General relativity contains solutions in which two distant black holes are
connected through the interior via a wormhole, or Einstein-Rosen bridge. These
solutions can be interpreted as maximally entangled states of two black holes
that form a complex EPR pair. We suggest that similar bridges might be present
for more general entangled states.
In the case of entangled black holes one can formulate versions of the
AMPS(S) paradoxes and resolve them. This suggests possible resolutions of the
firewall paradoxes for more general situations.
%0 Journal Article
%1 Maldacena2013Cool
%A Maldacena, Juan
%A Susskind, Leonard
%D 2013
%J Fortschritte der Physik
%K firewall
%N 9
%P 781--811
%R 10.1002/prop.201300020
%T Cool horizons for entangled black holes
%U http://dx.doi.org/10.1002/prop.201300020
%V 61
%X General relativity contains solutions in which two distant black holes are
connected through the interior via a wormhole, or Einstein-Rosen bridge. These
solutions can be interpreted as maximally entangled states of two black holes
that form a complex EPR pair. We suggest that similar bridges might be present
for more general entangled states.
In the case of entangled black holes one can formulate versions of the
AMPS(S) paradoxes and resolve them. This suggests possible resolutions of the
firewall paradoxes for more general situations.
@article{Maldacena2013Cool,
abstract = {{General relativity contains solutions in which two distant black holes are
connected through the interior via a wormhole, or Einstein-Rosen bridge. These
solutions can be interpreted as maximally entangled states of two black holes
that form a complex EPR pair. We suggest that similar bridges might be present
for more general entangled states.
In the case of entangled black holes one can formulate versions of the
AMPS(S) paradoxes and resolve them. This suggests possible resolutions of the
firewall paradoxes for more general situations.}},
added-at = {2019-02-26T10:37:35.000+0100},
archiveprefix = {arXiv},
author = {Maldacena, Juan and Susskind, Leonard},
biburl = {https://www.bibsonomy.org/bibtex/2386ef33b310ce4109d082b842bf46bce/acastro},
citeulike-article-id = {12390239},
citeulike-linkout-0 = {http://arxiv.org/abs/1306.0533},
citeulike-linkout-1 = {http://arxiv.org/pdf/1306.0533},
citeulike-linkout-2 = {http://dx.doi.org/10.1002/prop.201300020},
day = 11,
doi = {10.1002/prop.201300020},
eprint = {1306.0533},
interhash = {aba0218522d316f1a41c4bb934057368},
intrahash = {386ef33b310ce4109d082b842bf46bce},
issn = {00158208},
journal = {Fortschritte der Physik},
keywords = {firewall},
month = jul,
number = 9,
pages = {781--811},
posted-at = {2013-06-04 02:38:45},
priority = {2},
timestamp = {2019-02-26T10:37:35.000+0100},
title = {{Cool horizons for entangled black holes}},
url = {http://dx.doi.org/10.1002/prop.201300020},
volume = 61,
year = 2013
}