Tables of Hyperonic Matter Equation of State for Core-Collapse Supernovae

Abstract

We present sets of equation of state (EOS) of nuclear matter including hyperons using an SU_f(3) extended relativistic mean field (RMF) model with a wide coverage of density, temperature, and charge fraction for numerical simulations of core collapse supernovae. Coupling constants of Sigma and Xi hyperons with the sigma meson are determined to fit the hyperon potential depths in nuclear matter, U_Sigma(rho_0) ~ +30 MeV and U_Xi(rho_0) ~ -15 MeV, which are suggested from recent analyses of hyperon production reactions. At low densities, the EOS of uniform matter is connected with the EOS by Shen et al., in which formation of finite nuclei is included in the Thomas-Fermi approximation. In the present EOS, the maximum mass of neutron stars decreases from 2.17 M_sun (Ne mu) to 1.63 M_sun (NYe mu) when hyperons are included. In a spherical, adiabatic collapse of a 15$M_{\odot }$ star by the hydrodynamics without neutrino transfer, hyperon effects are found to be small, since the temperature and density do not reach the region of hyperon mixture, where the hyperon fraction is above 1 % (T > 40 MeV or rho_B > 0.4 fm^{-3}).

23 pages, 6 figures (Fig.3 and related comments on pion potential are corrected in v3.)

References in corpus (7)

• Cold uniform matter and neutron stars in the quark-mesons-coupling model
• Neutrino signals from the formation of black hole: a probe of equation of state of dense matter
• Semiclassical Distorted Wave Model Analysis of the $({\pi }^{-},K^{+})$ $\Sigma$ Formation Inclusive Spectrum
• Chiral dynamics of $\Sigma$-hyperons in the nuclear medium
• A chiral symmetric relativistic mean field model with logarithmic sigma potential
• Analysis of (pi^{+-},K^+) and (K^-,K^+) hypernuclear production spectra in distorted wave impulse approximation
• Hypernuclei and nuclear matter in a chiral SU(3) RMF model

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