Phase Structure of Holographic Superconductors With Spontaneous Scalarization
| Main Author: | |
|---|---|
| Publication Date: | 2025 |
| Other Authors: | , |
| 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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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 |
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Astronomische Nachrichten |
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info:eu-repo/semantics/openAccess |
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openAccess |
| dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
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Universidade Estadual Paulista (UNESP) |
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UNESP |
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UNESP |
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Repositório Institucional da UNESP |
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Repositório Institucional da UNESP |
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Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
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repositoriounesp@unesp.br |
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1834482628311384064 |