(Non-adiabatic) string creation on nice slices in Schwarzschild black holes
Autor(a) principal: | |
---|---|
Data de Publicação: | 2017 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1007/JHEP04(2017)156 http://hdl.handle.net/11449/174509 |
Resumo: | Nice slices have played a pivotal role in the discussion of the black hole information paradox as they avoid regions of strong spacetime curvature and yet smoothly cut through the infalling matter and the outgoing Hawking radiation, thus, justifying the use of low energy field theory. To avoid information loss it has been argued recently, however, that local effective field theory has to break down at the horizon. To assess the extent of this breakdown in a UV complete framework we study string-theoretic effects on nice slices in Schwarzschild black holes. Our purpose is two-fold. First, we use nice slices to address various open questions and caveats of [1] where it was argued that boost-enhanced non-adiabatic string-theoretic effects at the horizon could provide a dynamical mechanism for the firewall. Second, we identify two non-adiabatic effects on nice slices in Schwarzschild black holes: pair production of open strings near the horizon enhanced by the presence of the infinite tower of highly excited string states and a late-time non-adiabatic effect intrinsic to nice slices. |
id |
UNSP_c368c908fb7a4bf54f8e5d43e8613e2e |
---|---|
oai_identifier_str |
oai:repositorio.unesp.br:11449/174509 |
network_acronym_str |
UNSP |
network_name_str |
Repositório Institucional da UNESP |
repository_id_str |
2946 |
spelling |
(Non-adiabatic) string creation on nice slices in Schwarzschild black holesBlack HolesBlack Holes in String TheoryNice slices have played a pivotal role in the discussion of the black hole information paradox as they avoid regions of strong spacetime curvature and yet smoothly cut through the infalling matter and the outgoing Hawking radiation, thus, justifying the use of low energy field theory. To avoid information loss it has been argued recently, however, that local effective field theory has to break down at the horizon. To assess the extent of this breakdown in a UV complete framework we study string-theoretic effects on nice slices in Schwarzschild black holes. Our purpose is two-fold. First, we use nice slices to address various open questions and caveats of [1] where it was argued that boost-enhanced non-adiabatic string-theoretic effects at the horizon could provide a dynamical mechanism for the firewall. Second, we identify two non-adiabatic effects on nice slices in Schwarzschild black holes: pair production of open strings near the horizon enhanced by the presence of the infinite tower of highly excited string states and a late-time non-adiabatic effect intrinsic to nice slices.Jefferson Physical Laboratory Harvard UniversityBlack Hole Initiative Harvard UniversityDepartment of Physics University of CaliforniaInstituto de Física Teórica UNESP-Universidade Estadual Paulista, R. Dr. Bento T. Ferraz 271, Bl. IIKavli Institute for Theoretical Physics University of CaliforniaInstituto de Física Teórica UNESP-Universidade Estadual Paulista, R. Dr. Bento T. Ferraz 271, Bl. IIHarvard UniversityUniversity of CaliforniaUniversidade Estadual Paulista (Unesp)Puhm, AndreaRojas, Francisco [UNESP]Ugajin, Tomonori2018-12-11T17:11:28Z2018-12-11T17:11:28Z2017-04-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://dx.doi.org/10.1007/JHEP04(2017)156Journal of High Energy Physics, v. 2017, n. 4, 2017.1029-84791126-6708http://hdl.handle.net/11449/17450910.1007/JHEP04(2017)1562-s2.0-850184381462-s2.0-85018438146.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of High Energy Physics1,2271,227info:eu-repo/semantics/openAccess2024-01-05T06:27:14Zoai:repositorio.unesp.br:11449/174509Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T22:11:48.010723Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
(Non-adiabatic) string creation on nice slices in Schwarzschild black holes |
title |
(Non-adiabatic) string creation on nice slices in Schwarzschild black holes |
spellingShingle |
(Non-adiabatic) string creation on nice slices in Schwarzschild black holes Puhm, Andrea Black Holes Black Holes in String Theory |
title_short |
(Non-adiabatic) string creation on nice slices in Schwarzschild black holes |
title_full |
(Non-adiabatic) string creation on nice slices in Schwarzschild black holes |
title_fullStr |
(Non-adiabatic) string creation on nice slices in Schwarzschild black holes |
title_full_unstemmed |
(Non-adiabatic) string creation on nice slices in Schwarzschild black holes |
title_sort |
(Non-adiabatic) string creation on nice slices in Schwarzschild black holes |
author |
Puhm, Andrea |
author_facet |
Puhm, Andrea Rojas, Francisco [UNESP] Ugajin, Tomonori |
author_role |
author |
author2 |
Rojas, Francisco [UNESP] Ugajin, Tomonori |
author2_role |
author author |
dc.contributor.none.fl_str_mv |
Harvard University University of California Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Puhm, Andrea Rojas, Francisco [UNESP] Ugajin, Tomonori |
dc.subject.por.fl_str_mv |
Black Holes Black Holes in String Theory |
topic |
Black Holes Black Holes in String Theory |
description |
Nice slices have played a pivotal role in the discussion of the black hole information paradox as they avoid regions of strong spacetime curvature and yet smoothly cut through the infalling matter and the outgoing Hawking radiation, thus, justifying the use of low energy field theory. To avoid information loss it has been argued recently, however, that local effective field theory has to break down at the horizon. To assess the extent of this breakdown in a UV complete framework we study string-theoretic effects on nice slices in Schwarzschild black holes. Our purpose is two-fold. First, we use nice slices to address various open questions and caveats of [1] where it was argued that boost-enhanced non-adiabatic string-theoretic effects at the horizon could provide a dynamical mechanism for the firewall. Second, we identify two non-adiabatic effects on nice slices in Schwarzschild black holes: pair production of open strings near the horizon enhanced by the presence of the infinite tower of highly excited string states and a late-time non-adiabatic effect intrinsic to nice slices. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-04-01 2018-12-11T17:11:28Z 2018-12-11T17:11:28Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1007/JHEP04(2017)156 Journal of High Energy Physics, v. 2017, n. 4, 2017. 1029-8479 1126-6708 http://hdl.handle.net/11449/174509 10.1007/JHEP04(2017)156 2-s2.0-85018438146 2-s2.0-85018438146.pdf |
url |
http://dx.doi.org/10.1007/JHEP04(2017)156 http://hdl.handle.net/11449/174509 |
identifier_str_mv |
Journal of High Energy Physics, v. 2017, n. 4, 2017. 1029-8479 1126-6708 10.1007/JHEP04(2017)156 2-s2.0-85018438146 2-s2.0-85018438146.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Journal of High Energy Physics 1,227 1,227 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1808129403496955904 |