General Relativistic Neutrino-driven Turbulence in One-dimensional Core-collapse Supernovae

Boccioli, Luca; Mathews, Grant J.; O’Connor, Evan P.

doi:10.3847/1538-4357/abe767

Title: General Relativistic Neutrino-driven Turbulence in One-dimensional Core-collapse Supernovae

Journal Article · Fri Apr 30 00:00:00 EDT 2021 · The Astrophysical Journal

DOI:https://doi.org/10.3847/1538-4357/abe767· OSTI ID:1835322

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Convection and turbulence in core-collapse supernovae (CCSNe) are inherently three-dimensional (3D) in nature. However, 3D simulations of CCSNe are computationally demanding. Thus, it is valuable to modify simulations in spherical symmetry to incorporate 3D effects using some parametric model. In this paper, we report on the formulation and implementation of general relativistic neutrino-driven turbulent convection in the spherically symmetric core-collapse supernova codeGR1D. This is based upon the recently proposed method of Simulated Turbulence in Reduced Dimensionality (STIR) in Newtonian simulations from Couch et al. (2020). When the parameters of this model are calibrated to 3D simulations, we find that our general relativistic formulation of STIR requires larger turbulent eddies to achieve a shock evolution similar to the original STIR model. We also find that general relativity may alter the correspondence between progenitor mass and successful versus failed explosions.

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

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: FG02-95-ER40934; FG02-95ER40934

OSTI ID:: 1835322

Alternate ID(s):: OSTI ID: 1850100

Journal Information:: The Astrophysical Journal, Journal Name: The Astrophysical Journal Vol. 912 Journal Issue: 1; ISSN 0004-637X

Publisher:: American Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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