Influence of the nuclear symmetry energy slope on observables of compact stars with -admixed hypernuclear matter
arXiv:2112.12629 · doi:10.1103/PhysRevC.105.015802
Abstract
In this work, we study the effects of nuclear symmetry energy slope on neutron star dense matter equation of state and its impact on neutron star observables (mass-radius, tidal response). We construct the equation of state within the framework of covariant density functional theory implementing coupling schemes of non-linear and density-dependent models with viability of heavier non-nucleonic degrees of freedom. The slope of symmetry energy parameter () is adjusted following density-dependence of isovector meson coupling to baryons. We find that smaller values of at saturation favour early appearance of -resonances in comparison to hyperons leading to latter's threshold at higher matter densities. We also investigate the dependence of on tidal deformability and compactness parameter of a neutron star for different equation of states and observe similar converging behaviour for larger values.
14 pages, 10 figures, 8 tables; corrected some typos; matches with published version
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