2D and 3D core-collapse supernovae simulation results obtained with the CHIMERA code
Author:
Publisher
IOP Publishing
Subject
General Physics and Astronomy
Link
http://stacks.iop.org/1742-6596/180/i=1/a=012018/pdf
Reference19 articles.
1. The Hydrodynamic Behavior of Supernovae Explosions
2. Simulation of the Spherically Symmetric Stellar Core Collapse, Bounce, and Postbounce Evolution of a Star of 13 Solar Masses with Boltzmann Neutrino Transport, and Its Implications for the Supernova Mechanism
3. Probing the gravitational well: No supernova explosion in spherical symmetry with general relativistic Boltzmann neutrino transport
4. Supernova Simulations with Boltzmann Neutrino Transport: A Comparison of Methods
5. Supernova mechanisms
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1. A DG-IMEX Method for Two-moment Neutrino Transport: Nonlinear Solvers for Neutrino–Matter Coupling*;The Astrophysical Journal Supplement Series;2021-04-01
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3. A comparison of explosion energies for simulated and observed core-collapse supernovae;Monthly Notices of the Royal Astronomical Society;2019-08-22
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