We identify conditions for the entanglement entropy as a function of spatial
region to be compatible with causality in an arbitrary relativistic quantum
field theory. We then prove that the covariant holographic entanglement entropy
prescription (which relates entanglement entropy of a given spatial region on
the boundary to the area of a certain extremal surface in the bulk) obeys these
conditions, as long as the bulk obeys the null energy condition. While
necessary for the validity of the prescription, this consistency requirement is
quite nontrivial from the bulk standpoint, and therefore provides important
additional evidence for the prescription. In the process, we introduce a
codimension-zero bulk region, named the entanglement wedge, naturally
associated with the given boundary spatial region. We propose that the
entanglement wedge is the most natural bulk region corresponding to the
boundary reduced density matrix.
%0 Generic
%1 Headrick2014Causality
%A Headrick, Matthew
%A Hubeny, Veronika E.
%A Lawrence, Albion
%A Rangamani, Mukund
%D 2014
%K entanglement
%T Causality & holographic entanglement entropy
%U http://arxiv.org/abs/1408.6300
%X We identify conditions for the entanglement entropy as a function of spatial
region to be compatible with causality in an arbitrary relativistic quantum
field theory. We then prove that the covariant holographic entanglement entropy
prescription (which relates entanglement entropy of a given spatial region on
the boundary to the area of a certain extremal surface in the bulk) obeys these
conditions, as long as the bulk obeys the null energy condition. While
necessary for the validity of the prescription, this consistency requirement is
quite nontrivial from the bulk standpoint, and therefore provides important
additional evidence for the prescription. In the process, we introduce a
codimension-zero bulk region, named the entanglement wedge, naturally
associated with the given boundary spatial region. We propose that the
entanglement wedge is the most natural bulk region corresponding to the
boundary reduced density matrix.
@misc{Headrick2014Causality,
abstract = {{We identify conditions for the entanglement entropy as a function of spatial
region to be compatible with causality in an arbitrary relativistic quantum
field theory. We then prove that the covariant holographic entanglement entropy
prescription (which relates entanglement entropy of a given spatial region on
the boundary to the area of a certain extremal surface in the bulk) obeys these
conditions, as long as the bulk obeys the null energy condition. While
necessary for the validity of the prescription, this consistency requirement is
quite nontrivial from the bulk standpoint, and therefore provides important
additional evidence for the prescription. In the process, we introduce a
codimension-zero bulk region, named the entanglement wedge, naturally
associated with the given boundary spatial region. We propose that the
entanglement wedge is the most natural bulk region corresponding to the
boundary reduced density matrix.}},
added-at = {2019-02-26T10:37:35.000+0100},
archiveprefix = {arXiv},
author = {Headrick, Matthew and Hubeny, Veronika E. and Lawrence, Albion and Rangamani, Mukund},
biburl = {https://www.bibsonomy.org/bibtex/2079916454549765d8c313e74d0599dbb/acastro},
citeulike-article-id = {13342347},
citeulike-linkout-0 = {http://arxiv.org/abs/1408.6300},
citeulike-linkout-1 = {http://arxiv.org/pdf/1408.6300},
day = 27,
eprint = {1408.6300},
interhash = {fe6a92bf8b069ed47a659fd5ac95a63c},
intrahash = {079916454549765d8c313e74d0599dbb},
keywords = {entanglement},
month = aug,
posted-at = {2014-09-01 07:51:45},
priority = {2},
timestamp = {2019-02-26T10:37:35.000+0100},
title = {{Causality \& holographic entanglement entropy}},
url = {http://arxiv.org/abs/1408.6300},
year = 2014
}