38,397 research outputs found

    One Loop Tests of Higher Spin AdS/CFT

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    Vasiliev's type A higher spin theories in AdS4 have been conjectured to be dual to the U(N) or O(N) singlet sectors in 3-d conformal field theories with N-component scalar fields. We compare the O(N^0) correction to the 3-sphere free energy F in the CFTs with corresponding calculations in the higher spin theories. This requires evaluating a regularized sum over one loop vacuum energies of an infinite set of massless higher spin gauge fields in Euclidean AdS4. For the Vasiliev theory including fields of all integer spin and a scalar with Delta=1 boundary condition, we show that the regularized sum vanishes. This is in perfect agreement with the vanishing of subleading corrections to F in the U(N) singlet sector of the theory of N free complex scalar fields. For the minimal Vasiliev theory including fields of only even spin, the regularized sum remarkably equals the value of F for one free real scalar field. This result may agree with the O(N) singlet sector of the theory of N real scalar fields, provided the coupling constant in the Vasiliev theory is identified as G_N ~ 1/(N-1). Similarly, consideration of the USp(N) singlet sector for N complex scalar fields, which we conjecture to be dual to the husp(2;0|4) Vasiliev theory, requires G_N ~ 1/(N+1). We also test the higher spin AdS3/CFT2 conjectures by calculating the regularized sum over one loop vacuum energies of higher spin fields in AdS3. We match the result with the O(N^0) term in the central charge of the W_N minimal models; this requires a certain truncation of the CFT operator spectrum so that the bulk theory contains two real scalar fields with the same boundary conditions.Comment: 20 pages. v3: minor corrections, version published in JHE

    Universality of free homogeneous sums in every dimension

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    We prove a general multidimensional invariance principle for a family of U-statistics based on freely independent non-commutative random variables of the type Un(S)U_n(S), where Un(x)U_n(x) is the nn-th Chebyshev polynomial and SS is a standard semicircular element on a fixed WW^{\ast}-probability space. As a consequence, we deduce that homogeneous sums based on random variables of this type are universal with respect to both semicircular and free Poisson approximations. Our results are stated in a general multidimensional setting and can be seen as a genuine extension of some recent findings by Deya and Nourdin; our techniques are based on the combination of the free Lindeberg method and the Fourth moment Theorem

    Interpolating between aa and FF

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    We study the dimensional continuation of the sphere free energy in conformal field theories. In continuous dimension dd we define the quantity F~=sin(πd/2)logZ\tilde F=\sin (\pi d/2)\log Z, where ZZ is the path integral of the Euclidean CFT on the dd-dimensional round sphere. F~\tilde F smoothly interpolates between (1)d/2π/2(-1)^{d/2}\pi/2 times the aa-anomaly coefficient in even dd, and (1)(d+1)/2(-1)^{(d+1)/2} times the sphere free energy FF in odd dd. We calculate F~\tilde F in various examples of unitary CFT that can be continued to non-integer dimensions, including free theories, double-trace deformations at large NN, and perturbative fixed points in the ϵ\epsilon expansion. For all these examples F~\tilde F is positive, and it decreases under RG flow. Using perturbation theory in the coupling, we calculate F~\tilde F in the Wilson-Fisher fixed point of the O(N)O(N) vector model in d=4ϵd=4-\epsilon to order ϵ4\epsilon^4. We use this result to estimate the value of FF in the 3-dimensional Ising model, and find that it is only a few percent below FF of the free conformally coupled scalar field. We use similar methods to estimate the FF values for the U(N)U(N) Gross-Neveu model in d=3d=3 and the O(N)O(N) model in d=5d=5. Finally, we carry out the dimensional continuation of interacting theories with 4 supercharges, for which we suggest that F~\tilde F may be calculated exactly using an appropriate version of localization on SdS^d. Our approach provides an interpolation between the aa-maximization in d=4d=4 and the FF-maximization in d=3d=3.Comment: 41 pages, 4 figures. v4: Eqs. (1.6), (4.13) and (5.37) corrected; footnote 9 added discussing the Euler density counterter

    Higher Spin AdSd+1_{d+1}/CFTd_d at One Loop

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    Following arXiv:1308.2337, we carry out one loop tests of higher spin AdSd+1_{d+1}/CFTd_d correspondences for d2d\geq 2. The Vasiliev theories in AdSd+1_{d+1}, which contain each integer spin once, are related to the U(N)U(N) singlet sector of the dd-dimensional CFT of NN free complex scalar fields; the minimal theories containing each even spin once -- to the O(N)O(N) singlet sector of the CFT of NN free real scalar fields. Using analytic continuation of higher spin zeta functions, which naturally regulate the spin sums, we calculate one loop vacuum energies in Euclidean AdSd+1_{d+1}. In even dd we compare the result with the O(N0)O(N^0) correction to the aa-coefficient of the Weyl anomaly; in odd dd -- with the O(N0)O(N^0) correction to the free energy FF on the dd-dimensional sphere. For the theories of integer spins, the correction vanishes in agreement with the CFT of NN free complex scalars. For the minimal theories, the correction always equals the contribution of one real conformal scalar field in dd dimensions. As explained in arXiv:1308.2337, this result may agree with the O(N)O(N) singlet sector of the theory of NN real scalar fields, provided the coupling constant in the higher spin theory is identified as GN1/(N1)G_N\sim 1/(N-1). Our calculations in even dd are closely related to finding the regularized aa-anomalies of conformal higher spin theories. In each even dd we identify two such theories with vanishing aa-anomaly: a theory of all integer spins, and a theory of all even spins coupled to a complex conformal scalar. We also discuss an interacting UV fixed point in d=5d=5 obtained from the free scalar theory via an irrelevant double-trace quartic interaction. This interacting large NN theory is dual to the Vasiliev theory in AdS6_6 where the bulk scalar is quantized with the alternate boundary condition.Comment: 35 pages. v2: minor improvement

    High resolution kinematics of galactic globular clusters. II. On the significance of velocity dispersion measurements

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    Small number statistics may heavily affect the structure of the broadening function in integrated spectra of galactic globular cluster centers. As a consequence, it is a priori unknown how closely line broadening measure- ments gauge the intrinsic velocity dispersions at the cores of these stel- lar systems. We have tackled this general problem by means of Monte Carlo simulations. An examination of the mode and the frequency distribution of the measured values of the simulations indicates that the low value measured for the velocity dispersion of M30 (Zaggia etal 1992) is likely a reliable estimate of the velocity dispersion at the center of this cluster. The same methodology applied to the case of M15 suggests that the steep inward rise of the velocity dispersion found by Peterson, Seitzer and Cudworth (1989) is real, although less pronounced. Large-aperture observa- tions are less sensitive to statistical fluctuations, but are unable to detect strong variations in the dispersion wich occur within the aperture itself.Comment: 6 pages, 8 figures upon request, Latex A&A style version 3.0, DAPD-20

    On CJC_{J} and CTC_{T} in Conformal QED

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    QED with a large number NN of massless fermionic degrees of freedom has a conformal phase in a range of space-time dimensions. We use a large NN diagrammatic approach to calculate the leading corrections to CTC_T, the coefficient of the two-point function of the stress-energy tensor, and CJC_J, the coefficient of the two-point function of the global symmetry current. We present explicit formulae as a function of dd and check them versus the expectations in 2 and 4ϵ4-\epsilon dimensions. Using our results in higher even dimensions we find a concise formula for CTC_T of the conformal Maxwell theory with higher derivative action Fμν(2)d22FμνF_{\mu \nu} (-\nabla^2)^{\frac{d}{2}-2} F^{\mu \nu}. In d=3d=3, QED has a topological symmetry current, and we calculate the correction to its two-point function coefficient, CJtopC^{\textrm{top}}_{J}. We also show that some RG flows involving QED in d=3d=3 obey CTUV>CTIRC_T^{\rm UV} > C_T^{\rm IR} and discuss possible implications of this inequality for the symmetry breaking at small values of NN.Comment: 29 pages, 9 figures. v3: minor improvements, references adde

    A notion of graph likelihood and an infinite monkey theorem

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    We play with a graph-theoretic analogue of the folklore infinite monkey theorem. We define a notion of graph likelihood as the probability that a given graph is constructed by a monkey in a number of time steps equal to the number of vertices. We present an algorithm to compute this graph invariant and closed formulas for some infinite classes. We have to leave the computational complexity of the likelihood as an open problem.Comment: 6 pages, 1 EPS figur

    The Newtonian limit of the relativistic Boltzmann equation

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    The relativistic Boltzmann equation for a constant differential cross section and with periodic boundary conditions is considered. The speed of light appears as a parameter c>c0c>c_0 for a properly large and positive c0c_0. A local existence and uniqueness theorem is proved in an interval of time independent of c>c0c>c_0 and conditions are given such that in the limit c+c\to +\infty the solutions converge, in a suitable norm, to the solutions of the non-relativistic Boltzmann equation for hard spheres.Comment: 12 page

    Enumerating five families of pattern-avoiding inversion sequences; and introducing the powered Catalan numbers

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    The first problem addressed by this article is the enumeration of some families of pattern-avoiding inversion sequences. We solve some enumerative conjectures left open by the foundational work on the topics by Corteel et al., some of these being also solved independently by Lin, and Kim and Lin. The strength of our approach is its robustness: we enumerate four families F1F2F3F4F_1 \subset F_2 \subset F_3 \subset F_4 of pattern-avoiding inversion sequences ordered by inclusion using the same approach. More precisely, we provide a generating tree (with associated succession rule) for each family FiF_i which generalizes the one for the family Fi1F_{i-1}. The second topic of the paper is the enumeration of a fifth family F5F_5 of pattern-avoiding inversion sequences (containing F4F_4). This enumeration is also solved \emph{via} a succession rule, which however does not generalize the one for F4F_4. The associated enumeration sequence, which we call the \emph{powered Catalan numbers}, is quite intriguing, and further investigated. We provide two different succession rules for it, denoted ΩpCat\Omega_{pCat} and Ωsteady\Omega_{steady}, and show that they define two types of families enumerated by powered Catalan numbers. Among such families, we introduce the \emph{steady paths}, which are naturally associated with Ωsteady\Omega_{steady}. They allow us to bridge the gap between the two types of families enumerated by powered Catalan numbers: indeed, we provide a size-preserving bijection between steady paths and valley-marked Dyck paths (which are naturally associated with ΩpCat\Omega_{pCat}). Along the way, we provide several nice connections to families of permutations defined by the avoidance of vincular patterns, and some enumerative conjectures.Comment: V2 includes modifications suggested by referees (in particular, a much shorter Section 3, to account for arXiv:1706.07213

    Real-space Hopfield diagonalization of inhomogeneous dispersive media

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    We introduce a real-space technique able to extend the standard Hopfield approach commonly used in quantum polaritonics to the case of inhomogeneous lossless materials interacting with the electromagnetic field. We derive the creation and annihilation polaritonic operators for the system normal modes as linear, space-dependent superpositions of the microscopic light and matter fields, and we invert the Hopfield transformation expressing the microscopic fields as functions of the polaritonic operators. As an example, we apply our approach to the case of a planar interface between vacuum and a polar dielectric, showing how we can consistently treat both propagative and surface modes, and express their nonlinear interactions, arising from phonon anharmonicity, as polaritonic scattering terms. We also show that our theory can be naturally extended to the case of dissipative materials
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