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Hot quark matter and merger remnants

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Autor(es):
Issifu, Adamu ; Frederico, Tobias
Número total de Autores: 2
Tipo de documento: Artigo Científico
Fonte: EUROPEAN PHYSICAL JOURNAL A; v. 61, n. 8, p. 19-pg., 2025-08-05.
Resumo

This work investigates hot quark matter under the thermodynamic conditions characteristic of a binary neutron star (BNS) merger remnants. We used the density-dependent quark mass model (DDQM) to access the microscopic nuclear equation of state (EoS) in a series of snapshots. The strange quark matter (SQM) is studied at finite temperature and entropy, in the presence of electrons and muons and their corresponding neutrinos to simulate the BNS merger conditions. For the first time, we introduced temperature into the DDQM model using a lattice QCD-motivated approach to construct both isentropic and isothermal EoSs. We observe that as the entropy of the SQM increases, the merger remnant becomes more massive and increases in size, whereas the neutrino abundance also increases. In the fixed-temperature case, on the other hand, we observe that the entropy spreads from the surface towards the center of the remnant. We determine the particle distribution in the core of the remnants, the structure of the remnant, the temperature profile, sound velocity, and the polytropic index, and discuss their effects. The strange-quark star (SQS) remnants satisfy the 2M circle dot\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$2\,\mathrm{M_\odot }$$\end{document} mass constraint associated with neutron stars (NS). (AU)

Processo FAPESP: 23/09545-1 - Efeito da matéria escura na evolução de estrelas de neutron
Beneficiário:Adamu Issifu
Modalidade de apoio: Bolsas no Brasil - Pós-Doutorado
Processo FAPESP: 23/13749-1 - Análise de dados multidisciplinar em Big-data: de Física de Altas Energias à Astrofísica e Ciências Médicas
Beneficiário:Jun Takahashi
Modalidade de apoio: Auxílio à Pesquisa - Temático
Processo FAPESP: 19/07767-1 - Reações nucleares com núcleos fracamente ligados ou com estrutura de cluster, radioativos e estáveis
Beneficiário:Leandro Romero Gasques
Modalidade de apoio: Auxílio à Pesquisa - Temático