38,397 research outputs found
One Loop Tests of Higher Spin AdS/CFT
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
We prove a general multidimensional invariance principle for a family of
U-statistics based on freely independent non-commutative random variables of
the type , where is the -th Chebyshev polynomial and is
a standard semicircular element on a fixed -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 and
We study the dimensional continuation of the sphere free energy in conformal
field theories. In continuous dimension we define the quantity , where is the path integral of the Euclidean CFT on
the -dimensional round sphere. smoothly interpolates between
times the -anomaly coefficient in even , and
times the sphere free energy in odd . We calculate
in various examples of unitary CFT that can be continued to
non-integer dimensions, including free theories, double-trace deformations at
large , and perturbative fixed points in the expansion. For all
these examples is positive, and it decreases under RG flow. Using
perturbation theory in the coupling, we calculate in the
Wilson-Fisher fixed point of the vector model in to order
. We use this result to estimate the value of in the
3-dimensional Ising model, and find that it is only a few percent below of
the free conformally coupled scalar field. We use similar methods to estimate
the values for the Gross-Neveu model in and the model
in . Finally, we carry out the dimensional continuation of interacting
theories with 4 supercharges, for which we suggest that may be
calculated exactly using an appropriate version of localization on . Our
approach provides an interpolation between the -maximization in and
the -maximization in .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 AdS/CFT at One Loop
Following arXiv:1308.2337, we carry out one loop tests of higher spin
AdS/CFT correspondences for . The Vasiliev theories in
AdS, which contain each integer spin once, are related to the
singlet sector of the -dimensional CFT of free complex scalar fields;
the minimal theories containing each even spin once -- to the singlet
sector of the CFT of 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 AdS. In even we
compare the result with the correction to the -coefficient of the
Weyl anomaly; in odd -- with the correction to the free energy
on the -dimensional sphere. For the theories of integer spins, the
correction vanishes in agreement with the CFT of free complex scalars. For
the minimal theories, the correction always equals the contribution of one real
conformal scalar field in dimensions. As explained in arXiv:1308.2337, this
result may agree with the singlet sector of the theory of real
scalar fields, provided the coupling constant in the higher spin theory is
identified as . Our calculations in even are closely
related to finding the regularized -anomalies of conformal higher spin
theories. In each even we identify two such theories with vanishing
-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 obtained from the free scalar theory via an irrelevant
double-trace quartic interaction. This interacting large theory is dual to
the Vasiliev theory in AdS 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
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 and in Conformal QED
QED with a large number of massless fermionic degrees of freedom has a
conformal phase in a range of space-time dimensions. We use a large
diagrammatic approach to calculate the leading corrections to , the
coefficient of the two-point function of the stress-energy tensor, and ,
the coefficient of the two-point function of the global symmetry current. We
present explicit formulae as a function of and check them versus the
expectations in 2 and dimensions. Using our results in higher even
dimensions we find a concise formula for of the conformal Maxwell theory
with higher derivative action . In , QED has a topological symmetry current, and we calculate the
correction to its two-point function coefficient, . We
also show that some RG flows involving QED in obey and discuss possible implications of this inequality for the
symmetry breaking at small values of .Comment: 29 pages, 9 figures. v3: minor improvements, references adde
A notion of graph likelihood and an infinite monkey theorem
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
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 for a properly large and positive . A local
existence and uniqueness theorem is proved in an interval of time independent
of and conditions are given such that in the limit 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
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 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 which
generalizes the one for the family .
The second topic of the paper is the enumeration of a fifth family of
pattern-avoiding inversion sequences (containing ). This enumeration is
also solved \emph{via} a succession rule, which however does not generalize the
one for . 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 and
, 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 . 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
).
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
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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