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First order phase transition in the D3-D7 model from the point of view of the fermionic spectral functions

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dc.contributor.authorGe, Xian-Hui-
dc.contributor.authorIshigaki, Shuta-
dc.contributor.authorSin, Sang-Jin-
dc.contributor.authorYuk, Taewon-
dc.date.accessioned2024-11-28T08:28:12Z-
dc.date.available2024-11-28T08:28:12Z-
dc.date.issued2024-07-
dc.identifier.issn2470-0010-
dc.identifier.issn2470-0029-
dc.identifier.urihttps://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/195223-
dc.description.abstractWe consider the D3-D7 model and use the spectral function of a probe fermion on D7 to analyze the first order phase transition from the black-hole embedding phase to another black-hole embedding phase in the presence of the finite density and temperature. From the fermionic spectral functions, we study the temperature dependence of the decay rate, and we observe various phenomena that support the first order phase transition including jump in it at the critical temperature that corresponds to the first order phase transition.-
dc.format.extent11-
dc.language영어-
dc.language.isoENG-
dc.publisherAMER PHYSICAL SOC-
dc.titleFirst order phase transition in the D3-D7 model from the point of view of the fermionic spectral functions-
dc.typeArticle-
dc.publisher.location미국-
dc.identifier.doi10.1103/PhysRevD.110.026003-
dc.identifier.scopusid2-s2.0-85198249105-
dc.identifier.wosid001291091700008-
dc.identifier.bibliographicCitationPhysical Review D, v.110, no.2, pp 1 - 11-
dc.citation.titlePhysical Review D-
dc.citation.volume110-
dc.citation.number2-
dc.citation.startPage1-
dc.citation.endPage11-
dc.type.docTypeArticle-
dc.description.isOpenAccessN-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaAstronomy & Astrophysics-
dc.relation.journalResearchAreaPhysics-
dc.relation.journalWebOfScienceCategoryAstronomy & Astrophysics-
dc.relation.journalWebOfScienceCategoryPhysics, Particles & Fields-
dc.identifier.urlhttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.110.026003-
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