Phase Structure of Holographic Superconductors With Spontaneous Scalarization

Bibliographic Details
Main Author: Guo, Hong
Publication Date: 2025
Other Authors: Qian, Wei-Liang [UNESP], Wang, Bean
Format: Article
Language: eng
Source: Repositório Institucional da UNESP
Download full: http://dx.doi.org/10.1002/asna.20240145
https://hdl.handle.net/11449/296888
Summary: Within the holographic framework, we investigate the Einstein-scalar-Gauss-Bonnet theory coupled with a Maxwell field in an asymptotically anti-de Sitter (AdS) spacetime. Our findings reveal that holographic superconductor solutions exist when the Gauss-Bonnet coupling constant is below the critical value (Formula presented.), while spontaneous scalarization solutions emerge for (Formula presented.). This raises the question whether the hairy black holes triggered by different mechanisms are smoothly joined by a phase transition or whether these are actually identical solutions. To examine this transition in greater detail, we constructed a phase diagram in terms of temperature and chemical potential. By explicitly evaluating the Gibbs free energy and its derivatives, we demonstrate that a smooth yet first-order phase transition occurs between the two hairy solutions. In particular, a thermodynamic process can be devised in which a superconducting black hole transitions into a scalarized black hole by raising or lowering the temperature.
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spelling Phase Structure of Holographic Superconductors With Spontaneous Scalarizationfree energyholographic superconductorphase transitionspontaneous scalarizationWithin the holographic framework, we investigate the Einstein-scalar-Gauss-Bonnet theory coupled with a Maxwell field in an asymptotically anti-de Sitter (AdS) spacetime. Our findings reveal that holographic superconductor solutions exist when the Gauss-Bonnet coupling constant is below the critical value (Formula presented.), while spontaneous scalarization solutions emerge for (Formula presented.). This raises the question whether the hairy black holes triggered by different mechanisms are smoothly joined by a phase transition or whether these are actually identical solutions. To examine this transition in greater detail, we constructed a phase diagram in terms of temperature and chemical potential. By explicitly evaluating the Gibbs free energy and its derivatives, we demonstrate that a smooth yet first-order phase transition occurs between the two hairy solutions. In particular, a thermodynamic process can be devised in which a superconducting black hole transitions into a scalarized black hole by raising or lowering the temperature.Escola de Engenharia de Lorena UUniversidade de São Paulo, SPFaculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista, SPCenter for Gravitation and Cosmology College of Physical Science and Technology Yangzhou UniversityDepartment of Physical Sciences and Applied Mathematics Vanguard UniversityFaculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista, SPUniversidade de São Paulo (USP)Universidade Estadual Paulista (UNESP)Yangzhou UniversityVanguard UniversityGuo, HongQian, Wei-Liang [UNESP]Wang, Bean2025-04-29T18:04:54Z2025-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1002/asna.20240145Astronomische Nachrichten.1521-39940004-6337https://hdl.handle.net/11449/29688810.1002/asna.202401452-s2.0-85214823898Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengAstronomische Nachrichteninfo:eu-repo/semantics/openAccess2025-04-30T14:09:51Zoai:repositorio.unesp.br:11449/296888Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestrepositoriounesp@unesp.bropendoar:29462025-04-30T14:09:51Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Phase Structure of Holographic Superconductors With Spontaneous Scalarization
title Phase Structure of Holographic Superconductors With Spontaneous Scalarization
spellingShingle Phase Structure of Holographic Superconductors With Spontaneous Scalarization
Guo, Hong
free energy
holographic superconductor
phase transition
spontaneous scalarization
title_short Phase Structure of Holographic Superconductors With Spontaneous Scalarization
title_full Phase Structure of Holographic Superconductors With Spontaneous Scalarization
title_fullStr Phase Structure of Holographic Superconductors With Spontaneous Scalarization
title_full_unstemmed Phase Structure of Holographic Superconductors With Spontaneous Scalarization
title_sort Phase Structure of Holographic Superconductors With Spontaneous Scalarization
author Guo, Hong
author_facet Guo, Hong
Qian, Wei-Liang [UNESP]
Wang, Bean
author_role author
author2 Qian, Wei-Liang [UNESP]
Wang, Bean
author2_role author
author
dc.contributor.none.fl_str_mv Universidade de São Paulo (USP)
Universidade Estadual Paulista (UNESP)
Yangzhou University
Vanguard University
dc.contributor.author.fl_str_mv Guo, Hong
Qian, Wei-Liang [UNESP]
Wang, Bean
dc.subject.por.fl_str_mv free energy
holographic superconductor
phase transition
spontaneous scalarization
topic free energy
holographic superconductor
phase transition
spontaneous scalarization
description Within the holographic framework, we investigate the Einstein-scalar-Gauss-Bonnet theory coupled with a Maxwell field in an asymptotically anti-de Sitter (AdS) spacetime. Our findings reveal that holographic superconductor solutions exist when the Gauss-Bonnet coupling constant is below the critical value (Formula presented.), while spontaneous scalarization solutions emerge for (Formula presented.). This raises the question whether the hairy black holes triggered by different mechanisms are smoothly joined by a phase transition or whether these are actually identical solutions. To examine this transition in greater detail, we constructed a phase diagram in terms of temperature and chemical potential. By explicitly evaluating the Gibbs free energy and its derivatives, we demonstrate that a smooth yet first-order phase transition occurs between the two hairy solutions. In particular, a thermodynamic process can be devised in which a superconducting black hole transitions into a scalarized black hole by raising or lowering the temperature.
publishDate 2025
dc.date.none.fl_str_mv 2025-04-29T18:04:54Z
2025-01-01
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/10.1002/asna.20240145
Astronomische Nachrichten.
1521-3994
0004-6337
https://hdl.handle.net/11449/296888
10.1002/asna.20240145
2-s2.0-85214823898
url http://dx.doi.org/10.1002/asna.20240145
https://hdl.handle.net/11449/296888
identifier_str_mv Astronomische Nachrichten.
1521-3994
0004-6337
10.1002/asna.20240145
2-s2.0-85214823898
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Astronomische Nachrichten
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
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 repositoriounesp@unesp.br
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