Islands in linear dilaton black holes

Abstract We derive a novel four-dimensional black hole with planar horizon that asymptotes to the linear dilaton background. The usual growth of its entanglement entropy before Page’s time is established. After that, emergent islands modify to a large extent the entropy, which becomes finite and is...

Full description

Bibliographic Details
Main Authors: Georgios K. Karananas, Alex Kehagias, John Taskas
Format: Article
Language:English
Published: SpringerOpen 2021-03-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP03(2021)253
id doaj-4ecab958200f41c285f2ca792cb9dd6b
record_format Article
spelling doaj-4ecab958200f41c285f2ca792cb9dd6b2021-03-28T11:07:26ZengSpringerOpenJournal of High Energy Physics1029-84792021-03-012021312410.1007/JHEP03(2021)253Islands in linear dilaton black holesGeorgios K. Karananas0Alex Kehagias1John Taskas2Arnold Sommerfeld Center, Ludwig-Maximilians-Universität MünchenPhysics Division, National Technical University of AthensPhysics Division, National Technical University of AthensAbstract We derive a novel four-dimensional black hole with planar horizon that asymptotes to the linear dilaton background. The usual growth of its entanglement entropy before Page’s time is established. After that, emergent islands modify to a large extent the entropy, which becomes finite and is saturated by its Bekenstein-Hawking value in accordance with the finiteness of the von Neumann entropy of eternal black holes. We demonstrate that viewed from the string frame, our solution is the two-dimensional Witten black hole with two additional free bosons. We generalize our findings by considering a general class of linear dilaton black hole solutions at a generic point along the σ-model renormalization group (RG) equations. For those, we observe that the entanglement entropy is “running” i.e. it is changing along the RG flow with respect to the two-dimensional worldsheet length scale. At any fixed moment before Page’s time the aforementioned entropy increases towards the infrared (IR) domain, whereas the presence of islands leads the running entropy to decrease towards the IR at later times. Finally, we present a four-dimensional charged black hole that asymptotes to the linear dilaton background as well. We compute the associated entanglement entropy for the extremal case and we find that an island is needed in order for it to follow the Page curve.https://doi.org/10.1007/JHEP03(2021)253Black HolesBlack Holes in String Theory
collection DOAJ
language English
format Article
sources DOAJ
author Georgios K. Karananas
Alex Kehagias
John Taskas
spellingShingle Georgios K. Karananas
Alex Kehagias
John Taskas
Islands in linear dilaton black holes
Journal of High Energy Physics
Black Holes
Black Holes in String Theory
author_facet Georgios K. Karananas
Alex Kehagias
John Taskas
author_sort Georgios K. Karananas
title Islands in linear dilaton black holes
title_short Islands in linear dilaton black holes
title_full Islands in linear dilaton black holes
title_fullStr Islands in linear dilaton black holes
title_full_unstemmed Islands in linear dilaton black holes
title_sort islands in linear dilaton black holes
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2021-03-01
description Abstract We derive a novel four-dimensional black hole with planar horizon that asymptotes to the linear dilaton background. The usual growth of its entanglement entropy before Page’s time is established. After that, emergent islands modify to a large extent the entropy, which becomes finite and is saturated by its Bekenstein-Hawking value in accordance with the finiteness of the von Neumann entropy of eternal black holes. We demonstrate that viewed from the string frame, our solution is the two-dimensional Witten black hole with two additional free bosons. We generalize our findings by considering a general class of linear dilaton black hole solutions at a generic point along the σ-model renormalization group (RG) equations. For those, we observe that the entanglement entropy is “running” i.e. it is changing along the RG flow with respect to the two-dimensional worldsheet length scale. At any fixed moment before Page’s time the aforementioned entropy increases towards the infrared (IR) domain, whereas the presence of islands leads the running entropy to decrease towards the IR at later times. Finally, we present a four-dimensional charged black hole that asymptotes to the linear dilaton background as well. We compute the associated entanglement entropy for the extremal case and we find that an island is needed in order for it to follow the Page curve.
topic Black Holes
Black Holes in String Theory
url https://doi.org/10.1007/JHEP03(2021)253
work_keys_str_mv AT georgioskkarananas islandsinlineardilatonblackholes
AT alexkehagias islandsinlineardilatonblackholes
AT johntaskas islandsinlineardilatonblackholes
_version_ 1724200476978708480