Chiral transition and meson melting within improved holographic soft wall models
| dc.contributor.author | Ballon-Bayona, Alfonso | |
| dc.contributor.author | Bartz, Sean | |
| dc.contributor.author | Mamani, Luis A. H. | |
| dc.contributor.author | Rodrigues, Diego M. [UNESP] | |
| dc.contributor.institution | Universidade Federal do Rio de Janeiro (UFRJ) | |
| dc.contributor.institution | Indiana State University | |
| dc.contributor.institution | Universidade Federal Do Recosncavo da Bahia | |
| dc.contributor.institution | Universidade Estadual de Santa Cruz | |
| dc.contributor.institution | Universidade Estadual Paulista (UNESP) | |
| dc.date.accessioned | 2025-04-29T18:05:49Z | |
| dc.date.issued | 2025-02-01 | |
| dc.description.abstract | We describe the chiral transition for the quark condensate and the melting of scalar and vector mesons in two-flavor holographic quantum chromodynamics (holographic QCD). This is done by extending the improved holographic soft wall models proposed in Ballon-Bayona et al. [Phys. Rev. D 104, 126029 (2021)PRVDAQ2470-001010.1103/PhysRevD.104.126029] to finite temperature, by means of introducing an asymptotically anti-de Sitter black brane. We find that the chiral transition is second order in the chiral limit and a crossover for physical quark masses, as expected in two-flavor QCD. We investigate the melting of vector and scalar mesons in the deconfined plasma through the calculation of hadronic spectral functions. Fixing the model parameters by the meson spectrum at zero temperature, we find that the mesons melt at temperatures between 90 and 110 MeV and the chiral transition occurs around 129 MeV. We also provide a prediction for the hydrodynamic diffusion constant associated with a flavor current in the deconfined plasma. | en |
| dc.description.affiliation | Instituto de Física Universidade Federal Do Rio de Janeiro, 21.941-972 | |
| dc.description.affiliation | Department of Chemistry and Physics Indiana State University | |
| dc.description.affiliation | Centro de Ciências Exatas e Tecnológicas Universidade Federal Do Recosncavo da Bahia, Rua Rui Barbosa, 710, Bahia | |
| dc.description.affiliation | Laboratório de Astrofísica Teórica e Observacional Departamento de Ciências Exatas e Tecnológicas Universidade Estadual de Santa Cruz, Bahia | |
| dc.description.affiliation | Instituto de Física Teórica UNESP Universidade Estadual Paulista, R. Dr. Bento T. Ferraz 271, Bl. II | |
| dc.description.affiliationUnesp | Instituto de Física Teórica UNESP Universidade Estadual Paulista, R. Dr. Bento T. Ferraz 271, Bl. II | |
| dc.identifier | http://dx.doi.org/10.1103/PhysRevD.111.026011 | |
| dc.identifier.citation | Physical Review D, v. 111, n. 2, 2025. | |
| dc.identifier.doi | 10.1103/PhysRevD.111.026011 | |
| dc.identifier.issn | 2470-0029 | |
| dc.identifier.issn | 2470-0010 | |
| dc.identifier.scopus | 2-s2.0-85214982873 | |
| dc.identifier.uri | https://hdl.handle.net/11449/297180 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Physical Review D | |
| dc.source | Scopus | |
| dc.title | Chiral transition and meson melting within improved holographic soft wall models | en |
| dc.type | Artigo | pt |
| dspace.entity.type | Publication | |
| unesp.author.orcid | 0000-0001-5237-3456[1] | |
| unesp.author.orcid | 0000-0001-8683-8936[2] | |
| unesp.author.orcid | 0000-0002-8002-7072 0000-0002-8002-7072[3] | |
| unesp.author.orcid | 0000-0001-6372-5453[4] | |
| unesp.campus | Universidade Estadual Paulista (UNESP), Instituto de Física Teórica, São Paulo | pt |
