Bounds on the local energy density of holographic CFTs from bulk geometry
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Accepted version
Author(s)
Fischetti, S
Hickling, A
Wiseman, TAJ
Type
Journal Article
Abstract
The stress tensor is a basic local operator in any field theory; in the context of AdS/CFT, it is
the operator which is dual to the bulk geometry itself. Here we exploit this feature by using the
bulk geometry to place constraints on the local energy density in static states of holographic (2+ 1)-
dimensional CFTs living on a closed (but otherwise generally curved) spatial geometry. We allow
for the presence of a marginal scalar deformation, dual to a massless scalar field in the bulk. For
certain vacuum states in which the bulk geometry is well-behaved at zero temperature, we find that
the bulk equations of motion imply that the local energy density integrated over specific boundary
domains is negative. In the absence of scalar deformations, we use the inverse mean curvature flow
to show that if the CFT spatial geometry has spherical topology but non-constant curvature, the
local energy density must be positive somewhere. This result extends to other topologies, but only
for certain types of vacuum; in particular, for a generic toroidal boundary, the vacuum’s bulk dual
must be the zero-temperature limit of a toroidal black hole.
the operator which is dual to the bulk geometry itself. Here we exploit this feature by using the
bulk geometry to place constraints on the local energy density in static states of holographic (2+ 1)-
dimensional CFTs living on a closed (but otherwise generally curved) spatial geometry. We allow
for the presence of a marginal scalar deformation, dual to a massless scalar field in the bulk. For
certain vacuum states in which the bulk geometry is well-behaved at zero temperature, we find that
the bulk equations of motion imply that the local energy density integrated over specific boundary
domains is negative. In the absence of scalar deformations, we use the inverse mean curvature flow
to show that if the CFT spatial geometry has spherical topology but non-constant curvature, the
local energy density must be positive somewhere. This result extends to other topologies, but only
for certain types of vacuum; in particular, for a generic toroidal boundary, the vacuum’s bulk dual
must be the zero-temperature limit of a toroidal black hole.
Date Issued
2016-10-19
Date Acceptance
2016-09-01
Citation
Classical and Quantum Gravity, 2016, 33 (22)
ISSN
1361-6382
Publisher
IOP Publishing
Journal / Book Title
Classical and Quantum Gravity
Volume
33
Issue
22
Copyright Statement
© 2016 IOP Publishing Ltd. This article was published in Classical and Quantum Gravity, 2016, Vol: 33, no. 22.
Subjects
Science & Technology
Physical Sciences
Astronomy & Astrophysics
Physics, Multidisciplinary
Physics, Particles & Fields
Physics
black holes
CFT
energy density
AdS/CFT
MEAN-CURVATURE FLOW
GAUGED EXTENDED SUPERGRAVITY
PENROSE INEQUALITY
POSITIVE ENERGY
BLACK-HOLES
RENORMALIZATION
hep-th
gr-qc
Nuclear & Particles Physics
02 Physical Sciences
01 Mathematical Sciences
Publication Status
Published
Article Number
225003