0000000000116392

AUTHOR

Robert Bollig

showing 1 related works from this author

Core-collapse supernova simulations in one and two dimensions: comparison of codes and approximations

2018

We present spherically symmetric (1D) and axisymmetric (2D) supernova simulations for a convection-dominated 9 Msun and a 20 Msun progenitor that develops violent activity by the standing-accretion-shock instability (SASI). We compare in detail the Aenus-Alcar code, which uses fully multidimensional two-moment neutrino transport with an M1 closure, with a ray-by-ray-plus (RbR+) version of this code and with the Prometheus-Vertex code that employs RbR+ two-moment transport with a Boltzmann closure. Besides testing consequences of ignored non-radial neutrino-flux components in the RbR+ approximation, we also discuss the influence of various transport ingredients applied or not applied in rece…

High Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsScatteringAdvectionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsStrangenessType II supernova01 natural sciencesInstabilityComputational physicsSupernovaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesRadiative transferNeutrinoAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Monthly Notices of the Royal Astronomical Society
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