
Criteria for the density property of complex manifolds
In this paper we suggest new effective criteria for the density property. This enables us to give a trivial proof of the original Anders\'en-Lempert result and to establish (almost free of charge) the algebraic density property for all linear algebraic groups whose connected components are different from tori or $\C_+$. As another application of this approach we tackle the question (asked among others by F. Forstneri\v{c}) about the density of algebraic vector fields on Euclidean space vanishing on a codimension 2 subvariety.
math.CV
in this paper we suggest new effective criteria for the density property this enables us to give a trivial proof of the original andersenlempert result and to establish almost free of charge the algebraic density property for all linear algebraic groups whose connected components are different from tori or c_ as another application of this approach we tackle the question asked among others by f forstnerivc about the density of algebraic vector fields on euclidean space vanishing on a codimension 2 subvariety
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710.3865
Inhomogeneous exclusion processes with extended objects: The effect of defect locations
We study the effects of local inhomogeneities, i.e., slow sites of hopping rate $q<1$, in a totally asymmetric simple exclusion process (TASEP) for particles of size $\ell \geq 1$ (in units of the lattice spacing). We compare the simulation results of $\ell =1$ and $\ell >1$ and notice that the existence of local defects has qualitatively similar effects on the steady state. We focus on the stationary current as well as the density profiles. If there is only a single slow site in the system, we observe a significant dependence of the current on the \emph{location} of the slow site for both $\ell =1$ and $\ell >1$ cases. When two slow sites are introduced, more intriguing phenomena emerge, e.g., dramatic decreases in the current when the two are close together. In addition, we study the asymptotic behavior when $q\to 0$. We also explore the associated density profiles and compare our findings to an earlier study using a simple mean-field theory. We then outline the biological significance of these effects.
cond-mat.stat-mech
we study the effects of local inhomogeneities ie slow sites of hopping rate q1 in a totally asymmetric simple exclusion process tasep for particles of size ell geq 1 in units of the lattice spacing we compare the simulation results of ell 1 and ell 1 and notice that the existence of local defects has qualitatively similar effects on the steady state we focus on the stationary current as well as the density profiles if there is only a single slow site in the system we observe a significant dependence of the current on the emphlocation of the slow site for both ell 1 and ell 1 cases when two slow sites are introduced more intriguing phenomena emerge eg dramatic decreases in the current when the two are close together in addition we study the asymptotic behavior when qto 0 we also explore the associated density profiles and compare our findings to an earlier study using a simple meanfield theory we then outline the biological significance of these effects
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710.3866
Constraints on the Velocity and Spatial Distribution of Helium-like Ions in the Wind of SMC X-1 from Observations with XMM-Newton/RGS
We present here X-ray spectra of the HMXB SMC X-1 obtained in an observation with the XMM observatory beginning before eclipse and ending near the end of eclipse. With the Reflection Grating Spectrometers (RGS) on board XMM, we observe emission lines from hydrogen-like and helium-like ions of nitrogen, oxygen, neon, magnesium, and silicon. Though the resolution of the RGS is sufficient to resolve the helium-like n=2->1 emission into three line components, only one of these components, the intercombination line, is detected in our data. The lack of flux in the forbidden lines of the helium-like triplets is explained by pumping by ultraviolet photons from the B0 star and, from this, we set an upper limit on the distance of the emitting ions from the star. The lack of observable flux in the resonance lines of the helium-like triplets indicate a lack of enhancement due to resonance line scattering and, from this, we derive a new observational constraint on the distribution of the wind in SMC X-1 in velocity and coordinate space. We find that the solid angle subtended by the volume containing the helium-like ions at the neutron star multiplied by the velocity dispersion of the helium-like ions must be less than 4pi steradians km/s. This constraint will be satisfied if the helium-like ions are located primarily in clumps distributed throughout the wind or in a thin layer along the surface of the B0 star.
astro-ph
we present here xray spectra of the hmxb smc x1 obtained in an observation with the xmm observatory beginning before eclipse and ending near the end of eclipse with the reflection grating spectrometers rgs on board xmm we observe emission lines from hydrogenlike and heliumlike ions of nitrogen oxygen neon magnesium and silicon though the resolution of the rgs is sufficient to resolve the heliumlike n21 emission into three line components only one of these components the intercombination line is detected in our data the lack of flux in the forbidden lines of the heliumlike triplets is explained by pumping by ultraviolet photons from the b0 star and from this we set an upper limit on the distance of the emitting ions from the star the lack of observable flux in the resonance lines of the heliumlike triplets indicate a lack of enhancement due to resonance line scattering and from this we derive a new observational constraint on the distribution of the wind in smc x1 in velocity and coordinate space we find that the solid angle subtended by the volume containing the heliumlike ions at the neutron star multiplied by the velocity dispersion of the heliumlike ions must be less than 4pi steradians kms this constraint will be satisfied if the heliumlike ions are located primarily in clumps distributed throughout the wind or in a thin layer along the surface of the b0 star
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710.3867
Tidal debris from high-velocity collisions as fake dark galaxies: A numerical model of VirgoHI21
High speed collisions, although current in clusters of galaxies, have long been neglected, as they are believed to cause little damages to galaxies, except when they are repeated, a process called harassment. In fact, they are able to produce faint but extended gaseous tails. Such low-mass, starless, tidal debris may become detached and appear as free floating clouds in the very deep HI surveys that are currently being carried out. We show in this paper that these debris possess the same apparent properties as the so-called "Dark Galaxies", objects originally detected in HI, with no optical counterpart, and presumably dark matter dominated. We present a numerical model of the prototype of such Dark Galaxies - VirgoHI21 -, that is able to reproduce its main characteristics: the one-sided tail linking it to the spiral galaxy NGC 4254, the absence of stars, and above all the reversal of the velocity gradient along the tail originally attributed to rotation motions caused by a massive dark matter halo and which we find to be consistent with simple streaming motions plus projection effects. According to our numerical simulations, this tidal debris was expelled 750 Myr ago during a fly-by at 1100 km/s of NGC 4254 by a massive companion which should now lie at a projected distance of about 400 kpc. A candidate for the intruder is discussed. The existence of galaxies that have never been able to form stars had already been challenged based on theoretical and observational grounds. Tidal collisions, in particular those occurring at high speed, provide a much more simple explanation for the origin of such putative Dark Galaxies.
astro-ph
high speed collisions although current in clusters of galaxies have long been neglected as they are believed to cause little damages to galaxies except when they are repeated a process called harassment in fact they are able to produce faint but extended gaseous tails such lowmass starless tidal debris may become detached and appear as free floating clouds in the very deep hi surveys that are currently being carried out we show in this paper that these debris possess the same apparent properties as the socalled dark galaxies objects originally detected in hi with no optical counterpart and presumably dark matter dominated we present a numerical model of the prototype of such dark galaxies virgohi21 that is able to reproduce its main characteristics the onesided tail linking it to the spiral galaxy ngc 4254 the absence of stars and above all the reversal of the velocity gradient along the tail originally attributed to rotation motions caused by a massive dark matter halo and which we find to be consistent with simple streaming motions plus projection effects according to our numerical simulations this tidal debris was expelled 750 myr ago during a flyby at 1100 kms of ngc 4254 by a massive companion which should now lie at a projected distance of about 400 kpc a candidate for the intruder is discussed the existence of galaxies that have never been able to form stars had already been challenged based on theoretical and observational grounds tidal collisions in particular those occurring at high speed provide a much more simple explanation for the origin of such putative dark galaxies
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710.3868
Formation, Survival, and Destruction of Vortices in Accretion Disks
Two dimensional hydrodynamical disks are nonlinearly unstable to the formation of vortices. Once formed, these vortices essentially survive forever. What happens in three dimensions? We show with pseudospectral simulations that in 3D a vortex in a short box forms and survives just as in 2D. But a vortex in a tall box is unstable and is destroyed. In our simulation, the unstable vortex decays into a transient turbulent-like state that transports angular momentum outward at a nearly constant rate for hundreds of orbital times. The 3D instability that destroys vortices is a generalization of the 2D instability that forms them. We derive the conditions for these nonlinear instabilities to act by calculating the coupling between linear modes, and thereby derive the criterion for a vortex to survive in 3D as it does in 2D: the azimuthal extent of the vortex must be larger than the scale height of the accretion disk. When this criterion is violated, the vortex is unstable and decays. Because vortices are longer in azimuthal than in radial extent by a factor that is inversely proportional to their excess vorticity, a vortex with given radial extent will only survive in a 3D disk if it is sufficiently weak. This counterintuitive result explains why previous 3D simulations always yielded decaying vortices: their vortices were too strong. We conclude that in protoplanetary disks weak vortices can trap dust and serve as the nurseries of planet formation. Decaying strong vortices might be responsible for the outwards transport of angular momentum that is required to make accretion disks accrete.
astro-ph
two dimensional hydrodynamical disks are nonlinearly unstable to the formation of vortices once formed these vortices essentially survive forever what happens in three dimensions we show with pseudospectral simulations that in 3d a vortex in a short box forms and survives just as in 2d but a vortex in a tall box is unstable and is destroyed in our simulation the unstable vortex decays into a transient turbulentlike state that transports angular momentum outward at a nearly constant rate for hundreds of orbital times the 3d instability that destroys vortices is a generalization of the 2d instability that forms them we derive the conditions for these nonlinear instabilities to act by calculating the coupling between linear modes and thereby derive the criterion for a vortex to survive in 3d as it does in 2d the azimuthal extent of the vortex must be larger than the scale height of the accretion disk when this criterion is violated the vortex is unstable and decays because vortices are longer in azimuthal than in radial extent by a factor that is inversely proportional to their excess vorticity a vortex with given radial extent will only survive in a 3d disk if it is sufficiently weak this counterintuitive result explains why previous 3d simulations always yielded decaying vortices their vortices were too strong we conclude that in protoplanetary disks weak vortices can trap dust and serve as the nurseries of planet formation decaying strong vortices might be responsible for the outwards transport of angular momentum that is required to make accretion disks accrete
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710.3869
Khasminskii--Whitham averaging for randomly perturbed KdV equation
We consider the damped-driven KdV equation $$ \dot u-\nu{u_{xx}}+u_{xxx}-6uu_x=\sqrt\nu \eta(t,x), x\in S^1, \int u dx\equiv \int\eta dx\equiv0, $$ where $0<\nu\le1$ and the random process $\eta$ is smooth in $x$ and white in $t$. For any periodic function $u(x)$ let $ I=(I_1,I_2,...) $ be the vector, formed by the KdV integrals of motion, calculated for the potential $u(x)$. We prove that if $u(t,x)$ is a solution of the equation above, then for $0\le t\lesssim\nu^{-1}$ and $\nu\to0$ the vector $ I(t)=(I_1(u(t,\cdot)),I_2(u(t,\cdot)),...) $ satisfies the (Whitham) averaged equation.
math.AP math-ph math.MP
we consider the dampeddriven kdv equation dot unuu_xxu_xxx6uu_xsqrtnu etatx xin s1 int u dxequiv inteta dxequiv0 where 0nule1 and the random process eta is smooth in x and white in t for any periodic function ux let ii_1i_2 be the vector formed by the kdv integrals of motion calculated for the potential ux we prove that if utx is a solution of the equation above then for 0le tlesssimnu1 and nuto0 the vector iti_1utcdoti_2utcdot satisfies the whitham averaged equation
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710.387
The WKB method for conjugate points in the volumorphism group
In this paper, we are interested in the location of conjugate points along a geodesic in the volumorphism group of a compact three-dimensional manifold without boundary (the configuration space of an ideal fluid). As shown in the author's previous work, these are typically pathological, i.e., they can occur in clusters along a geodesic, unlike on finite-dimensional Riemannian manifolds. (This phenomenon does not occur for the volumorphism groups of two-dimensional manifolds, which are known to have discrete conjugate points along any geodesic by Ebin-Misiolek-Preston.) We give an explicit algorithm for finding them in terms of a certain ordinary differential equation, derived via the WKB-approximation methods of Lifschitz-Hameiri and Friedlander-Vishik. We prove that for a typical geodesic in the volumorphism group, there will be pathological conjugate point locations filling up closed intervals; hence typically the zeroes of Jacobi fields on the volumorphism group are dense in intervals.
math.AP math.DG
in this paper we are interested in the location of conjugate points along a geodesic in the volumorphism group of a compact threedimensional manifold without boundary the configuration space of an ideal fluid as shown in the authors previous work these are typically pathological ie they can occur in clusters along a geodesic unlike on finitedimensional riemannian manifolds this phenomenon does not occur for the volumorphism groups of twodimensional manifolds which are known to have discrete conjugate points along any geodesic by ebinmisiolekpreston we give an explicit algorithm for finding them in terms of a certain ordinary differential equation derived via the wkbapproximation methods of lifschitzhameiri and friedlandervishik we prove that for a typical geodesic in the volumorphism group there will be pathological conjugate point locations filling up closed intervals hence typically the zeroes of jacobi fields on the volumorphism group are dense in intervals
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710.3871
Algebraic Geometry over Free Metabelian Lie Algebra I: U-Algebras and Universal Classes
This paper is the first in a series of three, the aim of which is to lay the foundations of algebraic geometry over the free metabelian Lie algebra $F$. In the current paper we introduce the notion of a metabelian Lie $U$-algebra and establish connections between metabelian Lie $U$-algebras and special matrix Lie algebras. We define the $\Delta $-localisation of a metabelian Lie $U$-algebra $A$ and the direct module extension of the Fitting's radical of $A$ and show that these algebras lie in the universal closure of $A$.
math.AG math.LO
this paper is the first in a series of three the aim of which is to lay the foundations of algebraic geometry over the free metabelian lie algebra f in the current paper we introduce the notion of a metabelian lie ualgebra and establish connections between metabelian lie ualgebras and special matrix lie algebras we define the delta localisation of a metabelian lie ualgebra a and the direct module extension of the fittings radical of a and show that these algebras lie in the universal closure of a
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710.3872
Algebraic Geometry over Free Metabelian Lie Algebra II: Finite Field Case
This paper is the second in a series of three, the aim of which is to construct algebraic geometry over a free metabelian Lie algebra $F$. For the universal closure of free metabelian Lie algebra of finite rank $r \ge 2$ over a finite field $k$ we find a convenient set of axioms in the language of Lie algebras $L$ and the language $L_{F}$ enriched by constants from $F$. We give a description of: * The structure of finitely generated algebras from the universal closure of $F_r$ in both $L$ and $L_{F_r}$ * The structure of irreducible algebraic sets over $F_r $ and respective coordinate algebras. We also prove that the universal theory of a free metabelian Lie algebra over a finite field is decidable in both languages.
math.AG math.LO
this paper is the second in a series of three the aim of which is to construct algebraic geometry over a free metabelian lie algebra f for the universal closure of free metabelian lie algebra of finite rank r ge 2 over a finite field k we find a convenient set of axioms in the language of lie algebras l and the language l_f enriched by constants from f we give a description of the structure of finitely generated algebras from the universal closure of f_r in both l and l_f_r the structure of irreducible algebraic sets over f_r and respective coordinate algebras we also prove that the universal theory of a free metabelian lie algebra over a finite field is decidable in both languages
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710.3873
Semidomains and Metabelian Product of Metabelian Lie Algebras
This paper is the third in a series of papers, the aim of which is to construct algebraic geometry over metabelian Lie algebras.
math.AG math.LO
this paper is the third in a series of papers the aim of which is to construct algebraic geometry over metabelian lie algebras
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710.3874
Equilibrium sequences of non rotating and rapidly rotating crystalline color superconducting hybrid stars
The three-flavor crystalline color-superconducting (CCS) phase of quantum chromodynamics (QCD) is a candidate phase for the ground state of cold matter at moderate densities above the density of the deconfinement phase transition. Apart from being a superfluid, the CCS phase has properties of a solid, such as a lattice structure and a shear modulus, and hence the ability to sustain multipolar deformations in gravitational equilibrium. We construct equilibrium configurations of hybrid stars composed of nuclear matter at low, and CCS quark matter at high, densities. Phase equilibrium between these phases is possible only for rather stiff equations of state of nuclear matter and large couplings in the effective Nambu--Jona-Lasinio Lagrangian describing the CCS state. We identify a new branch of stable CCS hybrid stars within a broad range of central densities which, depending on the details of the equations of state, either bifurcate from the nuclear sequence of stars when the central density exceeds that of the deconfinement phase transition or form a new family of configurations separated from the purely nuclear sequence by an instability region. The maximum masses of our non-rotating hybrid configurations are consistent with the presently available astronomical bounds. The sequences of hybrid configurations that rotate near the mass-shedding limit are found to be more compact and thus support substantially larger spins than their same mass nuclear counterparts.
astro-ph cond-mat.supr-con hep-ph nucl-th
the threeflavor crystalline colorsuperconducting ccs phase of quantum chromodynamics qcd is a candidate phase for the ground state of cold matter at moderate densities above the density of the deconfinement phase transition apart from being a superfluid the ccs phase has properties of a solid such as a lattice structure and a shear modulus and hence the ability to sustain multipolar deformations in gravitational equilibrium we construct equilibrium configurations of hybrid stars composed of nuclear matter at low and ccs quark matter at high densities phase equilibrium between these phases is possible only for rather stiff equations of state of nuclear matter and large couplings in the effective nambujonalasinio lagrangian describing the ccs state we identify a new branch of stable ccs hybrid stars within a broad range of central densities which depending on the details of the equations of state either bifurcate from the nuclear sequence of stars when the central density exceeds that of the deconfinement phase transition or form a new family of configurations separated from the purely nuclear sequence by an instability region the maximum masses of our nonrotating hybrid configurations are consistent with the presently available astronomical bounds the sequences of hybrid configurations that rotate near the massshedding limit are found to be more compact and thus support substantially larger spins than their same mass nuclear counterparts
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710.3875
Dielectric loss of 2D metal-insulator composite near the percolation threshold
The frequency dependence of the dielectric loss angle for a metal-insulator composite was shown previously to be an efficient method to experimentally determine the percolation threshold. The statistical properties of this angle are found here to be similar to those of the critical links (supporting the total current) near the percolation threshold close to dc and for very high frequencies. A further discussion is provided about the way to connect this angle to the critical links. The second aim of these studies is to connect the frequency dependence of this angle to the proportion of the conductor or dielectric phase in this composite.
cond-mat.mtrl-sci
the frequency dependence of the dielectric loss angle for a metalinsulator composite was shown previously to be an efficient method to experimentally determine the percolation threshold the statistical properties of this angle are found here to be similar to those of the critical links supporting the total current near the percolation threshold close to dc and for very high frequencies a further discussion is provided about the way to connect this angle to the critical links the second aim of these studies is to connect the frequency dependence of this angle to the proportion of the conductor or dielectric phase in this composite
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710.3876
Acoustic Kappa-Density Fluctuation Waves in Suprathermal Kappa Function Fluids
We describe a new wave mode similar to the acoustic wave in which both density and velocity fluctuate. Unlike the acoustic wave in which the underlying distribution is Maxwellian, this new wave mode occurs when the underlying distribution is a suprathermal kappa function and involves fluctuations in the power law index, kappa. This wave mode always propagates faster than the acoustic wave with an equivalent effective temperature and becomes the acoustic wave in the Maxwellian limit as kappa goes to infinity.
astro-ph
we describe a new wave mode similar to the acoustic wave in which both density and velocity fluctuate unlike the acoustic wave in which the underlying distribution is maxwellian this new wave mode occurs when the underlying distribution is a suprathermal kappa function and involves fluctuations in the power law index kappa this wave mode always propagates faster than the acoustic wave with an equivalent effective temperature and becomes the acoustic wave in the maxwellian limit as kappa goes to infinity
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710.3877
Quasirandom groups
Babai and S\'os have asked whether there exists a constant c>0 such that every finite group G has a product-free subset of size at least c|G|: that is, a subset X that does not contain three elements x, y and z with xy=z. In this paper we show that the answer is no. Moreover, we give a simple sufficient condition for a group not to have any large product-free subset.
math.CO math.GR
babai and sos have asked whether there exists a constant c0 such that every finite group g has a productfree subset of size at least cg that is a subset x that does not contain three elements x y and z with xyz in this paper we show that the answer is no moreover we give a simple sufficient condition for a group not to have any large productfree subset
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710.3878
Fundamental Solutions for Wave Equation in de Sitter Model of Universe
In this article we construct the fundamental solutions for the wave equation arising in the de Sitter model of the universe. We use the fundamental solutions to represent solutions of the Cauchy problem and to prove the $L^p-L^q$-decay estimates for the solutions of the equation with and without a source term.
math.AP math-ph math.MP
in this article we construct the fundamental solutions for the wave equation arising in the de sitter model of the universe we use the fundamental solutions to represent solutions of the cauchy problem and to prove the lplqdecay estimates for the solutions of the equation with and without a source term
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710.3879
On Penrose's `before the big bang' ideas
We point out that algebraically special Einstein fields with twisting rays exhibit the basic properties of conformal Universes considered recently by Roger Penrose.
gr-qc math.DG
we point out that algebraically special einstein fields with twisting rays exhibit the basic properties of conformal universes considered recently by roger penrose
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710.388
Galileo satellite constellation and extensions to General Relativity
We consider the impact of some known extensions of General Relativity in observables that will be available with the Galileo positioning systems, and draw conclusions as to the possibility of measuring them. We specifically address the effects of the presence of a cosmological constant, a Yukawa-like addition to the Newtonian potential, and the existence of an extra, constant acceleration. We also consider the phenomenological impact of a broad class of metric theories, which can be classified through the parameterized Post-Newtonian formalism.
gr-qc
we consider the impact of some known extensions of general relativity in observables that will be available with the galileo positioning systems and draw conclusions as to the possibility of measuring them we specifically address the effects of the presence of a cosmological constant a yukawalike addition to the newtonian potential and the existence of an extra constant acceleration we also consider the phenomenological impact of a broad class of metric theories which can be classified through the parameterized postnewtonian formalism
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710.3881
The relation between the quantum games, communication complexity problems and Bell inequalities
We study the relation between the quantum games, communication complexity problems and Bell inequalities. In particular we are interested in answering the question whether for every element of one of these groups there is a corresponding element in the other two. We show that there are cases where there is no such relation. Moreover, in the communication complexity problems for which there is no Bell inequality the advantage of the quantum strategies over the classical ones is much higher.
quant-ph
we study the relation between the quantum games communication complexity problems and bell inequalities in particular we are interested in answering the question whether for every element of one of these groups there is a corresponding element in the other two we show that there are cases where there is no such relation moreover in the communication complexity problems for which there is no bell inequality the advantage of the quantum strategies over the classical ones is much higher
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710.3882
Special types of intuitionistic fuzzy left h-ideals of hemirings
Characteristic, normal and completely normal intuitionistic fuzzy left $h$-ideals of hemirings are described.
math.RA
characteristic normal and completely normal intuitionistic fuzzy left hideals of hemirings are described
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710.3883
Axion Inflation in Type II String Theory
Inflationary models driven by a large number of axion fields are discussed in the context of type IIB compactifications with N=1 supersymmetry. The inflatons arise as the scalar modes of the R-R two-forms evaluated on vanishing two-cycles in the compact geometry. The vanishing cycles are resolved by small two-volumes or NS-NS B-fields which sit together with the inflatons in the same supermultiplets. String world-sheets wrapping the vanishing cycles correct the metric of the R-R inflatons. They can help to generate kinetic terms close to the Planck scale and a mass hierarchy between the axions and their non-axionic partners during inflation. At small string coupling, D-brane corrections are subleading in the metric of the R-R inflatons. However, an axion potential can be generated by D1 instantons or gaugino condensates on D5 branes. Models with sufficiently large number of axions admit regions of chaotic inflation which can stretch over the whole axion field range for potentials from gaugino condensates. These models could allow for a possibly detectable amount of gravitational waves with tensor to scalar ratio as high as r<0.14.
hep-th astro-ph hep-ph
inflationary models driven by a large number of axion fields are discussed in the context of type iib compactifications with n1 supersymmetry the inflatons arise as the scalar modes of the rr twoforms evaluated on vanishing twocycles in the compact geometry the vanishing cycles are resolved by small twovolumes or nsns bfields which sit together with the inflatons in the same supermultiplets string worldsheets wrapping the vanishing cycles correct the metric of the rr inflatons they can help to generate kinetic terms close to the planck scale and a mass hierarchy between the axions and their nonaxionic partners during inflation at small string coupling dbrane corrections are subleading in the metric of the rr inflatons however an axion potential can be generated by d1 instantons or gaugino condensates on d5 branes models with sufficiently large number of axions admit regions of chaotic inflation which can stretch over the whole axion field range for potentials from gaugino condensates these models could allow for a possibly detectable amount of gravitational waves with tensor to scalar ratio as high as r014
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710.3884
Fuzzy n-ary groups as a generalization of Rosenfeld's fuzzy groups
The notion of an $n$-ary group is a natural generalization of the notion of a group and has many applications in different branches. In this paper, the notion of (normal) fuzzy $n$-ary subgroup of an $n$-ary group is introduced and some related properties are investigated. Characterizations of fuzzy $n$-ary subgroups are given.
math.RA
the notion of an nary group is a natural generalization of the notion of a group and has many applications in different branches in this paper the notion of normal fuzzy nary subgroup of an nary group is introduced and some related properties are investigated characterizations of fuzzy nary subgroups are given
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710.3885
Differentiating dark energy and modified gravity with galaxy redshift surveys
The observed cosmic acceleration today could be due to an unknown energy component (dark energy), or a modification to general relativity (modified gravity). If dark energy models and modified gravity models are required to predict the same cosmic expansion history H(z), they will predict different growth rate for cosmic large scale structure, f_g(z)=d\ln \delta/d\ln a (\delta=(\rho_m-\bar{\rho_m})/\bar{\rho_m}), a is the cosmic scale factor). If gravity is not modified, the measured H(z) leads to a unique prediction for f_g(z), f_g^H(z). Comparing f_g^H(z) with the measured f_g(z) provides a transparent and straightforward test of gravity. We show that a simple \chi^2 test provides a general figure-of-merit for our ability to distinguish between dark energy and modified gravity given the measured H(z) and f_g(z). We study a magnitude-limited NIR galaxy redshift survey covering >10,000 (deg)^2 and the redshift range of 0.5<z<2. The resultant data can be divided into 7 redshift bins, and yield the measurement of H(z) to the accuracy of 1-2% via baryon acoustic oscillation measurements, and f_g(z) to the accuracy of a few percent via the measurement of redshift space distortions and the bias factor which describes how light traces mass. We find that if the H(z) data are fit by both a DGP gravity model and an equivalent dark energy model that predict the same expansion history, a survey area of 11,931 (deg)^2 is required to rule out the DGP gravity model at the 99.99% confidence level. It is feasible for such a galaxy redshift survey to be carried out by the next generation space missions from NASA and ESA, and it will revolutionize our understanding of the universe by differentiating between dark energy and modified gravity.
astro-ph gr-qc hep-ph
the observed cosmic acceleration today could be due to an unknown energy component dark energy or a modification to general relativity modified gravity if dark energy models and modified gravity models are required to predict the same cosmic expansion history hz they will predict different growth rate for cosmic large scale structure f_gzdln deltadln a deltarho_mbarrho_mbarrho_m a is the cosmic scale factor if gravity is not modified the measured hz leads to a unique prediction for f_gz f_ghz comparing f_ghz with the measured f_gz provides a transparent and straightforward test of gravity we show that a simple chi2 test provides a general figureofmerit for our ability to distinguish between dark energy and modified gravity given the measured hz and f_gz we study a magnitudelimited nir galaxy redshift survey covering 10000 deg2 and the redshift range of 05z2 the resultant data can be divided into 7 redshift bins and yield the measurement of hz to the accuracy of 12 via baryon acoustic oscillation measurements and f_gz to the accuracy of a few percent via the measurement of redshift space distortions and the bias factor which describes how light traces mass we find that if the hz data are fit by both a dgp gravity model and an equivalent dark energy model that predict the same expansion history a survey area of 11931 deg2 is required to rule out the dgp gravity model at the 9999 confidence level it is feasible for such a galaxy redshift survey to be carried out by the next generation space missions from nasa and esa and it will revolutionize our understanding of the universe by differentiating between dark energy and modified gravity
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710.3886
alpha'^2-corrections to extremal dyonic black holes in heterotic string theory
We calculate alpha'^2-corrections to the entropy of the 5-dimensional 3-charge and the 4-dimensional 4-charge large extremal black holes using the low energy effective action of the heterotic string theory. In the 4-dimensional case, our results are in agreement with the microscopic statistical entropy both for the BPS and the non-BPS black holes. In the more interesting 5-dimensional case, where the direct microscopic stringy description is still unknown, our results for the BPS black holes are in agreement with the results obtained from the action supplemented with R^2-correction obtained by supersymmetric completion of the gravitational Chern-Simons term. This agreement does not extend to the non-BPS black holes, for which we propose a different expression for the entropy. We show that the new expression is supported by certain alpha'^3-order calculations, and by the arguments based on the AdS/CFT correspondence.
hep-th
we calculate alpha2corrections to the entropy of the 5dimensional 3charge and the 4dimensional 4charge large extremal black holes using the low energy effective action of the heterotic string theory in the 4dimensional case our results are in agreement with the microscopic statistical entropy both for the bps and the nonbps black holes in the more interesting 5dimensional case where the direct microscopic stringy description is still unknown our results for the bps black holes are in agreement with the results obtained from the action supplemented with r2correction obtained by supersymmetric completion of the gravitational chernsimons term this agreement does not extend to the nonbps black holes for which we propose a different expression for the entropy we show that the new expression is supported by certain alpha3order calculations and by the arguments based on the adscft correspondence
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710.3887
Ultra LI-ideals in lattice implication algebras and MTL-algebras
A mistake concerning the ultra \textit{LI}-ideal of a lattice implication algebra is pointed out, and some new sufficient and necessary conditions for an \textit{LI}-ideal to be an ultra \textit{LI}-ideal are given. Moreover, the notion of an \textit{LI}-ideal is extended to MTL-algebras, the notions of a (prime, ultra, obstinate, Boolean) \textit{LI}-ideal and an \textit{ILI}-ideal of an MTL-algebra are introduced, some important examples are given, and the following notions are proved to be equivalent in MTL-algebra: (1) prime proper \textit{LI}-ideal and Boolean \textit{LI}-ideal, (2) prime proper \textit{LI}-ideal and \textit{ILI}-ideal, (3) proper obstinate \textit{LI}-ideal, (4) ultra \textit{LI}-ideal.
math.LO math.GM
a mistake concerning the ultra textitliideal of a lattice implication algebra is pointed out and some new sufficient and necessary conditions for an textitliideal to be an ultra textitliideal are given moreover the notion of an textitliideal is extended to mtlalgebras the notions of a prime ultra obstinate boolean textitliideal and an textitiliideal of an mtlalgebra are introduced some important examples are given and the following notions are proved to be equivalent in mtlalgebra 1 prime proper textitliideal and boolean textitliideal 2 prime proper textitliideal and textitiliideal 3 proper obstinate textitliideal 4 ultra textitliideal
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710.3888
Cooperative Multi-Cell Networks: Impact of Limited-Capacity Backhaul and Inter-Users Links
Cooperative technology is expected to have a great impact on the performance of cellular or, more generally, infrastructure networks. Both multicell processing (cooperation among base stations) and relaying (cooperation at the user level) are currently being investigated. In this presentation, recent results regarding the performance of multicell processing and user cooperation under the assumption of limited-capacity interbase station and inter-user links, respectively, are reviewed. The survey focuses on related results derived for non-fading uplink and downlink channels of simple cellular system models. The analytical treatment, facilitated by these simple setups, enhances the insight into the limitations imposed by limited-capacity constraints on the gains achievable by cooperative techniques.
cs.IT math.IT
cooperative technology is expected to have a great impact on the performance of cellular or more generally infrastructure networks both multicell processing cooperation among base stations and relaying cooperation at the user level are currently being investigated in this presentation recent results regarding the performance of multicell processing and user cooperation under the assumption of limitedcapacity interbase station and interuser links respectively are reviewed the survey focuses on related results derived for nonfading uplink and downlink channels of simple cellular system models the analytical treatment facilitated by these simple setups enhances the insight into the limitations imposed by limitedcapacity constraints on the gains achievable by cooperative techniques
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710.3889
Epigenetic Chromatin Silencing: Bistability and Front Propagation
The role of post-translational modification of histones in eukaryotic gene regulation is well recognized. Epigenetic silencing of genes via heritable chromatin modifications plays a major role in cell fate specification in higher organisms. We formulate a coarse-grained model of chromatin silencing in yeast and study the conditions under which the system becomes bistable, allowing for different epigenetic states. We also study the dynamics of the boundary between the two locally stable states of chromatin: silenced and unsilenced. The model could be of use in guiding the discussion on chromatin silencing in general. In the context of silencing in budding yeast, it helps us understand the phenotype of various mutants, some of which may be non-trivial to see without the help of a mathematical model. One such example is a mutation that reduces the rate of background acetylation of particular histone side-chains that competes with the deacetylation by Sir2p. The resulting negative feedback due to a Sir protein depletion effect gives rise to interesting counter-intuitive consequences. Our mathematical analysis brings forth the different dynamical behaviors possible within the same molecular model and guides the formulation of more refined hypotheses that could be addressed experimentally.
q-bio.MN
the role of posttranslational modification of histones in eukaryotic gene regulation is well recognized epigenetic silencing of genes via heritable chromatin modifications plays a major role in cell fate specification in higher organisms we formulate a coarsegrained model of chromatin silencing in yeast and study the conditions under which the system becomes bistable allowing for different epigenetic states we also study the dynamics of the boundary between the two locally stable states of chromatin silenced and unsilenced the model could be of use in guiding the discussion on chromatin silencing in general in the context of silencing in budding yeast it helps us understand the phenotype of various mutants some of which may be nontrivial to see without the help of a mathematical model one such example is a mutation that reduces the rate of background acetylation of particular histone sidechains that competes with the deacetylation by sir2p the resulting negative feedback due to a sir protein depletion effect gives rise to interesting counterintuitive consequences our mathematical analysis brings forth the different dynamical behaviors possible within the same molecular model and guides the formulation of more refined hypotheses that could be addressed experimentally
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710.389
The genus of a curve of Fermat type
In this paper we begin to study curves on a weighted projective plane with one trivial weight, ${\mathbb P}(1,m,n)$, by determining the genus of curves of Fermat type. These are curves defined by a ``homogeneous'' polynomial analagous to the one from Fermat's last theorem. We begin by finding local coordinates for the standard affine cover of the plane, and then prove that the curve is smooth. This is done by pulling the curve up to the surface's desingularization. Then a map from the curve to ${\mathbb P^1}$ is constructed, and it's ramification divisor is determined. We conclude by applying Hurwitz's theorem to this map to obtain $C$'s genus.
math.AG
in this paper we begin to study curves on a weighted projective plane with one trivial weight mathbb p1mn by determining the genus of curves of fermat type these are curves defined by a homogeneous polynomial analagous to the one from fermats last theorem we begin by finding local coordinates for the standard affine cover of the plane and then prove that the curve is smooth this is done by pulling the curve up to the surfaces desingularization then a map from the curve to mathbb p1 is constructed and its ramification divisor is determined we conclude by applying hurwitzs theorem to this map to obtain cs genus
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710.3891
Analysis of Critical State Response in Thin Films by ac Susceptibility Measurements
Harmonic analysis of the temperature dependence of the nonlinear ac susceptibility of Nb thin film gives excellent agreement with the susceptibility calculated on basis of model of the hysteretic critical state in 2D disk.
cond-mat.supr-con
harmonic analysis of the temperature dependence of the nonlinear ac susceptibility of nb thin film gives excellent agreement with the susceptibility calculated on basis of model of the hysteretic critical state in 2d disk
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710.3892
Maturity-independent risk measures
The new notion of maturity-independent risk measures is introduced and contrasted with the existing risk measurement concepts. It is shown, by means of two examples, one set on a finite probability space and the other in a diffusion framework, that, surprisingly, some of the widely utilized risk measures cannot be used to build maturity-independent counterparts. We construct a large class of maturity-independent risk measures and give representative examples in both continuous- and discrete-time financial models.
q-fin.RM math.OC math.PR
the new notion of maturityindependent risk measures is introduced and contrasted with the existing risk measurement concepts it is shown by means of two examples one set on a finite probability space and the other in a diffusion framework that surprisingly some of the widely utilized risk measures cannot be used to build maturityindependent counterparts we construct a large class of maturityindependent risk measures and give representative examples in both continuous and discretetime financial models
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710.3893
Mass limits for heavy neutrinos
Neutrinos heavier than $M_Z/2\sim 45$ GeV are not excluded by particle physics data. Stable neutrinos heavier than this might contribute to the cosmic gamma ray background through annihilation in distant galaxies as well as to the dark matter content of the universe. We calculate the evolution of the heavy neutrino density in the universe as a function of its mass, $M_N$, and then the subsequent gamma ray spectrum from annihilation of distant $N\bar{N}$ (from $0<z<5$). The evolution of the heavy neutrino density in the universe is calculated numerically. In order to obtain the enhancement due to structure formation in the universe, we approximate the distribution of $N$ to be proportional to that of dark matter in the GalICS model. The calculated gamma ray spectrum is compared to the measured EGRET data. A conservative exclusion region for the heavy neutrino mass is 100 to 200 GeV, both from EGRET data and our re-evalutation of the Kamiokande data. The heavy neutrino contribution to dark matter is found to be at most 15%.
astro-ph
neutrinos heavier than m_z2sim 45 gev are not excluded by particle physics data stable neutrinos heavier than this might contribute to the cosmic gamma ray background through annihilation in distant galaxies as well as to the dark matter content of the universe we calculate the evolution of the heavy neutrino density in the universe as a function of its mass m_n and then the subsequent gamma ray spectrum from annihilation of distant nbarn from 0z5 the evolution of the heavy neutrino density in the universe is calculated numerically in order to obtain the enhancement due to structure formation in the universe we approximate the distribution of n to be proportional to that of dark matter in the galics model the calculated gamma ray spectrum is compared to the measured egret data a conservative exclusion region for the heavy neutrino mass is 100 to 200 gev both from egret data and our reevalutation of the kamiokande data the heavy neutrino contribution to dark matter is found to be at most 15
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710.3894
Upper and lower bounds on resonances for manifolds hyperbolic near infinity
For a conformally compact manifold that is hyperbolic near infinity and of dimension $n+1$, we complete the proof of the optimal $O(r^{n+1})$ upper bound on the resonance counting function, correcting a mistake in the existing literature. In the case of a compactly supported perturbation of a hyperbolic manifold, we establish a Poisson formula expressing the regularized wave trace as a sum over scattering resonances. This leads to an $r^{n+1}$ lower bound on the counting function for scattering poles.
math.SP math.DG
for a conformally compact manifold that is hyperbolic near infinity and of dimension n1 we complete the proof of the optimal orn1 upper bound on the resonance counting function correcting a mistake in the existing literature in the case of a compactly supported perturbation of a hyperbolic manifold we establish a poisson formula expressing the regularized wave trace as a sum over scattering resonances this leads to an rn1 lower bound on the counting function for scattering poles
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710.3895
Thermal/quantum effects and induced superstring cosmologies
We consider classical superstring theories on flat four dimensional space-times, and where N=4 or N=2 supersymmetry is spontaneously broken. We obtain the thermal and quantum corrections at the string one-loop level and show that the back-reaction on the space-time metric induces a cosmological evolution. We concentrate on heterotic string models obtained by compactification on a T^6 torus and on T^6/Z_2 orbifolds. The temperature T and the supersymmetry breaking scale M are generated via the Scherk-Schwarz mechanism on the Euclidean time cycle and on an internal spatial cycle respectively. The effective field theory corresponds to a no-scale supergravity, where the corresponding no-scale modulus controls the Susy-breaking scale. The classical flatness of this modulus is lifted by an effective thermal potential, given by the free energy. The gravitational field equations admit solutions where M, T and the inverse scale factor 1/a of the universe remain proportional. In particular the ratio M/T is fixed during the time evolution. The induced cosmology is governed by a Friedmann-Hubble equation involving an effective radiation term ~1/a^4 and an effective curvature term ~1/a^2, whose coefficients are functions of the complex structure ratio M/T.
hep-th gr-qc hep-ph
we consider classical superstring theories on flat four dimensional spacetimes and where n4 or n2 supersymmetry is spontaneously broken we obtain the thermal and quantum corrections at the string oneloop level and show that the backreaction on the spacetime metric induces a cosmological evolution we concentrate on heterotic string models obtained by compactification on a t6 torus and on t6z_2 orbifolds the temperature t and the supersymmetry breaking scale m are generated via the scherkschwarz mechanism on the euclidean time cycle and on an internal spatial cycle respectively the effective field theory corresponds to a noscale supergravity where the corresponding noscale modulus controls the susybreaking scale the classical flatness of this modulus is lifted by an effective thermal potential given by the free energy the gravitational field equations admit solutions where m t and the inverse scale factor 1a of the universe remain proportional in particular the ratio mt is fixed during the time evolution the induced cosmology is governed by a friedmannhubble equation involving an effective radiation term 1a4 and an effective curvature term 1a2 whose coefficients are functions of the complex structure ratio mt
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710.3896
Verifying the Cosmological Utility of Type Ia Supernovae: Implications of a Dispersion in the Ultraviolet Spectra
We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae (SNe Ia) and its dispersion using high signal-to-noise Keck-I/LRIS-B spectroscopy for a sample of 36 events at intermediate redshift (z=0.5) discovered by the Canada-France-Hawaii Telescope Supernova Legacy Survey (SNLS). We introduce a new method for removing host galaxy contamination in our spectra, exploiting the comprehensive photometric coverage of the SNLS SNe and their host galaxies, thereby providing the first quantitative view of the UV spectral properties of a large sample of distant SNe Ia. Although the mean SN Ia spectrum has not evolved significantly over the past 40% of cosmic history, precise evolutionary constraints are limited by the absence of a comparable sample of high quality local spectra. Within the high-redshift sample, we discover significant UV spectral variations and exclude dust extinction as the primary cause by examining trends with the optical SN color. Although progenitor metallicity may drive some of these trends, the variations we see are much larger than predicted in recent models and do not follow expected patterns. An interesting new result is a variation seen in the wavelength of selected UV features with phase. We also demonstrate systematic differences in the SN Ia spectral features with SN light curve width in both the UV and the optical. We show that these intrinsic variations could represent a statistical limitation in the future use of high-redshift SNe Ia for precision cosmology. We conclude that further detailed studies are needed, both locally and at moderate redshift where the rest-frame UV can be studied precisely, in order that future missions can confidently be planned to fully exploit SNe Ia as cosmological probes [ABRIDGED].
astro-ph
we analyze the mean restframe ultraviolet uv spectrum of type ia supernovae sne ia and its dispersion using high signaltonoise keckilrisb spectroscopy for a sample of 36 events at intermediate redshift z05 discovered by the canadafrancehawaii telescope supernova legacy survey snls we introduce a new method for removing host galaxy contamination in our spectra exploiting the comprehensive photometric coverage of the snls sne and their host galaxies thereby providing the first quantitative view of the uv spectral properties of a large sample of distant sne ia although the mean sn ia spectrum has not evolved significantly over the past 40 of cosmic history precise evolutionary constraints are limited by the absence of a comparable sample of high quality local spectra within the highredshift sample we discover significant uv spectral variations and exclude dust extinction as the primary cause by examining trends with the optical sn color although progenitor metallicity may drive some of these trends the variations we see are much larger than predicted in recent models and do not follow expected patterns an interesting new result is a variation seen in the wavelength of selected uv features with phase we also demonstrate systematic differences in the sn ia spectral features with sn light curve width in both the uv and the optical we show that these intrinsic variations could represent a statistical limitation in the future use of highredshift sne ia for precision cosmology we conclude that further detailed studies are needed both locally and at moderate redshift where the restframe uv can be studied precisely in order that future missions can confidently be planned to fully exploit sne ia as cosmological probes abridged
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710.3897
Constraining Muon Internal Bremsstrahlung as a Contribution to the MiniBooNE Low Energy Excess
Using a cleanly tagged data sample of $\nu_\mu$ charged current events, it is demonstrated that the rate at which such events are mis-identified as $\nu_e$'s is accurately simulated in the MiniBooNE $\nu_\mu \to \nu_e$ analysis. Such mis-identification, which could arise from muon internal bremsstrahlung, is decisively ruled out as a source of the low energy electron-like events reported in the MiniBooNE search for $\nu_\mu \to \nu_e$ oscillations. This refutes the conclusions of a recent paper which postulates that hard bremsstrahlung could form a substantial background to the MiniBooNE $\nu_e$ sample.
hep-ex
using a cleanly tagged data sample of nu_mu charged current events it is demonstrated that the rate at which such events are misidentified as nu_es is accurately simulated in the miniboone nu_mu to nu_e analysis such misidentification which could arise from muon internal bremsstrahlung is decisively ruled out as a source of the low energy electronlike events reported in the miniboone search for nu_mu to nu_e oscillations this refutes the conclusions of a recent paper which postulates that hard bremsstrahlung could form a substantial background to the miniboone nu_e sample
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710.3898
Around MOND: Lagrangians, Hubble Equations, Perturbations and External Field Effect
The MOdified Newtonian Dynamics (MOND) is presented here, as well as a theory that can be linked to it: the theory of the Aether, a four-vector field breaking Lorentz invariance. The form of its Lagrangian is studied, then basic equations of the theory are rederived in a detailed way, and calculated for different metrics, exploring the impact of non-zero spatial terms of the Aether. A brief attempt of making the Aether Lagrangian depend on a scalar field is presented. An analytic solving of a galaxy model with an external field is described, which highlights the MONDian external field effect that breaks the strong equivalence principle.
astro-ph
the modified newtonian dynamics mond is presented here as well as a theory that can be linked to it the theory of the aether a fourvector field breaking lorentz invariance the form of its lagrangian is studied then basic equations of the theory are rederived in a detailed way and calculated for different metrics exploring the impact of nonzero spatial terms of the aether a brief attempt of making the aether lagrangian depend on a scalar field is presented an analytic solving of a galaxy model with an external field is described which highlights the mondian external field effect that breaks the strong equivalence principle
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710.3899
Possible Enhanced Flux of Glassy Solid Helium in Cylindrical Corrugated Nanopores
By using the glassy (helium-)fluid model and boundary perturbation method, we can obtain the velocity fields (as well as the flow rate; up to the second order) inside the wavy-rough cylindrical nanopores which are of the same size as those samples prepared by Kim and Chan as well as Day {\it et al.} Our results show that the velocities measured in porous Vycor samples could be reproduced by carefully selecting relevant parameters but those in glass capillaries are difficult to obtain.
cond-mat.other cond-mat.dis-nn
by using the glassy heliumfluid model and boundary perturbation method we can obtain the velocity fields as well as the flow rate up to the second order inside the wavyrough cylindrical nanopores which are of the same size as those samples prepared by kim and chan as well as day it et al our results show that the velocities measured in porous vycor samples could be reproduced by carefully selecting relevant parameters but those in glass capillaries are difficult to obtain
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710.39
Law without Law
We consider a model for spacetime in which there is an ubiquitous background Dark Energy which is the Zero Point Field. This is further modeled in terms of a Weiner process that leads to a Random or Brownian characterization. Nevertheless we are able to recover meaningful physics, very much in the spirit of Wheeler's Law without Law, that is laws emerging from an underpinning of lawlessness.
physics.gen-ph
we consider a model for spacetime in which there is an ubiquitous background dark energy which is the zero point field this is further modeled in terms of a weiner process that leads to a random or brownian characterization nevertheless we are able to recover meaningful physics very much in the spirit of wheelers law without law that is laws emerging from an underpinning of lawlessness
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710.3901
A recursive linear time modular decomposition algorithm via LexBFS
A module of a graph G is a set of vertices that have the same set of neighbours outside. Modules of a graphs form a so-called partitive family and thereby can be represented by a unique tree MD(G), called the modular decomposition tree. Motivated by the central role of modules in numerous algorithmic graph theory questions, the problem of efficiently computing MD(G) has been investigated since the early 70's. To date the best algorithms run in linear time but are all rather complicated. By combining previous algorithmic paradigms developed for the problem, we are able to present a simpler linear-time that relies on very simple data-structures, namely slice decomposition and sequences of rooted ordered trees.
cs.DM
a module of a graph g is a set of vertices that have the same set of neighbours outside modules of a graphs form a socalled partitive family and thereby can be represented by a unique tree mdg called the modular decomposition tree motivated by the central role of modules in numerous algorithmic graph theory questions the problem of efficiently computing mdg has been investigated since the early 70s to date the best algorithms run in linear time but are all rather complicated by combining previous algorithmic paradigms developed for the problem we are able to present a simpler lineartime that relies on very simple datastructures namely slice decomposition and sequences of rooted ordered trees
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710.3902
Strangeness and bulk freeze-out properties at RHIC
Identified charged kaon, pion, and proton spectra and ratios from sqrt(s_NN) = 200 and 62.4 GeV Cu+Cu collisions are studied with a hydro-motivated blast-wave and a statistical model framework in order to explore the strangeness production at RHIC and characterize the bulk freeze-out properties of the created system. The spectra are measured at mid-rapidity |y|<0.1 over the transverse momentum range of 0.25 < p_T < 1.2 GeV/c with particle identification derived from the ionization energy loss in the STAR Time Projection Chamber. The multi-dimensional systematic study of pi(+/-), K(+/-), p and pbar production in Cu+Cu, Au+Au, d+Au and p+p collisions is used to discuss the energy, system size and inferred energy density dependence of freeze-out parameters and strangeness production. The new data from Cu+Cu collisions bridge the gap between the smaller d+Au and larger Au+Au systems, allowing a detailed study of the onset of strangeness equilibration at RHIC.
nucl-ex
identified charged kaon pion and proton spectra and ratios from sqrts_nn 200 and 624 gev cucu collisions are studied with a hydromotivated blastwave and a statistical model framework in order to explore the strangeness production at rhic and characterize the bulk freezeout properties of the created system the spectra are measured at midrapidity y01 over the transverse momentum range of 025 p_t 12 gevc with particle identification derived from the ionization energy loss in the star time projection chamber the multidimensional systematic study of pi k p and pbar production in cucu auau dau and pp collisions is used to discuss the energy system size and inferred energy density dependence of freezeout parameters and strangeness production the new data from cucu collisions bridge the gap between the smaller dau and larger auau systems allowing a detailed study of the onset of strangeness equilibration at rhic
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710.3903
Lorentzian spacetimes with constant curvature invariants in three dimensions
In this paper we study Lorentzian spacetimes for which all polynomial scalar invariants constructed from the Riemann tensor and its covariant derivatives are constant (CSI spacetimes) in three dimensions. We determine all such CSI metrics explicitly, and show that for every CSI with particular constant invariants there is a locally homogeneous spacetime with precisely the same constant invariants. We prove that a three-dimensional CSI spacetime is either (i) locally homogeneous or (ii) it is locally a Kundt spacetime. Moreover, we show that there exists a null frame in which the Riemann (Ricci) tensor and its derivatives are of boost order zero with constant boost weight zero components at each order. Lastly, these spacetimes can be explicitly constructed from locally homogeneous spacetimes and vanishing scalar invariant spacetimes.
gr-qc
in this paper we study lorentzian spacetimes for which all polynomial scalar invariants constructed from the riemann tensor and its covariant derivatives are constant csi spacetimes in three dimensions we determine all such csi metrics explicitly and show that for every csi with particular constant invariants there is a locally homogeneous spacetime with precisely the same constant invariants we prove that a threedimensional csi spacetime is either i locally homogeneous or ii it is locally a kundt spacetime moreover we show that there exists a null frame in which the riemann ricci tensor and its derivatives are of boost order zero with constant boost weight zero components at each order lastly these spacetimes can be explicitly constructed from locally homogeneous spacetimes and vanishing scalar invariant spacetimes
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710.3904
Aharanov-Bohm effect for the edge states of zigzag carbon nanotubes
Two delocalized states of metallic zigzag carbon nanotubes near the Dirac point can be localized by the Aharanov-Bohm magnetic field around 20 Tesla. The dependence of the localization on the length and diameter of the nanotubes shows that the localization-delocalization transition can be observed for 2 nm diameter tube. The mechanism of the localization is explained in terms of the deformation-induced gauge field, which shows a topological nature of the localization. The transition from the delocalized states to the localized states can be observed by scanning tunneling microscopy and spectroscopy. A similarity between the transition and the spin Hall effect is discussed.
cond-mat.mes-hall cond-mat.mtrl-sci
two delocalized states of metallic zigzag carbon nanotubes near the dirac point can be localized by the aharanovbohm magnetic field around 20 tesla the dependence of the localization on the length and diameter of the nanotubes shows that the localizationdelocalization transition can be observed for 2 nm diameter tube the mechanism of the localization is explained in terms of the deformationinduced gauge field which shows a topological nature of the localization the transition from the delocalized states to the localized states can be observed by scanning tunneling microscopy and spectroscopy a similarity between the transition and the spin hall effect is discussed
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710.3905
The (ir)Relevance of Initial Conditions in Soft Leptogenesis
We explore how the initial conditions affect the final lepton asymmetry in Soft Leptogenesis. It has been usually assumed that the initial state is a statistical mixture of sterile sneutrinos and anti-sneutrinos with equal abundances. We calculate the lepton asymmetry due to the most general initial mixture. The usually assumed equal mixture produces a small, but sufficient, lepton asymmetry which is proportional to the ratio of the supersymmetry breaking scale over the Majorana scale. A more generic mixture, still with equal contents of sneutrinos and anti sneutrinos, yields an unsuppressed lepton asymmetry. Mixtures of non equal contents of sneutrinos and anti sneutrinos result in a large lepton asymmetry too. While these results establish the robustness of Soft Leptogenesis and other mixing based mechanisms, they also expose their lack of predictive power.
hep-ph
we explore how the initial conditions affect the final lepton asymmetry in soft leptogenesis it has been usually assumed that the initial state is a statistical mixture of sterile sneutrinos and antisneutrinos with equal abundances we calculate the lepton asymmetry due to the most general initial mixture the usually assumed equal mixture produces a small but sufficient lepton asymmetry which is proportional to the ratio of the supersymmetry breaking scale over the majorana scale a more generic mixture still with equal contents of sneutrinos and anti sneutrinos yields an unsuppressed lepton asymmetry mixtures of non equal contents of sneutrinos and anti sneutrinos result in a large lepton asymmetry too while these results establish the robustness of soft leptogenesis and other mixing based mechanisms they also expose their lack of predictive power
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710.3906
A Parameter Study of the Dust and Gas Temperature in a Field of Young Stars
We model the thermal effect of young stars on their surrounding environment in order to understand clustered star formation. We take radiative heating of dust, dust-gas collisional heating, cosmic-ray heating, and molecular cooling into account. Using Dusty, a spherical continuum radiative transfer code, we model the dust temperature distribution around young stellar objects with various luminosities and surrounding gas and dust density distributions. We have created a grid of dust temperature models, based on our modeling with Dusty, which we can use to calculate the dust temperature in a field of stars with various parameters. We then determine the gas temperature assuming energy balance. Our models can be used to make large-scale simulations of clustered star formation more realistic.
astro-ph
we model the thermal effect of young stars on their surrounding environment in order to understand clustered star formation we take radiative heating of dust dustgas collisional heating cosmicray heating and molecular cooling into account using dusty a spherical continuum radiative transfer code we model the dust temperature distribution around young stellar objects with various luminosities and surrounding gas and dust density distributions we have created a grid of dust temperature models based on our modeling with dusty which we can use to calculate the dust temperature in a field of stars with various parameters we then determine the gas temperature assuming energy balance our models can be used to make largescale simulations of clustered star formation more realistic
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710.3907
Impacts of preference and geography on epidemic spreading
We investigate the standard susceptible-infected-susceptible model on a random network to study the effects of preference and geography on diseases spreading. The network grows by introducing one random node with $m$ links on a Euclidean space at unit time. The probability of a new node $i$ linking to a node $j$ with degree $k_j$ at distance $d_{ij}$ from node $i$ is proportional to $k_{j}^{A}/d_{ij}^{B}$, where $A$ and $B$ are positive constants governing preferential attachment and the cost of the node-node distance. In the case of A=0, we recover the usual epidemic behavior with a critical threshold below which diseases eventually die out. Whereas for B=0, the critical behavior is absent only in the condition A=1. While both ingredients are proposed simultaneously, the network becomes robust to infection for larger $A$ and smaller $B$.
physics.soc-ph
we investigate the standard susceptibleinfectedsusceptible model on a random network to study the effects of preference and geography on diseases spreading the network grows by introducing one random node with m links on a euclidean space at unit time the probability of a new node i linking to a node j with degree k_j at distance d_ij from node i is proportional to k_jad_ijb where a and b are positive constants governing preferential attachment and the cost of the nodenode distance in the case of a0 we recover the usual epidemic behavior with a critical threshold below which diseases eventually die out whereas for b0 the critical behavior is absent only in the condition a1 while both ingredients are proposed simultaneously the network becomes robust to infection for larger a and smaller b
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710.3908
Lie Rinehart Bialgebras for Crossed Products
In this paper, we study Lie Rinehart bialgebras, the algebraic generalization of Lie bialgebroids. More precisely, we analyze the structure of Lie Rinehart bialgebras for crossed products induced by actions of Lie algebras on K[t].
math.AC math.RA
in this paper we study lie rinehart bialgebras the algebraic generalization of lie bialgebroids more precisely we analyze the structure of lie rinehart bialgebras for crossed products induced by actions of lie algebras on kt
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710.3909
On the Existence of Global Bisections of Lie Groupoids
We show that every source connected Lie groupoid always has global bisections through any given point. This bisection can be chosen to be the multiplication of some exponentials as close as possible to a prescribed curve. The existence of bisections through more than one prescribed points is also discussed. We give some interesting applications of these results.
math.DG
we show that every source connected lie groupoid always has global bisections through any given point this bisection can be chosen to be the multiplication of some exponentials as close as possible to a prescribed curve the existence of bisections through more than one prescribed points is also discussed we give some interesting applications of these results
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710.391
On the photoionization of the outer electrons in noble gas endohedral atoms
We demonstrate the prominent modification of the outer shell photoionization cross-section in noble gas (NG) endohedral atoms NG@F under the action of the fullerene F electron shell. This shell leads to two important effects, namely to strong enhancement of the cross-section due to fullerenes shell polarization under the action of the incoming electromagnetic wave and to prominent oscillation of this cross-section due to the reflection of the photoelectron from NG by the F shell. All but He noble gas atoms are considered. The polarization of the fullerene shell is expressed via the total photoabsorption cross-section of F. The reflection of the photoelectron is taken into account in the frame of the so-called bubble potential that is a spherical zero --thickness potential. It is assumed in the derivations that NG is centrally located in the fullerene. It is assumed also, in accord with the existing experimental data, that the fullerenes radius R is much bigger than the atomic radius and the thickness of the fullerenes shell . These assumptions permit, as it was demonstrated recently, to present the NG@F photoionization cross-section as a product of the NG cross-section and two well defined calculated factors.
physics.atm-clus physics.atom-ph
we demonstrate the prominent modification of the outer shell photoionization crosssection in noble gas ng endohedral atoms ngf under the action of the fullerene f electron shell this shell leads to two important effects namely to strong enhancement of the crosssection due to fullerenes shell polarization under the action of the incoming electromagnetic wave and to prominent oscillation of this crosssection due to the reflection of the photoelectron from ng by the f shell all but he noble gas atoms are considered the polarization of the fullerene shell is expressed via the total photoabsorption crosssection of f the reflection of the photoelectron is taken into account in the frame of the socalled bubble potential that is a spherical zero thickness potential it is assumed in the derivations that ng is centrally located in the fullerene it is assumed also in accord with the existing experimental data that the fullerenes radius r is much bigger than the atomic radius and the thickness of the fullerenes shell these assumptions permit as it was demonstrated recently to present the ngf photoionization crosssection as a product of the ng crosssection and two well defined calculated factors
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710.3911
Helium stars as supernova progenitors
We follow the evolution of helium stars of initial mass $(2.2 - 2.5) M_\odot$, and show that they undergo off-center carbon burning, which leaves behind ${\mathbf \sim 0.01 M_\odot}$ of unburnt carbon in the inner part of the core. When the carbon-oxygen core grows to Chandrasekhar mass, the amount of left-over carbon is sufficient to ignite thermonuclear runaway. At the moment of explosion, the star will possess an envelope of several $0.1 M_{\odot}$, consisting of He, C, and possibly some H, perhaps producing a kind of peculiar SN. Based on the results of Waldman and Barkat (2007) for accreting white dwarfs, we expect to get thermonuclear runaway at a broad range of $\rho_c \approx (1 - 6) \times 10^9 \mathrm{g cm^{-3}}$, depending on the amount of residual carbon. We verified the feasibility of this scenario by showing that in a close binary system with initial masses $(8.5 + 7.7) M_{\odot}$ and initial period of 150 day the primary produces a helium remnant of $2.3 M_{\odot}$ that evolves further like the model we considered.
astro-ph
we follow the evolution of helium stars of initial mass 22 25 m_odot and show that they undergo offcenter carbon burning which leaves behind mathbf sim 001 m_odot of unburnt carbon in the inner part of the core when the carbonoxygen core grows to chandrasekhar mass the amount of leftover carbon is sufficient to ignite thermonuclear runaway at the moment of explosion the star will possess an envelope of several 01 m_odot consisting of he c and possibly some h perhaps producing a kind of peculiar sn based on the results of waldman and barkat 2007 for accreting white dwarfs we expect to get thermonuclear runaway at a broad range of rho_c approx 1 6 times 109 mathrmg cm3 depending on the amount of residual carbon we verified the feasibility of this scenario by showing that in a close binary system with initial masses 85 77 m_odot and initial period of 150 day the primary produces a helium remnant of 23 m_odot that evolves further like the model we considered
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710.3912
The sectional curvature remains positive when taking quotients by certain nonfree actions
We study some cases when the sectional curvature remains positive under the taking of quotients by certain nonfree isometric actions of Lie groups. We consider the actions of the groups $S^1$ and $S^3$ such that the quotient space can be endowed with a smooth structure using the fibrations $S^3/S^1{\simeq}S^2$ and $S^7/S^3\simeq S^4$. We prove that the quotient space carries a metric of positive sectional curvature, provided that the original metric has positive sectional curvature on all 2-planes orthogonal to the orbits of the action.
math.DG
we study some cases when the sectional curvature remains positive under the taking of quotients by certain nonfree isometric actions of lie groups we consider the actions of the groups s1 and s3 such that the quotient space can be endowed with a smooth structure using the fibrations s3s1simeqs2 and s7s3simeq s4 we prove that the quotient space carries a metric of positive sectional curvature provided that the original metric has positive sectional curvature on all 2planes orthogonal to the orbits of the action
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710.3913
Charged fundamental particles in Wesson's IMT
In the framework of the Weyl-Dirac version of Wesson's Induced Matter Theory, spherically symmetric entities filled with an electrically charged substance are obtained in the empty 4D space-time, the brane. The substance, characterized by mass and charge density as well by pressure, is induced by the 5D bulk. The entity is separated from the surrounding vacuum by a boundary surface, where the metric satisfy the Schwarzschild conditions. Outside one has the Reissner-Nordstroem metric with M=Q. These entities may be regarded as classical (non-quantum) fundamental particles serving as constituents of quarks and leptons.
gr-qc
in the framework of the weyldirac version of wessons induced matter theory spherically symmetric entities filled with an electrically charged substance are obtained in the empty 4d spacetime the brane the substance characterized by mass and charge density as well by pressure is induced by the 5d bulk the entity is separated from the surrounding vacuum by a boundary surface where the metric satisfy the schwarzschild conditions outside one has the reissnernordstroem metric with mq these entities may be regarded as classical nonquantum fundamental particles serving as constituents of quarks and leptons
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710.3914
Protecting entanglement via the quantum Zeno effect
We study the exact entanglement dynamics of two atoms in a lossy resonator. Besides discussing the steady-state entanglement, we show that in the strong coupling regime the system-reservoir correlations induce entanglement revivals and oscillations and propose a strategy to fight against the deterioration of the entanglement using the quantum Zeno effect.
quant-ph
we study the exact entanglement dynamics of two atoms in a lossy resonator besides discussing the steadystate entanglement we show that in the strong coupling regime the systemreservoir correlations induce entanglement revivals and oscillations and propose a strategy to fight against the deterioration of the entanglement using the quantum zeno effect
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710.3915
Inverse spectral results for Schr\"odinger operators on the unit interval with potentials in L^P spaces
We consider the Schr\"odinger operator on $[0,1]$ with potential in $L^1$. We prove that two potentials already known on $[a,1]$ ($a\in(0,{1/2}]$) and having their difference in $L^p$ are equal if the number of their common eigenvalues is sufficiently large. The result here is to write down explicitly this number in terms of $p$ (and $a$) showing the role of $p$.
math.SP
we consider the schrodinger operator on 01 with potential in l1 we prove that two potentials already known on a1 ain012 and having their difference in lp are equal if the number of their common eigenvalues is sufficiently large the result here is to write down explicitly this number in terms of p and a showing the role of p
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710.3916
Optimized Design of Survivable MPLS over Optical Transport Networks. Optical Switching and Networking
In this paper we study different options for the survivability implementation in MPLS over Optical Transport Networks in terms of network resource usage and configuration cost. We investigate two approaches to the survivability deployment: single layer and multilayer survivability and present various methods for spare capacity allocation (SCA) to reroute disrupted traffic. The comparative analysis shows the influence of the traffic granularity on the survivability cost: for high bandwidth LSPs, close to the optical channel capacity, the multilayer survivability outperforms the single layer one, whereas for low bandwidth LSPs the single layer survivability is more cost-efficient. For the multilayer survivability we demonstrate that by mapping efficiently the spare capacity of the MPLS layer onto the resources of the optical layer one can achieve up to 22% savings in the total configuration cost and up to 37% in the optical layer cost. Further savings (up to 9 %) in the wavelength use can be obtained with the integrated approach to network configuration over the sequential one, however, at the increase in the optimization problem complexity. These results are based on a cost model with actual technology pricing and were obtained for networks targeted to a nationwide coverage.
cs.NI cs.PF
in this paper we study different options for the survivability implementation in mpls over optical transport networks in terms of network resource usage and configuration cost we investigate two approaches to the survivability deployment single layer and multilayer survivability and present various methods for spare capacity allocation sca to reroute disrupted traffic the comparative analysis shows the influence of the traffic granularity on the survivability cost for high bandwidth lsps close to the optical channel capacity the multilayer survivability outperforms the single layer one whereas for low bandwidth lsps the single layer survivability is more costefficient for the multilayer survivability we demonstrate that by mapping efficiently the spare capacity of the mpls layer onto the resources of the optical layer one can achieve up to 22 savings in the total configuration cost and up to 37 in the optical layer cost further savings up to 9 in the wavelength use can be obtained with the integrated approach to network configuration over the sequential one however at the increase in the optimization problem complexity these results are based on a cost model with actual technology pricing and were obtained for networks targeted to a nationwide coverage
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710.3917
Heuristic Solution to Protect Communications in WDM Networks using P-cycles
Optical WDM mesh networks are able to transport huge amount of information. The use of such technology however poses the problem of protection against failures such as fibre cuts. One of the principal methods for link protection used in optical WDM networks is pre-configured protection cycle (p-cycle). The major problem of this method of protection resides in finding the optimal set of p-cycles which protect the network for a given distribution of working capacity. Existing heuristics generate a large set of p-cycle candidates which are entirely independent of the network state, and from then the good sub-set of p-cycles which will protect the network is selected. In this paper, we propose a new algorithm of generation of p-cycles based on the incremental aggregation of the shortest cycles. Our generation of p-cycles depends on the state of the network. This enables us to choose an efficient set of p-cycles which will protect the network. The set of p-cycles that we generate is the final set which will protect the network, in other words our heuristic does not go through the additional step of p-cycle selection
cs.NI
optical wdm mesh networks are able to transport huge amount of information the use of such technology however poses the problem of protection against failures such as fibre cuts one of the principal methods for link protection used in optical wdm networks is preconfigured protection cycle pcycle the major problem of this method of protection resides in finding the optimal set of pcycles which protect the network for a given distribution of working capacity existing heuristics generate a large set of pcycle candidates which are entirely independent of the network state and from then the good subset of pcycles which will protect the network is selected in this paper we propose a new algorithm of generation of pcycles based on the incremental aggregation of the shortest cycles our generation of pcycles depends on the state of the network this enables us to choose an efficient set of pcycles which will protect the network the set of pcycles that we generate is the final set which will protect the network in other words our heuristic does not go through the additional step of pcycle selection
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710.3918
Dependable k-coverage algorithms for sensor networks
Redundant sensing capabilities are often required in sensor network applications due to various reasons, e.g. robustness, fault tolerance, or increased accuracy. At the same time high sensor redundancy offers the possibility of increasing network lifetime by scheduling sleep intervals for some sensors and still providing continuous service with help of the remaining active sensors. In this paper centralized and distributed algorithms are proposed to solve the k-coverage sensing problem and maximize network lifetime. When physically possible, the proposed robust Controlled Greedy Sleep Algorithm provides guaranteed service independently of node and communication errors in the network. The performance of the algorithm is illustrated and compared to results of a random solution by simulation examples.
cs.NI
redundant sensing capabilities are often required in sensor network applications due to various reasons eg robustness fault tolerance or increased accuracy at the same time high sensor redundancy offers the possibility of increasing network lifetime by scheduling sleep intervals for some sensors and still providing continuous service with help of the remaining active sensors in this paper centralized and distributed algorithms are proposed to solve the kcoverage sensing problem and maximize network lifetime when physically possible the proposed robust controlled greedy sleep algorithm provides guaranteed service independently of node and communication errors in the network the performance of the algorithm is illustrated and compared to results of a random solution by simulation examples
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710.3919
Bounding sectional curvature along a K\"ahler-Ricci flow
If a normalized K\"{a}hler-Ricci flow $g(t),t\in[0,\infty),$ on a compact K\"{a}hler $n$-manifold, $n\geq 3$, of positive first Chern class satisfies $g(t)\in 2\pi c_{1}(M)$ and has $L^{n}$ curvature operator uniformly bounded, then the curvature operator will also uniformly bounded along the flow. Consequently the flow will converge along a subsequence to a K\"{a}hler-Ricci soliton.
math.DG
if a normalized kahlerricci flow gttin0infty on a compact kahler nmanifold ngeq 3 of positive first chern class satisfies gtin 2pi c_1m and has ln curvature operator uniformly bounded then the curvature operator will also uniformly bounded along the flow consequently the flow will converge along a subsequence to a kahlerricci soliton
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710.392
An Introduction to Potential Theory in Calibrated Geometry
We introduce and study the notion of plurisubharmonic functions in calibrated geometry. These functions generalize the classical plurisubharmonic functions from complex geometry and enjoy their important properties. Moreover, they exist in abundance whereas the corresponding pluriharmonics are generally quite scarce. A number of the results established in complex analysis via plurisubharmonic functions are extended to calibrated manifolds. In particular, the notion of pseudo-convexity for a calibrated manifold (X,\phi) is introduced and studied. Analogues of totally real submanifolds are also introduced and used to construct enormous families of strictly \phi-convex spaces with every topological type allowed by Morse Theory. Specific calibrations are used as examples throughout.
math.DG math.CV
we introduce and study the notion of plurisubharmonic functions in calibrated geometry these functions generalize the classical plurisubharmonic functions from complex geometry and enjoy their important properties moreover they exist in abundance whereas the corresponding pluriharmonics are generally quite scarce a number of the results established in complex analysis via plurisubharmonic functions are extended to calibrated manifolds in particular the notion of pseudoconvexity for a calibrated manifold xphi is introduced and studied analogues of totally real submanifolds are also introduced and used to construct enormous families of strictly phiconvex spaces with every topological type allowed by morse theory specific calibrations are used as examples throughout
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710.3921
Duality of Positive Currents and Plurisubharmonic Functions in Calibrated Geometry
Recently the authors showed that there is a robust potential theory attached to any calibrated manifold (X,\phi). In particular, on X there exist \phi-plurisubharmonic functions, \phi-convex domains, \phi-convex boundaries, etc., all inter-related and having a number of good properties. In this paper we show that, in a strong sense, the plurisubharmonic functions are the polar duals of the \phi-submanifolds, or more generally, the \phi-currents studied in the original paper on calibrations. In particular, we establish an analogue of Duval-Sibony Duality which characterizes points in the \phi-convex hull of a compact set K in X in terms of \phi-positive Green's currents on X and Jensen measures on K. We also characterize boundaries of \phi-currents entirely in terms of \phi-plurisubharmonic functions. Specific calibrations are used as examples throughout. Analogues of the Hodge Conjecture in calibrated geometry are considered.
math.DG math.CV
recently the authors showed that there is a robust potential theory attached to any calibrated manifold xphi in particular on x there exist phiplurisubharmonic functions phiconvex domains phiconvex boundaries etc all interrelated and having a number of good properties in this paper we show that in a strong sense the plurisubharmonic functions are the polar duals of the phisubmanifolds or more generally the phicurrents studied in the original paper on calibrations in particular we establish an analogue of duvalsibony duality which characterizes points in the phiconvex hull of a compact set k in x in terms of phipositive greens currents on x and jensen measures on k we also characterize boundaries of phicurrents entirely in terms of phiplurisubharmonic functions specific calibrations are used as examples throughout analogues of the hodge conjecture in calibrated geometry are considered
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710.3922
Hysteresis Models of Dynamic Mode Atomic Force Microscopes: Analysis and Identification
A new class of models based on hysteresis functions is developed to describe atomic force microscopes operating in dynamic mode. Such models are able to account for dissipative phenomena in the tip-sample interaction which are peculiar of this operation mode. The model analysis, which can be pursued using frequency domain techniques, provides a clear insight of specific nonlinear behaviours. Experiments show good agreement with the identified models.
nlin.CD
a new class of models based on hysteresis functions is developed to describe atomic force microscopes operating in dynamic mode such models are able to account for dissipative phenomena in the tipsample interaction which are peculiar of this operation mode the model analysis which can be pursued using frequency domain techniques provides a clear insight of specific nonlinear behaviours experiments show good agreement with the identified models
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710.3923
Creation of fundamental particles in Wesson's IMT
Fundamental particles, regarded as the constituents of quarks and leptons, are described classicaly in the framework of the Weyl-Dirac version of Wesson's Induced Matter Theory. There are neutral particles and particles having charge Q=+/-(1/3e). The particles appear on the 4D brane, our universe, and are filled with a substance induced by the 5D bulk. This substace is taken to have mass density, charge density, pressure and is characterized by the prematter eq. of state P+\rho=0. The interior is separated from the surrounding vacuum by a boundary surface where the 4D metric tensor satisfies an a'la Schwarzschild condition. Outside of the boundary holds the Schwarzschild, or the Reissner-Nordstroem Metric, while the particles are characterized by mass, radius, charge.
gr-qc
fundamental particles regarded as the constituents of quarks and leptons are described classicaly in the framework of the weyldirac version of wessons induced matter theory there are neutral particles and particles having charge q13e the particles appear on the 4d brane our universe and are filled with a substance induced by the 5d bulk this substace is taken to have mass density charge density pressure and is characterized by the prematter eq of state prho0 the interior is separated from the surrounding vacuum by a boundary surface where the 4d metric tensor satisfies an ala schwarzschild condition outside of the boundary holds the schwarzschild or the reissnernordstroem metric while the particles are characterized by mass radius charge
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710.3924
Convexity properties for generalized moment maps I
We study generalized moment maps for a Hamiltonian action on a connected compact $H$-twisted generalized complex manifold introduced by Lin and Tolman and prove the convexity and connectedness properties of the generalized moment maps for a Hamiltonian torus action.
math.DG math.SG
we study generalized moment maps for a hamiltonian action on a connected compact htwisted generalized complex manifold introduced by lin and tolman and prove the convexity and connectedness properties of the generalized moment maps for a hamiltonian torus action
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710.3925
Regge behaviour of structure functions and solution of Dokshitzer-Gribov-Lipatov-Altarelli-Parisi Evolution equations in next-to-leading order at low-x
Deuteron and proton structure functions are derived from Dokshitzer-Gribov-Lipatov-Altarelli-Parisi (DGLAP) evolution equations of singlet and non-singlet structure functions in next-to-leading order (NLO) at low-x assuming the Regge behaviour of singlet and non-singlet structure functions at this limit and results are compared with New Muon Collaboration (NMC) and E665 collaboration data sets.
hep-ph
deuteron and proton structure functions are derived from dokshitzergribovlipatovaltarelliparisi dglap evolution equations of singlet and nonsinglet structure functions in nexttoleading order nlo at lowx assuming the regge behaviour of singlet and nonsinglet structure functions at this limit and results are compared with new muon collaboration nmc and e665 collaboration data sets
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710.3926
From an Antiferromagnet to a Valence Bond Solid: Evidence for a First Order Phase Transition
Using a loop-cluster algorithm we investigate the spin 1/2 Heisenberg antiferromagnet on a square lattice with exchange coupling $J$ and an additional four-spin interaction of strength $Q$. We confirm the existence of a phase transition separating antiferromagnetism at $J/Q > J_c/Q$ from a valence bond solid (VBS) state at $J/Q < J_c/Q$. Although our Monte Carlo data are consistent with those of previous studies, we do not confirm the existence of a deconfined quantum critical point. Instead, using a flowgram method on lattices as large as $80^2$, we find evidence for a weak first order phase transition. We also present a detailed study of the antiferromagnetic phase. For $J/Q > J_c/Q$ the staggered magnetization, the spin stiffness, and the spinwave velocity of the antiferromagnet are determined by fitting Monte Carlo data to analytic results from the systematic low-energy effective field theory for magnons. Finally, we also investigate the physics of the VBS state at $J/Q < J_c/Q$, and we show that long but finite antiferromagnetic correlations are still present.
cond-mat.str-el
using a loopcluster algorithm we investigate the spin 12 heisenberg antiferromagnet on a square lattice with exchange coupling j and an additional fourspin interaction of strength q we confirm the existence of a phase transition separating antiferromagnetism at jq j_cq from a valence bond solid vbs state at jq j_cq although our monte carlo data are consistent with those of previous studies we do not confirm the existence of a deconfined quantum critical point instead using a flowgram method on lattices as large as 802 we find evidence for a weak first order phase transition we also present a detailed study of the antiferromagnetic phase for jq j_cq the staggered magnetization the spin stiffness and the spinwave velocity of the antiferromagnet are determined by fitting monte carlo data to analytic results from the systematic lowenergy effective field theory for magnons finally we also investigate the physics of the vbs state at jq j_cq and we show that long but finite antiferromagnetic correlations are still present
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710.3927
On repulsive gravitational actions
In particular instances and in particular regions the Einsteinian gravity exerts a repulsive action -- and without any cosmological term. This fact could have an interest for the explanation of the dark energy, and for the gravitational collapses.
physics.gen-ph
in particular instances and in particular regions the einsteinian gravity exerts a repulsive action and without any cosmological term this fact could have an interest for the explanation of the dark energy and for the gravitational collapses
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710.3928
Message passing for the coloring problem: Gallager meets Alon and Kahale
Message passing algorithms are popular in many combinatorial optimization problems. For example, experimental results show that {\em survey propagation} (a certain message passing algorithm) is effective in finding proper $k$-colorings of random graphs in the near-threshold regime. In 1962 Gallager introduced the concept of Low Density Parity Check (LDPC) codes, and suggested a simple decoding algorithm based on message passing. In 1994 Alon and Kahale exhibited a coloring algorithm and proved its usefulness for finding a $k$-coloring of graphs drawn from a certain planted-solution distribution over $k$-colorable graphs. In this work we show an interpretation of Alon and Kahale's coloring algorithm in light of Gallager's decoding algorithm, thus showing a connection between the two problems - coloring and decoding. This also provides a rigorous evidence for the usefulness of the message passing paradigm for the graph coloring problem. Our techniques can be applied to several other combinatorial optimization problems and networking-related issues.
math.CO cs.DM math.PR
message passing algorithms are popular in many combinatorial optimization problems for example experimental results show that em survey propagation a certain message passing algorithm is effective in finding proper kcolorings of random graphs in the nearthreshold regime in 1962 gallager introduced the concept of low density parity check ldpc codes and suggested a simple decoding algorithm based on message passing in 1994 alon and kahale exhibited a coloring algorithm and proved its usefulness for finding a kcoloring of graphs drawn from a certain plantedsolution distribution over kcolorable graphs in this work we show an interpretation of alon and kahales coloring algorithm in light of gallagers decoding algorithm thus showing a connection between the two problems coloring and decoding this also provides a rigorous evidence for the usefulness of the message passing paradigm for the graph coloring problem our techniques can be applied to several other combinatorial optimization problems and networkingrelated issues
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710.3929
Supersymmetry, quark confinement and the harmonic oscillator
We study some quantum systems described by noncanonical commutation relations formally expressed as [q,p]=ihbar(I + chi H), where H is the associated (harmonic oscillator-like) Hamiltonian of the system, and chi is a Hermitian (constant) operator, i.e. [H,chi]=0 . In passing, we also consider a simple (chi=0 canonical) model, in the framework of a relativistic Klein-Gordon-like wave equation.
quant-ph
we study some quantum systems described by noncanonical commutation relations formally expressed as qpihbari chi h where h is the associated harmonic oscillatorlike hamiltonian of the system and chi is a hermitian constant operator ie hchi0 in passing we also consider a simple chi0 canonical model in the framework of a relativistic kleingordonlike wave equation
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710.393
Interactions of Heavy Hadrons using Regge Phenomenology and the Quark Gluon String Model
The search for stable heavy exotic hadrons is a promising way to observe new physics processes at collider experiments. The discovery potential for such particles can be enhanced or suppressed by their interactions with detector material. This paper describes a model for the interactions in matter of stable hadrons containing an exotic quark of charges $\pm {1/3}e$ or $\pm {2/3}e$ using Regge phenomenology and the Quark Gluon String Model. The influence of such interactions on searches at the LHC is also discussed.
hep-ph
the search for stable heavy exotic hadrons is a promising way to observe new physics processes at collider experiments the discovery potential for such particles can be enhanced or suppressed by their interactions with detector material this paper describes a model for the interactions in matter of stable hadrons containing an exotic quark of charges pm 13e or pm 23e using regge phenomenology and the quark gluon string model the influence of such interactions on searches at the lhc is also discussed
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710.3931
Geometric phases in semiconductor spin qubits: Manipulations and decoherence
We describe the effect of geometric phases induced by either classical or quantum electric fields acting on single electron spins in quantum dots in the presence of spin-orbit coupling. On one hand, applied electric fields can be used to control the geometric phases, which allows performing quantum coherent spin manipulations without using high-frequency magnetic fields. On the other hand, fluctuating fields induce random geometric phases that lead to spin relaxation and dephasing, thus limiting the use of such spins as qubits. We estimate the decay rates due to piezoelectric phonons and conduction electrons in the circuit, both representing dominant electric noise sources with characteristically differing power spectra.
cond-mat.mes-hall
we describe the effect of geometric phases induced by either classical or quantum electric fields acting on single electron spins in quantum dots in the presence of spinorbit coupling on one hand applied electric fields can be used to control the geometric phases which allows performing quantum coherent spin manipulations without using highfrequency magnetic fields on the other hand fluctuating fields induce random geometric phases that lead to spin relaxation and dephasing thus limiting the use of such spins as qubits we estimate the decay rates due to piezoelectric phonons and conduction electrons in the circuit both representing dominant electric noise sources with characteristically differing power spectra
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710.3932
Complementarity of perturbations driving insulator-to-metal transition in a charge ordered manganite
Modulation of charge carrier dynamics and hence electrical conductivity of solids by photoexcitation has been a rich field of research with numerous applications. Similarly, electric and magnetic field assisted enhancement of conductivity are of fundamental importance and technological use. Hole doped manganites of the type (A$_{1-x}$B$_{x})$MnO$_{3}$, where A and B are rare and alkaline earth metals respectively have the distinction of showing all three effects. Here we establish the complementarity of the electric, magnetic and photon fields in driving an insulator-metal transition in epitaxial thin films of La$_{0.175}$Pr$_{0.45}$Ca$_{0.375}$MnO$_{3}$ whose electrical ground state is insulating. Both pulsed and CW lasers cause a giant photon flux dependent enhancement of conductivity. It is further observed that electric and magnetic fields trigger the persistent enhancement of conductivity whose magnitude can be accentuated by application of these fields in parallel.
cond-mat.str-el cond-mat.mtrl-sci
modulation of charge carrier dynamics and hence electrical conductivity of solids by photoexcitation has been a rich field of research with numerous applications similarly electric and magnetic field assisted enhancement of conductivity are of fundamental importance and technological use hole doped manganites of the type a_1xb_xmno_3 where a and b are rare and alkaline earth metals respectively have the distinction of showing all three effects here we establish the complementarity of the electric magnetic and photon fields in driving an insulatormetal transition in epitaxial thin films of la_0175pr_045ca_0375mno_3 whose electrical ground state is insulating both pulsed and cw lasers cause a giant photon flux dependent enhancement of conductivity it is further observed that electric and magnetic fields trigger the persistent enhancement of conductivity whose magnitude can be accentuated by application of these fields in parallel
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710.3933
Energy-momentum tensor in thermal strong-field QED with unstable vacuum
The mean value of the one-loop energy-momentum tensor in thermal QED with electric-like background that creates particles from vacuum is calculated. The problem differes essentially from calculations of effective actions (similar to that of Heisenberg--Euler) in backgrounds that do not violate the stability of vacuum. The role of a constant electric background in the violation of both the stability of vacuum and the thermal character of particle distribution is investigated. Restrictions on the electric field and its duration under which one can neglect the back-reaction of created particles are established.
hep-th
the mean value of the oneloop energymomentum tensor in thermal qed with electriclike background that creates particles from vacuum is calculated the problem differes essentially from calculations of effective actions similar to that of heisenbergeuler in backgrounds that do not violate the stability of vacuum the role of a constant electric background in the violation of both the stability of vacuum and the thermal character of particle distribution is investigated restrictions on the electric field and its duration under which one can neglect the backreaction of created particles are established
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710.3934
New mechanism of generation of large-scale magnetic field in a sheared turbulent plasma
A review of recent studies on a new mechanism of generation of large-scale magnetic field in a sheared turbulent plasma is presented. This mechanism is associated with the shear-current effect which is related to the W x J-term in the mean electromotive force. This effect causes the generation of the large-scale magnetic field even in a nonrotating and nonhelical homogeneous sheared turbulent convection whereby the alpha effect vanishes. It is found that turbulent convection promotes the shear-current dynamo instability, i.e., the heat flux causes positive contribution to the shear-current effect. However, there is no dynamo action due to the shear-current effect for small hydrodynamic and magnetic Reynolds numbers even in a turbulent convection, if the spatial scaling for the turbulent correlation time is k^{-2}, where k is the small-scale wave number. We discuss here also the nonlinear mean-field dynamo due to the shear-current effect and take into account the transport of magnetic helicity as a dynamical nonlinearity. The magnetic helicity flux strongly affects the magnetic field dynamics in the nonlinear stage of the dynamo action. When the magnetic helicity flux is not small, the saturated level of the mean magnetic field is of the order of the equipartition field determined by the turbulent kinetic energy. The obtained results are important for elucidation of origin of the large-scale magnetic fields in astrophysical and cosmic sheared turbulent plasma.
astro-ph
a review of recent studies on a new mechanism of generation of largescale magnetic field in a sheared turbulent plasma is presented this mechanism is associated with the shearcurrent effect which is related to the w x jterm in the mean electromotive force this effect causes the generation of the largescale magnetic field even in a nonrotating and nonhelical homogeneous sheared turbulent convection whereby the alpha effect vanishes it is found that turbulent convection promotes the shearcurrent dynamo instability ie the heat flux causes positive contribution to the shearcurrent effect however there is no dynamo action due to the shearcurrent effect for small hydrodynamic and magnetic reynolds numbers even in a turbulent convection if the spatial scaling for the turbulent correlation time is k2 where k is the smallscale wave number we discuss here also the nonlinear meanfield dynamo due to the shearcurrent effect and take into account the transport of magnetic helicity as a dynamical nonlinearity the magnetic helicity flux strongly affects the magnetic field dynamics in the nonlinear stage of the dynamo action when the magnetic helicity flux is not small the saturated level of the mean magnetic field is of the order of the equipartition field determined by the turbulent kinetic energy the obtained results are important for elucidation of origin of the largescale magnetic fields in astrophysical and cosmic sheared turbulent plasma
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710.3935
Magnetic Reversal Time in Open Long Range Systems
Topological phase space disconnection has been recently found to be a general phenomenon in isolated anisotropic spin systems. It sets a general framework to understand the emergence of ferromagnetism in finite magnetic systems starting from microscopic models without phenomenological on-site barriers. Here we study its relevance for finite systems with long range interacting potential in contact with a thermal bath. We show that, even in this case, the induced magnetic reversal time is exponentially large in the number of spins, thus determining {\it stable} (to any experimental observation time) ferromagnetic behavior. Moreover, the explicit temperature dependence of the magnetic reversal time obtained from the microcanonical results, is found to be in good agreement with numerical simulations. Also, a simple and suggestive expression, indicating the Topological Energy Threshold at which the disconnection occurs, as a real energy barrier for many body systems, is obtained analytically for low temperature.
cond-mat.stat-mech cond-mat.mes-hall
topological phase space disconnection has been recently found to be a general phenomenon in isolated anisotropic spin systems it sets a general framework to understand the emergence of ferromagnetism in finite magnetic systems starting from microscopic models without phenomenological onsite barriers here we study its relevance for finite systems with long range interacting potential in contact with a thermal bath we show that even in this case the induced magnetic reversal time is exponentially large in the number of spins thus determining it stable to any experimental observation time ferromagnetic behavior moreover the explicit temperature dependence of the magnetic reversal time obtained from the microcanonical results is found to be in good agreement with numerical simulations also a simple and suggestive expression indicating the topological energy threshold at which the disconnection occurs as a real energy barrier for many body systems is obtained analytically for low temperature
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710.3936
Improved Hardy-Sobolev inequalities
The main result includes features of a Hardy-type inequality and an inequality of either Sobolev or Gagliardo-Nirenberg type. It is inspired by the method of proof of a recent improved Sobolev inequality derived by M. Ledoux which brings out the connection between Sobolev embeddings and heat kernel bounds. Here Ledoux's technique is applied to the operator $L:= {\bf{x}} \cdot \nabla$ and the analysis requires the determination of the operator semigroup $\{e^{-tL^{*}L}\}_{t>0}$ and its properties.
math.SP math-ph math.MP
the main result includes features of a hardytype inequality and an inequality of either sobolev or gagliardonirenberg type it is inspired by the method of proof of a recent improved sobolev inequality derived by m ledoux which brings out the connection between sobolev embeddings and heat kernel bounds here ledouxs technique is applied to the operator l bfx cdot nabla and the analysis requires the determination of the operator semigroup etll_t0 and its properties
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710.3937
An Analytic Proof of the Matrix Spectral Factorization Theorem
An analytic proof is proposed of Wiener's theorem on factorization of positive definite matrix-functions.
math.CV
an analytic proof is proposed of wieners theorem on factorization of positive definite matrixfunctions
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710.3938
Multiplicity Fluctuations in Limited Segments of Momentum Space in Statistical Models
Multiplicity fluctuations in limited segments of momentum space are calculated for a classical pion gas within the statistical model. Results for the grand canonical, canonical, and micro-canonical ensemble are obtained, compared and discussed. We demonstrate that even in the large volume limit correlations between macroscopic subsystems due to energy and momentum conservation persist. Based on the micro-canonical formulation we make qualitative predictions for the rapidity and transverse momentum dependence of multiplicity fluctuations. The resulting effects are of similar magnitude as the predicted enhancement due to a phase transition from a quark-gluon plasma to a hadron gas phase, or due to the critical point of strongly interacting matter, and qualitatively agree with recently published preliminary multiplicity fluctuation data of the NA49 SPS experiment.
nucl-th
multiplicity fluctuations in limited segments of momentum space are calculated for a classical pion gas within the statistical model results for the grand canonical canonical and microcanonical ensemble are obtained compared and discussed we demonstrate that even in the large volume limit correlations between macroscopic subsystems due to energy and momentum conservation persist based on the microcanonical formulation we make qualitative predictions for the rapidity and transverse momentum dependence of multiplicity fluctuations the resulting effects are of similar magnitude as the predicted enhancement due to a phase transition from a quarkgluon plasma to a hadron gas phase or due to the critical point of strongly interacting matter and qualitatively agree with recently published preliminary multiplicity fluctuation data of the na49 sps experiment
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710.3939
Rotational symmetry breaking in baby Skyrme models
We consider multisolitons with charges 1 =< B =< 5 in the baby Skyrme model for the one-parametric family of potentials U=\mu^2 (1-\phi_3)^s with 0<s =< 4. This class of potentials is a generalization of the `old' (s=1) and `holomorphic' (s=4) baby Skyrme models. We find that for charge one, stable solutions exist for every value of s and they are rotationally-symmetric. For higher charges, stable solutions exist only below s \approx 2. In the charge-two sector the stable solutions are always rotationally-symmetric and ring-like. For charge three and above, rotational symmetry is exhibited only in the small s region; above a certain critical value of s, this symmetry is broken and a strong repulsion between the constituent one-Skyrmions becomes apparent. We also compute the spatial energy distributions of these solutions.
hep-th
we consider multisolitons with charges 1 b 5 in the baby skyrme model for the oneparametric family of potentials umu2 1phi_3s with 0s 4 this class of potentials is a generalization of the old s1 and holomorphic s4 baby skyrme models we find that for charge one stable solutions exist for every value of s and they are rotationallysymmetric for higher charges stable solutions exist only below s approx 2 in the chargetwo sector the stable solutions are always rotationallysymmetric and ringlike for charge three and above rotational symmetry is exhibited only in the small s region above a certain critical value of s this symmetry is broken and a strong repulsion between the constituent oneskyrmions becomes apparent we also compute the spatial energy distributions of these solutions
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710.394
A classical picture of the role of vacancies and interstitials in Helium-4
Motivated by experimental hints for supersolidity in Helium-4, we perform Monte Carlo simulations of vacancies and interstitials in a classical two-and three-dimensional Lennard-Jones solid. We confirm a strong binding energy of vacancies which is of the order of Lennard-Jones attraction. This is reminiscent of what has been found for vacancies in Quantum Monte Carlo simulations. In addition, we find a strong attraction and large binding energy of interstitials in two-dimensional simulations. This is mainly due to the formation of a pair of dislocations by clustering interstitials, in which minimizes the elastic deformation energy. We interpret the results in light of the properties of Helium-4.
cond-mat.other
motivated by experimental hints for supersolidity in helium4 we perform monte carlo simulations of vacancies and interstitials in a classical twoand threedimensional lennardjones solid we confirm a strong binding energy of vacancies which is of the order of lennardjones attraction this is reminiscent of what has been found for vacancies in quantum monte carlo simulations in addition we find a strong attraction and large binding energy of interstitials in twodimensional simulations this is mainly due to the formation of a pair of dislocations by clustering interstitials in which minimizes the elastic deformation energy we interpret the results in light of the properties of helium4
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710.3941
Solutions of Nuclear Pairing
We give the exact solution of orbit dependent nuclear pairing problem between two non-degenerate energy levels using the Bethe ansatz technique. Our solution reduces to previously solved cases in the appropriate limits including Richardson's treatment of reduced pairing in terms of rational Gaudin algebra operators.
nucl-th
we give the exact solution of orbit dependent nuclear pairing problem between two nondegenerate energy levels using the bethe ansatz technique our solution reduces to previously solved cases in the appropriate limits including richardsons treatment of reduced pairing in terms of rational gaudin algebra operators
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710.3942
Bottom Baryon Decays in Non-relativistic Quark Model
The reactions $\Sigma_b^* \to \Lambda_b \pi$, $\Sigma_b \to \Lambda_b \pi$, and $\Xi_b^* \to \Xi_b \pi$ are studied in the $^3P_0$ non-relativistic quark model with all the model parameters fixed in the sector of light quarks. The theoretical predictions for the decay widths $\Gamma_{\Sigma_b^* \to \Lambda_b \pi}$ and $\Gamma_{\Sigma_b \to \Lambda_b \pi}$ are consistent with the experimental data of the CDF Collaboration. Using as an input the recent mass of $\Xi_b$ and the theoretical predictions mass of $\Xi_b^{*}$, a narrow decay width about 1 MeV is predicted for the bottom baryon $\Xi_b^*$. The work suggests that the $^3P_0$ quark dynamics is of independence of environments where heavy quarks may or may not be a component of baryons.
hep-ph
the reactions sigma_b to lambda_b pi sigma_b to lambda_b pi and xi_b to xi_b pi are studied in the 3p_0 nonrelativistic quark model with all the model parameters fixed in the sector of light quarks the theoretical predictions for the decay widths gamma_sigma_b to lambda_b pi and gamma_sigma_b to lambda_b pi are consistent with the experimental data of the cdf collaboration using as an input the recent mass of xi_b and the theoretical predictions mass of xi_b a narrow decay width about 1 mev is predicted for the bottom baryon xi_b the work suggests that the 3p_0 quark dynamics is of independence of environments where heavy quarks may or may not be a component of baryons
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710.3943
Change of strength of vortex pinning in YBCO due to BaZrO_3 inclusions
We probe the short-range pinning properties with the application of microwave currents at very high driving frequencies (47.7 GHz) on YBa$_2$Cu$_3$O$_{7-\delta}$ films with and without sub-micrometer BaZrO$_3$ inclusions. We explore the temperature and field ranges 60 K$<T<T_c$ and 0$<\mu_0H<$0.8 T, with the field applied along the c-axis. The magnetic field induces a much smaller increase of the microwave resistivity, $\Delta \rho_1(H)+\mathrm{i}\Delta \rho_2(H)$, in YBa$_2$Cu$_3$O$_{7-\delta}$/BaZrO$_3$ with respect to pure YBa$_2$Cu$_3$O$_{7-\delta}$. $\Delta \rho_1(H)$ is slightly superlinear in pure YBa$_2$Cu$_3$O$_{7-\delta}$ (suggesting a possible contribution of thermal activation), but linear or sublinear in YBa$_2$Cu$_3$O$_{7-\delta}$/BaZrO$_3$ (suggesting a possible suppression of thermal activation as a consequence of BaZrO$_3$ inclusions). These features persist up to close to $T_c$. We discuss our data in terms of the ratio $r=\Delta X_s'(H)/\Delta R_s'(H)$ in the framework of the models for the microwave surface impedance in the mixed state. Large $r$ are found in YBa$_2$Cu$_3$O$_{7-\delta}$/BaZrO$_3$, with little field dependence. By contrast, smaller values and stronger field dependences are found in pure YBa$_2$Cu$_3$O$_{7-\delta}$. We discuss the different field dependence of the pinning constant.
cond-mat.supr-con cond-mat.mtrl-sci
we probe the shortrange pinning properties with the application of microwave currents at very high driving frequencies 477 ghz on yba_2cu_3o_7delta films with and without submicrometer bazro_3 inclusions we explore the temperature and field ranges 60 ktt_c and 0mu_0h08 t with the field applied along the caxis the magnetic field induces a much smaller increase of the microwave resistivity delta rho_1hmathrmidelta rho_2h in yba_2cu_3o_7deltabazro_3 with respect to pure yba_2cu_3o_7delta delta rho_1h is slightly superlinear in pure yba_2cu_3o_7delta suggesting a possible contribution of thermal activation but linear or sublinear in yba_2cu_3o_7deltabazro_3 suggesting a possible suppression of thermal activation as a consequence of bazro_3 inclusions these features persist up to close to t_c we discuss our data in terms of the ratio rdelta x_shdelta r_sh in the framework of the models for the microwave surface impedance in the mixed state large r are found in yba_2cu_3o_7deltabazro_3 with little field dependence by contrast smaller values and stronger field dependences are found in pure yba_2cu_3o_7delta we discuss the different field dependence of the pinning constant
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710.3944
Crystallographic modelling of protein loops and their heterogeneity with Rappertk
Background. All-atom crystallographic refinement of proteins is a laborious manually driven procedure, as a result of which, alternative and multiconformer interpretations are not routinely investigated. Results. We describe efficient loop sampling procedures in Rappertk and demonstrate that single loops in proteins can be automatically and accurately modelled with few positional restraints. Loops constructed with a composite CNS/Rappertk protocol consistently have better Rfree than those with CNS alone. This approach is extended to a more realistic scenario where there are often large positional uncertainties in loops along with small imperfections in the secondary structural framework. Both ensemble and collection methods are used to estimate the structural heterogeneity of loop regions. Conclusion. Apart from benchmarking Rappertk for the all-atom protein refinement task, this work also demonstrates its utility in both aspects of loop modelling - building a single conformer and estimating structural heterogeneity the loops can exhibit.
q-bio.BM
background allatom crystallographic refinement of proteins is a laborious manually driven procedure as a result of which alternative and multiconformer interpretations are not routinely investigated results we describe efficient loop sampling procedures in rappertk and demonstrate that single loops in proteins can be automatically and accurately modelled with few positional restraints loops constructed with a composite cnsrappertk protocol consistently have better rfree than those with cns alone this approach is extended to a more realistic scenario where there are often large positional uncertainties in loops along with small imperfections in the secondary structural framework both ensemble and collection methods are used to estimate the structural heterogeneity of loop regions conclusion apart from benchmarking rappertk for the allatom protein refinement task this work also demonstrates its utility in both aspects of loop modelling building a single conformer and estimating structural heterogeneity the loops can exhibit
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710.3945
Pinning down the New Minimal Supersymmetric GUT
We show that generic $ {\bf{10\oplus 120\oplus {\bar {126}}}}$ fits of fermion masses and mixings, using real superpotential couplings but with complex `Higgs fractions' leading to complex yukawa couplings in the effective MSSM, \emph{overdetermine}(by one extra constraint) the superpotential parameters of the New Minimal Supersymmetric SO(10) GUT\cite{nmsgut}. Therefore fits should properly be done by generating the 24 generic fit parameters from the 23 parameters of the NMSGUT superpotential, given $\tan\beta$ as input. Each numerical fit then \emph{fully specifies} the parameters of the NMSGUT. An analysis of all its implications, modulo only the residual uncertainty of supersymmetry breaking parameters, is now feasible. Thus the NMSGUT offers the possibility of a confrontation between the scale of gauge unification and the fit to fermion masses due to their extractable common dependence on the NMSGUT parameters. If and when `smoking gun' discoveries of Supersymmetry and Proton decay occur they will find the NMSGUT fully vulnerable to falsification.
hep-ph
we show that generic bf10oplus 120oplus bar 126 fits of fermion masses and mixings using real superpotential couplings but with complex higgs fractions leading to complex yukawa couplings in the effective mssm emphoverdetermineby one extra constraint the superpotential parameters of the new minimal supersymmetric so10 gutcitenmsgut therefore fits should properly be done by generating the 24 generic fit parameters from the 23 parameters of the nmsgut superpotential given tanbeta as input each numerical fit then emphfully specifies the parameters of the nmsgut an analysis of all its implications modulo only the residual uncertainty of supersymmetry breaking parameters is now feasible thus the nmsgut offers the possibility of a confrontation between the scale of gauge unification and the fit to fermion masses due to their extractable common dependence on the nmsgut parameters if and when smoking gun discoveries of supersymmetry and proton decay occur they will find the nmsgut fully vulnerable to falsification
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710.3946
Search for Supersymmetry in Di-Photon Final States at sqrt{s} = 1.96 TeV
We report results of a search for supersymmetry (SUSY) with gauge-mediated symmetry breaking in di-photon events collected by the D0 experiment at the Fermilab Tevatron Collider in 2002--2006. In 1.1 fb$^{-1}$ of data, we find no significant excess beyond the background expected from the standard model and set the most stringent lower limits to date for a standard benchmark model on the lightest neutralino and chargino masses of 125 GeV and 229 GeV, respectively, at 95% confidence.
hep-ex
we report results of a search for supersymmetry susy with gaugemediated symmetry breaking in diphoton events collected by the d0 experiment at the fermilab tevatron collider in 20022006 in 11 fb1 of data we find no significant excess beyond the background expected from the standard model and set the most stringent lower limits to date for a standard benchmark model on the lightest neutralino and chargino masses of 125 gev and 229 gev respectively at 95 confidence
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710.3947
First Eigenvalues of Geometric Operators under the Ricci Flow
In this paper, we prove that the first eigenvalues of $-\Delta + cR$ ($c\geq \frac14$) is nondecreasing under the Ricci flow. We also prove the monotonicity under the normalized flow for the case $c=1/4$, and $r\le 0$.
math.DG
in this paper we prove that the first eigenvalues of delta cr cgeq frac14 is nondecreasing under the ricci flow we also prove the monotonicity under the normalized flow for the case c14 and rle 0
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710.3948
RNA sampling and crystallographic refinement using Rappertk
Background. Dramatic increases in RNA structural data have made it possible to recognize its conformational preferences much better than a decade ago. This has created an opportunity to use discrete restraint-based conformational sampling for modelling RNA and automating its crystallographic refinement. Results. All-atom sampling of entire RNA chains, termini and loops is achieved using the Richardson RNA backbone rotamer library and an unbiased distribution for glycosidic dihedral angle. Sampling behaviour of Rappertk on a diverse dataset of RNA chains under varying spatial restraints is benchmarked. The iterative composite crystallographic refinement protocol developed here is demonstrated to outperform CNS-only refinement on parts of tRNA(Asp) structure. Conclusion. This work opens exciting possibilities for further work in RNA modelling and crystallography.
q-bio.BM
background dramatic increases in rna structural data have made it possible to recognize its conformational preferences much better than a decade ago this has created an opportunity to use discrete restraintbased conformational sampling for modelling rna and automating its crystallographic refinement results allatom sampling of entire rna chains termini and loops is achieved using the richardson rna backbone rotamer library and an unbiased distribution for glycosidic dihedral angle sampling behaviour of rappertk on a diverse dataset of rna chains under varying spatial restraints is benchmarked the iterative composite crystallographic refinement protocol developed here is demonstrated to outperform cnsonly refinement on parts of trnaasp structure conclusion this work opens exciting possibilities for further work in rna modelling and crystallography
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710.3949
A note on pairs of metrics in a two-dimensional linear vector space
Pairs of metrics in a two-dimensional linear vector space are considered, one of which is a Minkowski type metric. Their simultaneous diagonalizability is studied and canonical presentations for them are suggested.
math.MG
pairs of metrics in a twodimensional linear vector space are considered one of which is a minkowski type metric their simultaneous diagonalizability is studied and canonical presentations for them are suggested
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710.395
Geometric phase gate on an optical transition for ion trap quantum computation
We propose a geometric phase gate of two ion qubits that are encoded in two levels linked by an optical dipole-forbidden transition. Compared to hyperfine geometric phase gates mediated by electric dipole transitions, the gate has many interesting properties, such as very low spontaneous emission rates, applicability to magnetic field insensitive states, and use of a co-propagating laser beam geometry. We estimate that current technology allows for infidelities of around 10$^{-4}$.
quant-ph
we propose a geometric phase gate of two ion qubits that are encoded in two levels linked by an optical dipoleforbidden transition compared to hyperfine geometric phase gates mediated by electric dipole transitions the gate has many interesting properties such as very low spontaneous emission rates applicability to magnetic field insensitive states and use of a copropagating laser beam geometry we estimate that current technology allows for infidelities of around 104
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710.3951
Nonlinear elasticity of composite networks of stiff biopolymers with flexible linkers
Motivated by recent experiments showing nonlinear elasticity of in vitro networks of the biopolymer actin cross-linked with filamin, we present an effective medium theory of flexibly cross-linked stiff polymer networks. We model such networks by randomly oriented elastic rods connected by flexible connectors to a surrounding elastic continuum, which self-consistently represents the behavior of the rest of the network. This model yields a crossover from a linear elastic regime to a highly nonlinear elastic regime that stiffens in a way quantitatively consistent with experiment.
cond-mat.soft
motivated by recent experiments showing nonlinear elasticity of in vitro networks of the biopolymer actin crosslinked with filamin we present an effective medium theory of flexibly crosslinked stiff polymer networks we model such networks by randomly oriented elastic rods connected by flexible connectors to a surrounding elastic continuum which selfconsistently represents the behavior of the rest of the network this model yields a crossover from a linear elastic regime to a highly nonlinear elastic regime that stiffens in a way quantitatively consistent with experiment
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710.3952
The fractional stochastic heat equation on the circle: Time regularity and potential theory
We consider a system of $d$ linear stochastic heat equations driven by an additive infinite-dimensional fractional Brownian noise on the unit circle $S^1$. We obtain sharp results on the H\"older continuity in time of the paths of the solution $u=\{u(t, x)\}_{t \in \mathbb{R}_+, x \in S^1}$. We then establish upper and lower bounds on hitting probabilities of $u$, in terms of respectively Hausdorff measure and Newtonian capacity.
math.PR
we consider a system of d linear stochastic heat equations driven by an additive infinitedimensional fractional brownian noise on the unit circle s1 we obtain sharp results on the holder continuity in time of the paths of the solution uut x_t in mathbbr_ x in s1 we then establish upper and lower bounds on hitting probabilities of u in terms of respectively hausdorff measure and newtonian capacity
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