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Holographic c-theorems in arbitrary dimensions (2011)

by R C Myers, A Sinha
Venue:JHEP
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The Exact Superconformal R-Symmetry Extremizes Z

by Daniel L. Jafferis , 2011
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Massive Gravity in Three Dimensions

by Hamid R. Afshar, Eric A. Bergshoeff, Wout Merbis
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... bulk mode. Deformations in unitary two dimensional CFTs are restricted by Zamolodchikov’s ctheorem [8]. The presence of a holographic c-theorem [9] can clarify the role of the higher-curvature terms =-=[10]-=-, as it implies a restriction on the coupling constants of these higher-derivative interactions in the bulk. The main aim of this paper is to systematically construct higher-derivative extensions of t...

Exact results for five-dimensional superconformal field theories with gravity duals,” arXiv:1207.4359 [hep-th

by Daniel L. Jafferis, Silviu S. Pufu
"... We apply the technique of supersymmetric localization to exactly compute the S5 par-tition function of several large N superconformal field theories in five dimensions that have AdS6 duals in massive type IIA supergravity. The localization computations are performed in the non-renormalizable effecti ..."
Abstract - Cited by 31 (0 self) - Add to MetaCart
We apply the technique of supersymmetric localization to exactly compute the S5 par-tition function of several large N superconformal field theories in five dimensions that have AdS6 duals in massive type IIA supergravity. The localization computations are performed in the non-renormalizable effective field theories obtained through relevant deformations of the UV superconformal field theories. We compare the S5 free energy to a holographic compu-tation of entanglement entropy in the AdS6 duals and find perfect agreement. In particular, we reproduce the N5/2 scaling of the S5 free energy that was expected from supergravity.
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...ed in three dimensions [17, 35–37]. This statement is consistent with the observation 3 that in theories with holographic duals, the entanglement entropy across a three-sphere decreases under RG flow =-=[35,38]-=-, and at the endpoints of the flow it approaches −F [30]. It is also consistent with the observation that −F decreases under slightly relevant perturbations of a CFT, and that it remains constant unde...

Entanglement entropy of black holes

by Sergey Solodukhin - Living Rev. Rel
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...l and it does not contain covariant derivatives of the Riemann tensor then the tensor Qµναβ is a partial derivative of the Lagrangian, Qµναβ = ∂L ∂Rαβµν . (74) Now, as was observed by Myers and Sinha =-=[180]-=- (see also [4]), one can re-express 2∑ i,j=1 (nµi n α i )(n ν jn β j )− (nµi nβi )(nνjnαj ) = ǫµνǫαβ , (75) where ǫαβ = nα1n β 2 − nα2nβ1 is the two-dimensional volume form in the space transverse to ...

Some Calculable Contributions to Holographic Entanglement Entropy

by Ling-yan Hung, Robert C. Myers, Michael Smolkin - JHEP , 2011
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...ose relation of these new terms with the trace anomaly. As is well known, with even d, EE in a CFT can be directly calculated using the trace anomaly, at least for geometries with sufficient symmetry =-=[3, 8, 6, 9]-=-. Typically, we consider the trace anomaly in a curved background, where it is usually related to various conformally invariant combinations of the curvature [24]. However, deforming the CFT with a re...

Entanglement entropy in higher derivative holography

by Arpan Bhattacharyya, Apratim Kaviraj, Aninda Sinha , 2013
"... We consider holographic entanglement entropy in higher derivative gravity theories. Recently Lewkowycz and Maldacena [1] have provided a method to derive the equations for the entangling surface from first principles. We use this method to compute the entangling surface in four derivative gravity. C ..."
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We consider holographic entanglement entropy in higher derivative gravity theories. Recently Lewkowycz and Maldacena [1] have provided a method to derive the equations for the entangling surface from first principles. We use this method to compute the entangling surface in four derivative gravity. Certain interesting differences compared to the two derivative case are pointed out. For Gauss-Bonnet gravity, we show that in the regime where this method is applicable, the resulting equations coincide with proposals in the literature as well as with what follows from considerations of the stress tensor on the entangling surface. Finally we demonstrate that the area functional in Gauss-Bonnet holography arises as a counterterm needed to make the Euclidean action free of power law divergences.

Holographic evolution of the mutual information

by Andrea Allais, Erik Tonni , 2011
"... We compute the time evolution of the mutual information in out of equilibrium quantum systems whose gravity duals are Vaidya spacetimes in three and four dimensions, which describe the formation of a black hole through the collapse of null dust. We find the holographic mutual information to be non m ..."
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We compute the time evolution of the mutual information in out of equilibrium quantum systems whose gravity duals are Vaidya spacetimes in three and four dimensions, which describe the formation of a black hole through the collapse of null dust. We find the holographic mutual information to be non monotonic in time and always monogamous in the ranges explored. We also find that there is a region in the configuration space where it vanishes at all times. We show that the null energy condition is a necessary condition for both the strong subadditivity of the holographic entanglement entropy and the monogamy of the holographic mutual information.

F-Theorem without Supersymmetry

by Igor R. Klebanov, Silviu S. Pufu, Benjamin R. Safdi , 2011
"... The conjectured F-theorem for three-dimensional field theories states that the finite part of the free energy on S3 decreases along RG trajectories and is stationary at the fixed points. In previous work various successful tests of this proposal were carried out for theories with N = 2 supersymmetry ..."
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The conjectured F-theorem for three-dimensional field theories states that the finite part of the free energy on S3 decreases along RG trajectories and is stationary at the fixed points. In previous work various successful tests of this proposal were carried out for theories with N = 2 supersymmetry. In this paper we perform more general tests that do not rely on supersymmetry. We study perturbatively the RG flows produced by weakly relevant operators and show that the free energy decreases monotonically. We also consider large N field theories perturbed by relevant double trace operators, free massive field theories, and some Chern-Simons gauge theories. In all cases the free energy in the IR is smaller than in the UV, consistent with the F-theorem. We discuss other odd-dimensional Euclidean theories on Sd and provide evidence that (−1)(d−1)/2 log |Z | decreases along RG flow; in the particular case d = 1 this is the well-known g-theorem.

Rényi Entropies for Free Field Theories

by Igor R. Klebanov, Silviu S. Pufu, Subir Sachdev, Benjamin R. Safdi
"... Rényi entropies Sq are useful measures of quantum entanglement; they can be calculated from traces of the reduced density matrix raised to power q, with q ≥ 0. For (d + 1)-dimensional conformal field theories, the Rényi entropies across Sd−1 may be extracted from the thermal partition functions of ..."
Abstract - Cited by 16 (2 self) - Add to MetaCart
Rényi entropies Sq are useful measures of quantum entanglement; they can be calculated from traces of the reduced density matrix raised to power q, with q ≥ 0. For (d + 1)-dimensional conformal field theories, the Rényi entropies across Sd−1 may be extracted from the thermal partition functions of these theories on either (d+1)-dimensional de Sitter space or R×Hd, where Hd is the d-dimensional hyperbolic space. These thermal partition functions can in turn be expressed as path integrals on branched coverings of the (d+ 1)-dimensional sphere and S1 × Hd, respectively. We calculate the Rényi entropies of free massless scalars and fermions in d = 2, and show how using zeta-function regularization one finds agreement between the calculations on the branched coverings of S3 and on S1 × H2. Analogous calculations for massive free fields provide monotonic interpolating functions between the Rényi entropies at the Gaussian and the trivial fixed points. Finally, we discuss similar Rényi entropy calculations in d> 2.
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...s on the AdS/CFT correspondence [38–40]. This approach has been used to calculate entanglement entropy across Sd−1 in CFTs that possess a dual description with weakly curved gravitational backgrounds =-=[28,41]-=-. All these results have led to conjectures that the 3-sphere free energy F , or equivalently minus the entanglement entropy across a circle, decreases along any RG flow and is stationary at the fixed...

On higher derivative gravity, c-theorems and cosmology

by Aninda Sinha
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...se in supersymmetric string theory, R3 corrections arise in nonsupersymmetric string theories [6]. Six derivative theories have featured recently in [7, 8, 9, 10, 11]. Following a suggestion by Myers =-=[7, 32]-=-, one of the main goals of this paper is to construct general lagrangians such that when – 1 – one considers fluctuations around (anti) de Sitter space, the linearized equations of motion are two deri...

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