Effect of the Nuclear Equation of State on Relativistic Turbulence-induced Core-collapse Supernovae

Boccioli, Luca; Mathews, Grant J.; Suh, In-Saeng; O’Connor, Evan P.

doi:10.3847/1538-4357/ac4603

Title: Effect of the Nuclear Equation of State on Relativistic Turbulence-induced Core-collapse Supernovae

Journal Article · 20 February 2022 · The Astrophysical Journal

DOI: https://doi.org/10.3847/1538-4357/ac4603 · OSTI ID:1845939

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Abstract The nuclear equation of state (EOS) is an important component in the evolution of core-collapse supernovae. In this paper we make a survey of various EOSs in the literature and analyze their effect on spherical core-collapse models in which the effects of three-dimensional turbulence is modeled by a general relativistic formulation of Supernova Turbulence In Reduced-dimensionality (STIR). We show that the viability of the explosion is quite EOS dependent and that it best correlates with the early-time interior entropy density of the proto–neutron star. We check that this result is not progenitor dependent, although the lowest-mass progenitors show different explosion properties, due to the different pre-collapse nuclear composition. Larger central entropies also induce more vigorous proto–neutron star convection in our one-dimensional turbulence model, as well as a wider convective layer.

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Research Organization:: University of Notre Dame, IN (United States)

Sponsoring Organization:: USDOE; USDOE Office of Science (SC)

Grant/Contract Number:: FG02-95ER40934

OSTI ID:: 1845939

Journal Information:: The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 2 Vol. 926; ISSN 0004-637X

Publisher:: American Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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Title: Effect of the Nuclear Equation of State on Relativistic Turbulence-induced Core-collapse Supernovae

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