Generating string solutions in BTZ
Autor(a) principal: | |
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Data de Publicação: | 2013 |
Outros Autores: | , |
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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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:29462024-08-05T16:12:06.193022Repositório 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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1808128618445930496 |