Holographic p-wave superfluid with Weyl corrections
Autor(a) principal: | |
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Data de Publicação: | 2020 |
Outros Autores: | , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1007/s11433-019-9604-x http://hdl.handle.net/11449/195322 |
Resumo: | In this work, we study the effects of the Weyl corrections on the p-wave superfluid phase transition in terms of an Einstein-Maxwell theory coupled to a complex vector field. In the probe limit, it is observed that the phase structure is significantly modified owing to the presence of the higher order Weyl corrections. The latter, in general, facilitates the emergence of the superfluid phase as the condensate increases with the Weyl coupling measured by gamma. Moreover, several features about the phase structure of the holographic superfluid are carefully investigated. In a specific region, the phase transition from the normal phase to the superfluid phase is identified to be the first order, instead of being the second order, as in the cases for many holographic superconductors. By carrying out a numerical scan of model parameters, the boundary dividing these two types of transitions is located and shown to be rather sensitive to the strength of Weyl coupling. Also, a feature known as Cave of Winds, associated with the emergence of a second superfluid phase, is observed for specific choices of model parameters. However, it becomes less prominent and eventually disappears as gamma increases. Furthermore, for temperature in the vicinity of the critical one for vanishing superfluid velocity, denoted by T-0, the supercurrent is found to be independent of the Weyl coupling. The calculated ratio, of the condensate with vanishing superfluid velocity to that with maximal superfluid velocity, is in good agreement with that predicted by Ginzburg-Landau theory. While compared with the impact on the phase structure owing to the higher curvature corrections, the findings in our present study demonstrate entirely different characteristics. Further implications are discussed. |
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Holographic p-wave superfluid with Weyl correctionsAdSCFT correspondenceWeyl correctionsholographic superfluidIn this work, we study the effects of the Weyl corrections on the p-wave superfluid phase transition in terms of an Einstein-Maxwell theory coupled to a complex vector field. In the probe limit, it is observed that the phase structure is significantly modified owing to the presence of the higher order Weyl corrections. The latter, in general, facilitates the emergence of the superfluid phase as the condensate increases with the Weyl coupling measured by gamma. Moreover, several features about the phase structure of the holographic superfluid are carefully investigated. In a specific region, the phase transition from the normal phase to the superfluid phase is identified to be the first order, instead of being the second order, as in the cases for many holographic superconductors. By carrying out a numerical scan of model parameters, the boundary dividing these two types of transitions is located and shown to be rather sensitive to the strength of Weyl coupling. Also, a feature known as Cave of Winds, associated with the emergence of a second superfluid phase, is observed for specific choices of model parameters. However, it becomes less prominent and eventually disappears as gamma increases. Furthermore, for temperature in the vicinity of the critical one for vanishing superfluid velocity, denoted by T-0, the supercurrent is found to be independent of the Weyl coupling. The calculated ratio, of the condensate with vanishing superfluid velocity to that with maximal superfluid velocity, is in good agreement with that predicted by Ginzburg-Landau theory. While compared with the impact on the phase structure owing to the higher curvature corrections, the findings in our present study demonstrate entirely different characteristics. Further implications are discussed.National Natural Science Foundation of ChinaHunan Provincial Natural Science Foundation of ChinaFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Hunan Normal Univ, Synerget Innovat Ctr Quantum ffects & Applicat, Minist Educ, Key Lab Low Dimens Quantum Struct & Quantum Contr, Changsha 410081, Peoples R ChinaHunan Normal Univ, Dept Phys, Changsha 410081, Peoples R ChinaYangzhou Univ, Coll Phys Sci & Technol, Ctr Gravitat & Cosmol, Yangzhou 225009, Jiangsu, Peoples R ChinaUniv Sao Paulo, Escola Engn Lorena, BR-12602810 Lorena, BrazilUniv Estadual Paulista, Fac Engn Guaratingueta, BR-12516410 Guaratingueta, BrazilCent South Univ, Sch Phys & Elect, Changsha 410083, Peoples R ChinaUniv Estadual Paulista, Fac Engn Guaratingueta, BR-12516410 Guaratingueta, BrazilNational Natural Science Foundation of China: 11775076National Natural Science Foundation of China: 11875025National Natural Science Foundation of China: 11475061National Natural Science Foundation of China: 11690034Hunan Provincial Natural Science Foundation of China: 2016JJ1012Science PressHunan Normal UnivYangzhou UnivUniversidade de São Paulo (USP)Universidade Estadual Paulista (Unesp)Cent South UnivHuang, YongHaoPan, QiYuanQian, Wei-Liang [UNESP]Jing, JiLiangWang, ShiLiang2020-12-10T17:30:37Z2020-12-10T17:30:37Z2020-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article11http://dx.doi.org/10.1007/s11433-019-9604-xScience China-physics Mechanics & Astronomy. Beijing: Science Press, v. 63, n. 3, 11 p., 2020.1674-7348http://hdl.handle.net/11449/19532210.1007/s11433-019-9604-xWOS:000526927100001Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengScience China-physics Mechanics & Astronomyinfo:eu-repo/semantics/openAccess2021-10-23T07:46:13Zoai:repositorio.unesp.br:11449/195322Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T23:35:24.543231Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Holographic p-wave superfluid with Weyl corrections |
title |
Holographic p-wave superfluid with Weyl corrections |
spellingShingle |
Holographic p-wave superfluid with Weyl corrections Huang, YongHao AdS CFT correspondence Weyl corrections holographic superfluid |
title_short |
Holographic p-wave superfluid with Weyl corrections |
title_full |
Holographic p-wave superfluid with Weyl corrections |
title_fullStr |
Holographic p-wave superfluid with Weyl corrections |
title_full_unstemmed |
Holographic p-wave superfluid with Weyl corrections |
title_sort |
Holographic p-wave superfluid with Weyl corrections |
author |
Huang, YongHao |
author_facet |
Huang, YongHao Pan, QiYuan Qian, Wei-Liang [UNESP] Jing, JiLiang Wang, ShiLiang |
author_role |
author |
author2 |
Pan, QiYuan Qian, Wei-Liang [UNESP] Jing, JiLiang Wang, ShiLiang |
author2_role |
author author author author |
dc.contributor.none.fl_str_mv |
Hunan Normal Univ Yangzhou Univ Universidade de São Paulo (USP) Universidade Estadual Paulista (Unesp) Cent South Univ |
dc.contributor.author.fl_str_mv |
Huang, YongHao Pan, QiYuan Qian, Wei-Liang [UNESP] Jing, JiLiang Wang, ShiLiang |
dc.subject.por.fl_str_mv |
AdS CFT correspondence Weyl corrections holographic superfluid |
topic |
AdS CFT correspondence Weyl corrections holographic superfluid |
description |
In this work, we study the effects of the Weyl corrections on the p-wave superfluid phase transition in terms of an Einstein-Maxwell theory coupled to a complex vector field. In the probe limit, it is observed that the phase structure is significantly modified owing to the presence of the higher order Weyl corrections. The latter, in general, facilitates the emergence of the superfluid phase as the condensate increases with the Weyl coupling measured by gamma. Moreover, several features about the phase structure of the holographic superfluid are carefully investigated. In a specific region, the phase transition from the normal phase to the superfluid phase is identified to be the first order, instead of being the second order, as in the cases for many holographic superconductors. By carrying out a numerical scan of model parameters, the boundary dividing these two types of transitions is located and shown to be rather sensitive to the strength of Weyl coupling. Also, a feature known as Cave of Winds, associated with the emergence of a second superfluid phase, is observed for specific choices of model parameters. However, it becomes less prominent and eventually disappears as gamma increases. Furthermore, for temperature in the vicinity of the critical one for vanishing superfluid velocity, denoted by T-0, the supercurrent is found to be independent of the Weyl coupling. The calculated ratio, of the condensate with vanishing superfluid velocity to that with maximal superfluid velocity, is in good agreement with that predicted by Ginzburg-Landau theory. While compared with the impact on the phase structure owing to the higher curvature corrections, the findings in our present study demonstrate entirely different characteristics. Further implications are discussed. |
publishDate |
2020 |
dc.date.none.fl_str_mv |
2020-12-10T17:30:37Z 2020-12-10T17:30:37Z 2020-01-01 |
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/s11433-019-9604-x Science China-physics Mechanics & Astronomy. Beijing: Science Press, v. 63, n. 3, 11 p., 2020. 1674-7348 http://hdl.handle.net/11449/195322 10.1007/s11433-019-9604-x WOS:000526927100001 |
url |
http://dx.doi.org/10.1007/s11433-019-9604-x http://hdl.handle.net/11449/195322 |
identifier_str_mv |
Science China-physics Mechanics & Astronomy. Beijing: Science Press, v. 63, n. 3, 11 p., 2020. 1674-7348 10.1007/s11433-019-9604-x WOS:000526927100001 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Science China-physics Mechanics & Astronomy |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
11 |
dc.publisher.none.fl_str_mv |
Science Press |
publisher.none.fl_str_mv |
Science Press |
dc.source.none.fl_str_mv |
Web of Science 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_ |
1808129533897867264 |