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AdS / CFT对CFT纠缠的理解是基于双重体时空中的HRT表面。 尽管此类表面不必在足够普遍的时空中存在,但maximin构造表明,它们可以在任何光滑的渐近局部AdS时空中找到,而没有视界或仅具有Kasner类奇点。 在这项工作中,我们介绍了锚定到特定边界柯西切片C restricted的受限极大值曲面。 我们表明,当受限的极大值表面位于时空的平滑区域时,结果与原始的非受限的极大值处方相符。 然后,我们使用此构造将HRT表面的存在性定理扩展到其质量通胀奇异性不像Kasner一样的带电或自旋的AdS黑洞。 我们还将讨论与时间无关的带电虫洞中的相关问题。
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JHEP05(2019)127
Published for SISSA by Springer
Received: May 4, 2019
Accepted: May 13, 2019
Published: May 22, 2019
Restricted Maximin surfaces and HRT in generic
black hole spacetimes
Donald Marolf,
a
Aron C. Wall
b
and Zhencheng Wang
a
a
Department of Physics, University of California,
Santa Barbara, CA 93106, U.S.A.
b
Stanford Institute for Theoretical Physics, Stanford University,
382 Via Pueblo, Stanford, CA 94305, U.S.A.
E-mail: marolf@physics.ucsb.edu, aroncwall@gmail.com,
zhencheng@physics.ucsb.edu
Abstract: The AdS/CFT understanding of CFT entanglement is based on HRT sur-
faces in the dual bulk spacetime. While such surfaces need not exist in sufficiently general
spacetimes, the maximin construction demonstrates that they can be found in any smooth
asymptotically locally AdS spacetime without horizons or with only Kasner-like singu-
larities. In this work, we introduce restricted maximin surfaces anchored to a particular
boundary Cauchy slice C
∂
. We show that the result agrees with the original unrestricted
maximin prescription when the restricted maximin surface lies in a smooth region of space-
time. We then use this construction to extend the existence theorem for HRT surfaces to
generic charged or spinning AdS black holes whose mass-inflation singularities are not
Kasner-like. We also discuss related issues in time-independent charged wormholes.
Keywords: AdS-CFT Correspondence, Gauge-gravity correspondence, Black Holes
ArXiv ePrint: 1901.03879
Open Access,
c
The Authors.
Article funded by SCOAP
3
.
https://doi.org/10.1007/JHEP05(2019)127
JHEP05(2019)127
Contents
1 Introduction 1
2 Restricted maximin surfaces 3
2.1 Equivalence of HRT surfaces and restricted maximin surfaces in smooth
regions of spacetime 4
2.2 Existence of HRT surfaces in standard charged and rotating black holes 5
3 Discussion 6
1 Intro duction
As is by now well established [1, 2], in AdS/CFT the Ryu-Takayangi [3, 4] and Hubeny-
Rangamani-Takayanagi (HRT) [5] prescriptions generally describe the von Neumann en-
tropy of CFT regions A in terms of the area of an appropriate bulk surface. In particular,
S
A
=
Area[ext(A)]
4G
, (1.1)
where ext(A) is the smallest extremal surface satisfying ∂(ext(A)) = ∂A and with ext(A)
homologous to A. When there is more than one such surface with minimal area, the HRT
surface is ambiguous. Such situations arise at HRT phase transitions, when the HRT
surface jumps discontinuously as one varies the region A.
Now, there are spacetimes in which HRT surfaces fail to exist or where those that do
exist do not correctly compute the von Neumann entropy [6]. However, known spacetimes
M
0
with the latter issue are λ → 0 limits of spacetimes M
λ
in which the HRT prescription
succeeds, but where the correct (smallest) extremal surface recedes to the future or past
singularity as λ → 0. Similarly, known spacetimes M
0
0
where extremal surfaces fail to exist
are again λ → 0 limits of spacetimes M
λ
where HRT succeeds but in which all extremal
surfaces recede in this way.
One thus expects that HRT surfaces do in fact correctly compute the entropy in con-
texts such recessions are forbidden; i.e., where extremal surfaces are guaranteed to exist as
surfaces in smooth regions of the bulk. The maximin construction of [7] shows this to be
the case in asymptotically locally-AdS (AlAdS) spacetimes without horizons or where the
future and past boundaries consist only of Kasner-like singularities.
1
Ref. [7] also shows in
this context that HRT surfaces satisfy strong subadditivity.
1
In contrast, the examples of [6] contain smooth de Sitter-like pieces of future or past infinity as well
as special non-Kasner-like singular points where the smooth parts of future/past infinity meet otherwise-
Kasner-like singularities.
– 1 –
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