arXiv · 1401.1653
Equation of state of hypernuclear matter: tuning hyperon--scalar-meson couplings
Abstract
We discuss to which extent the modifications of the hyperon--scalar-meson coupling constants affect the equation of state (EoS) hypernuclear matter. The study is carried out within a relativistic density functional theory. The nucleonic matter is described in terms of a density-dependent parametrization of nucleon-meson couplings, whereas the hyperon--meson couplings are deduced from the octet model. We identify the parameter space of hyperon-meson couplings for which massive stellar configurations with $M\le 2.25 M_{\odot}$ exist. We also discuss the EoS at finite temperatures with and without of a trapped neutrino component and show that neutrinos stiffen the EoS and change qualitatively the composition of stellar matter.
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Giuseppe Colucci, Armen Sedrakian. 2014-01-08. Equation of state of hypernuclear matter: tuning hyperon--scalar-meson couplings. https://doi.org/10.1088/1742-6596/496/1/012003
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