1. Equation of State of Hot Dense Hyperonic Matter in the Quark-Meson-Coupling (QMC-A) model
- Author
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Veronica Dexheimer, Anthony W. Thomas, S. Typel, P. A. M. Guichon, Jirina Stone, Département de Physique Nucléaire (ex SPhN) (DPHN), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, and HEP, INSPIRE
- Subjects
[PHYS.NUCL] Physics [physics]/Nuclear Theory [nucl-th] ,Equation of state ,Nuclear Theory ,baryon number: density ,hyperon ,01 natural sciences ,conformal ,star ,stars: evolution ,Nuclear Experiment ,neutron star ,010303 astronomy & astrophysics ,threshold: density ,Physics ,High Energy Astrophysical Phenomena (astro-ph.HE) ,critical phenomena ,equilibrium: chemical ,velocity: acoustic ,temperature: effect ,Astrophysics - Solar and Stellar Astrophysics ,adiabatic ,nucleon hyperon ,baryon: octet ,Neutrino ,Astrophysics - High Energy Astrophysical Phenomena ,Quark ,dense matter ,Meson ,[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th] ,FOS: Physical sciences ,finite temperature ,Nuclear physics ,Nuclear Theory (nucl-th) ,stars: neutron ,mean field approximation: chiral ,nuclear physics ,0103 physical sciences ,meson quark: coupling ,Solar and Stellar Astrophysics (astro-ph.SR) ,equation of state ,010308 nuclear & particles physics ,model: relativistic ,High Energy Physics::Phenomenology ,Hyperon ,temperature ,Astronomy and Astrophysics ,Baryon ,star: massive ,Neutron star ,Space and Planetary Science ,Baryon number ,[PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph] ,entropy ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] - Abstract
We report a new equation of state (EoS) of cold and hot hyperonic matter constructed in the framework of the quark-meson-coupling (QMC-A) model. The QMC-A EoS yields results compatible with available nuclear physics constraints and astrophysical observations. It covers the range of temperatures from T=0 to 100 MeV, entropies per particle S/A between 0 and 6, lepton fractions from Y$_L$=0.0 to 0.6, and baryon number densities n$_B$=0.05-1.2 fm$^{-3}$. Applications of the QMC-A EoS are made to cold neutron stars (NS) and to hot proto-neutron stars (PNS) in two scenarios, (i) lepton rich matter with trapped neutrinos and (ii) deleptonized chemically equilibrated matter. We find that the QMC-A model predicts hyperons in amounts growing with increasing temperature and density, thus suggesting not only their presence in PNS but also, most likely, in NS merger remnants. The nucleon-hyperon phase transition is studied through the adiabatic index and the speed of sound c$_s$. It is shown that the lowering of (c$_s$/c)$^2$ to and below the conformal limit of 1/3 is a general consequence of instabilities due to any phase transition and is not a unique fingerprint of the hadron-quark matter transition. Rigid rotation of cold and hot stars, their moments of inertia and Kepler frequencies are also explored. The QMC-A model results are compared with two relativistic models, the chiral mean field model (CMF), and the generalized relativistic density functional with hyperons (GRDF-Y). Similarities and differences are discussed., Comment: 14 pages, 14 figures. Final version accepted for publication in MNRAS 2020 December 17
- Published
- 2019
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