{ "id": "2104.00775", "version": "v1", "published": "2021-04-01T21:43:50.000Z", "updated": "2021-04-01T21:43:50.000Z", "title": "Equation of State table with hyperon and antikaon for supernova and neutron star merger", "authors": [ "Tuhin Malik", "Sarmistha Banik", "Debades Bandyopadhyay" ], "comment": "6 figures", "journal": "The Astrophysical Journal, Volume 910, Number 2, 2021", "doi": "10.3847/1538-4357/abe860", "categories": [ "astro-ph.HE", "nucl-th" ], "abstract": "We develop a new equation of state (EoS) table involving thermal (anti)kaons, Bose-Einstein condensate of $K^{-}$ mesons and $\\Lambda$-hyperons for core-collapse supernova and neutron star merger simulations. This EoS table is based on a finite temperature density-dependent relativistic hadron field theory where baryon-baryon interaction is mediated by scalar $\\sigma$, vector $\\omega$ and $\\rho$ mesons, using the parameter set DD2 for nucleons. The repulsive hyperon-hyperon interaction is mediated by an additional strange $\\phi$ meson. The EoS for the $K^-$ condensed matter is also calculated within the framework of relativistic mean field model, whereas the low-density, inhomogeneous matter is calculated in the extended Nuclear Statistical Equilibrium model (NSE). The EoS table is generated for a wide range of values of three parameters - baryon density ($10^{-12}$ to $\\sim$ 1 fm$^{-3}$), positive charge fraction(0.01 to 0.60) and temperature(0.1 to 158.48 MeV).", "revisions": [ { "version": "v1", "updated": "2021-04-01T21:43:50.000Z" } ], "analyses": { "keywords": [ "neutron star merger", "nuclear statistical equilibrium model", "state table", "density-dependent relativistic hadron field theory", "temperature density-dependent relativistic hadron field" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }