Generating string solutions in BTZ

Detalhes bibliográficos
Autor(a) principal: David, Justin R.
Data de Publicação: 2013
Outros Autores: Kalousios, Chrysostomos [UNESP], Sadhukhan, Abhishake
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1007/JHEP02(2013)013
http://hdl.handle.net/11449/74599
Resumo: Integrability of classical strings in the BTZ black hole enables the construction and study of classical string propagation in this background. We first apply the dressing method to obtain classical string solutions in the BTZ black hole. We dress time like geodesics in the BTZ black hole and obtain open string solutions which are pinned on the boundary at a single point and whose end points move on time like geodesics. These strings upon regularising their charge and spins have a dispersion relation similar to that of giant magnons. We then dress space like geodesics which start and end on the boundary of the BTZ black hole and obtain minimal surfaces which can penetrate the horizon of the black hole while being pinned at the boundary. Finally we embed the giant gluon solutions in the BTZ background in two different ways. They can be embedded as a spiral which contracts and expands touching the horizon or a spike which originates from the boundary and touches the horizon. © 2013 SISSA, Trieste, Italy.
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spelling Generating string solutions in BTZAdS-CFT CorrespondenceBlack HolesIntegrable Equations in PhysicsIntegrability of classical strings in the BTZ black hole enables the construction and study of classical string propagation in this background. We first apply the dressing method to obtain classical string solutions in the BTZ black hole. We dress time like geodesics in the BTZ black hole and obtain open string solutions which are pinned on the boundary at a single point and whose end points move on time like geodesics. These strings upon regularising their charge and spins have a dispersion relation similar to that of giant magnons. We then dress space like geodesics which start and end on the boundary of the BTZ black hole and obtain minimal surfaces which can penetrate the horizon of the black hole while being pinned at the boundary. Finally we embed the giant gluon solutions in the BTZ background in two different ways. They can be embedded as a spiral which contracts and expands touching the horizon or a spike which originates from the boundary and touches the horizon. © 2013 SISSA, Trieste, Italy.Centre for High Energy Physics Indian Institute of Science, C.V. Raman Avenue, Bangalore 560012Institut für Physik der Humboldt-Universität zu Berlin, Newtonstraße 15, D-12489 BerlinICTP South American Institute for Fundamental Research Instituto de Física Teórica UNESP-Universidade Estadual Paulista, R. Dr. Bento T. Ferraz 271 - Bl. II, 01140-070 São Paulo SPICTP South American Institute for Fundamental Research Instituto de Física Teórica UNESP-Universidade Estadual Paulista, R. Dr. Bento T. Ferraz 271 - Bl. II, 01140-070 São Paulo SPIndian Institute of ScienceInstitut für Physik der Humboldt-Universität zu BerlinUniversidade Estadual Paulista (Unesp)David, Justin R.Kalousios, Chrysostomos [UNESP]Sadhukhan, Abhishake2014-05-27T11:28:27Z2014-05-27T11:28:27Z2013-02-18info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://dx.doi.org/10.1007/JHEP02(2013)013Journal of High Energy Physics, v. 2013, n. 2, 2013.1126-67081029-8479http://hdl.handle.net/11449/7459910.1007/JHEP02(2013)013WOS:0003162729000132-s2.0-848736759172-s2.0-84873675917.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of High Energy Physics5.5411,2271,227info:eu-repo/semantics/openAccess2023-10-27T06:12:54Zoai:repositorio.unesp.br:11449/74599Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462023-10-27T06:12:54Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Generating string solutions in BTZ
title Generating string solutions in BTZ
spellingShingle Generating string solutions in BTZ
David, Justin R.
AdS-CFT Correspondence
Black Holes
Integrable Equations in Physics
title_short Generating string solutions in BTZ
title_full Generating string solutions in BTZ
title_fullStr Generating string solutions in BTZ
title_full_unstemmed Generating string solutions in BTZ
title_sort Generating string solutions in BTZ
author David, Justin R.
author_facet David, Justin R.
Kalousios, Chrysostomos [UNESP]
Sadhukhan, Abhishake
author_role author
author2 Kalousios, Chrysostomos [UNESP]
Sadhukhan, Abhishake
author2_role author
author
dc.contributor.none.fl_str_mv Indian Institute of Science
Institut für Physik der Humboldt-Universität zu Berlin
Universidade Estadual Paulista (Unesp)
dc.contributor.author.fl_str_mv David, Justin R.
Kalousios, Chrysostomos [UNESP]
Sadhukhan, Abhishake
dc.subject.por.fl_str_mv AdS-CFT Correspondence
Black Holes
Integrable Equations in Physics
topic AdS-CFT Correspondence
Black Holes
Integrable Equations in Physics
description Integrability of classical strings in the BTZ black hole enables the construction and study of classical string propagation in this background. We first apply the dressing method to obtain classical string solutions in the BTZ black hole. We dress time like geodesics in the BTZ black hole and obtain open string solutions which are pinned on the boundary at a single point and whose end points move on time like geodesics. These strings upon regularising their charge and spins have a dispersion relation similar to that of giant magnons. We then dress space like geodesics which start and end on the boundary of the BTZ black hole and obtain minimal surfaces which can penetrate the horizon of the black hole while being pinned at the boundary. Finally we embed the giant gluon solutions in the BTZ background in two different ways. They can be embedded as a spiral which contracts and expands touching the horizon or a spike which originates from the boundary and touches the horizon. © 2013 SISSA, Trieste, Italy.
publishDate 2013
dc.date.none.fl_str_mv 2013-02-18
2014-05-27T11:28:27Z
2014-05-27T11:28:27Z
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/JHEP02(2013)013
Journal of High Energy Physics, v. 2013, n. 2, 2013.
1126-6708
1029-8479
http://hdl.handle.net/11449/74599
10.1007/JHEP02(2013)013
WOS:000316272900013
2-s2.0-84873675917
2-s2.0-84873675917.pdf
url http://dx.doi.org/10.1007/JHEP02(2013)013
http://hdl.handle.net/11449/74599
identifier_str_mv Journal of High Energy Physics, v. 2013, n. 2, 2013.
1126-6708
1029-8479
10.1007/JHEP02(2013)013
WOS:000316272900013
2-s2.0-84873675917
2-s2.0-84873675917.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Journal of High Energy Physics
5.541
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
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