Effects of Different Closure Choices in Core-collapse Supernova Simulations

The two-moment method is widely used to approximate the full neutrino transport equation in core-collapse supernova (CCSN) simulations, and different closures lead to subtle differences in the simulation results. In this paper, we compare the effects of closure choices on various physical quantities...

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Main Authors: Tianshu Wang, Adam Burrows
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/aca75c
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author Tianshu Wang
Adam Burrows
author_facet Tianshu Wang
Adam Burrows
author_sort Tianshu Wang
collection DOAJ
description The two-moment method is widely used to approximate the full neutrino transport equation in core-collapse supernova (CCSN) simulations, and different closures lead to subtle differences in the simulation results. In this paper, we compare the effects of closure choices on various physical quantities in 1D and 2D time-dependent CCSN simulations with our multigroup radiation hydrodynamics code F ornax . We find that choices of the third-order closure relations influence the time-dependent simulations only slightly. Choices of the second-order closure relation have larger consequences than choices of the third-order closure, but these are still small compared to the remaining variations due to ambiguities in some physical inputs such as the nuclear equation of state. We also find that deviations in Eddington factors are not monotonically related to deviations in physical quantities, which means that simply comparing the Eddington factors does not inform one concerning which closure is better.
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spelling doaj.art-0369bb146dc34e72a644313a1f5b4bad2023-09-03T09:29:26ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-0194327810.3847/1538-4357/aca75cEffects of Different Closure Choices in Core-collapse Supernova SimulationsTianshu Wang0https://orcid.org/0000-0002-0042-9873Adam Burrows1https://orcid.org/0000-0002-3099-5024Department of Astrophysical Sciences , Princeton, NJ 08544, USA ; tianshuw@princeton.eduDepartment of Astrophysical Sciences , Princeton, NJ 08544, USA ; tianshuw@princeton.eduThe two-moment method is widely used to approximate the full neutrino transport equation in core-collapse supernova (CCSN) simulations, and different closures lead to subtle differences in the simulation results. In this paper, we compare the effects of closure choices on various physical quantities in 1D and 2D time-dependent CCSN simulations with our multigroup radiation hydrodynamics code F ornax . We find that choices of the third-order closure relations influence the time-dependent simulations only slightly. Choices of the second-order closure relation have larger consequences than choices of the third-order closure, but these are still small compared to the remaining variations due to ambiguities in some physical inputs such as the nuclear equation of state. We also find that deviations in Eddington factors are not monotonically related to deviations in physical quantities, which means that simply comparing the Eddington factors does not inform one concerning which closure is better.https://doi.org/10.3847/1538-4357/aca75cCore-collapse supernovaeRadiative transferSupernova neutrinos
spellingShingle Tianshu Wang
Adam Burrows
Effects of Different Closure Choices in Core-collapse Supernova Simulations
The Astrophysical Journal
Core-collapse supernovae
Radiative transfer
Supernova neutrinos
title Effects of Different Closure Choices in Core-collapse Supernova Simulations
title_full Effects of Different Closure Choices in Core-collapse Supernova Simulations
title_fullStr Effects of Different Closure Choices in Core-collapse Supernova Simulations
title_full_unstemmed Effects of Different Closure Choices in Core-collapse Supernova Simulations
title_short Effects of Different Closure Choices in Core-collapse Supernova Simulations
title_sort effects of different closure choices in core collapse supernova simulations
topic Core-collapse supernovae
Radiative transfer
Supernova neutrinos
url https://doi.org/10.3847/1538-4357/aca75c
work_keys_str_mv AT tianshuwang effectsofdifferentclosurechoicesincorecollapsesupernovasimulations
AT adamburrows effectsofdifferentclosurechoicesincorecollapsesupernovasimulations