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A successful 3D core-collapse supernova explosion model
David Vartanyan
,
Adam S. Burrows
, David Radice
, M. Aaron Skinner
, Joshua Dolence
Astrophysical Sciences
Princeton Institute for Computational Science and Engineering
Research output
:
Contribution to journal
›
Article
›
peer-review
159
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Keyphrases
Supernovae
100%
Supernova Explosion
100%
Ejecta
100%
Core-collapse Supernovae
100%
Explode
100%
Mass Density
50%
Radiation Hydrodynamics Simulation
50%
Shock
50%
Three-dimensional (3D)
50%
Spatial Distribution
50%
Plume
50%
Wasp
50%
Large-scale Structure
50%
Patchy
50%
Velocity-dependent
50%
Advection
50%
Neutrino-nucleus Scattering
50%
Scattering Rate
50%
Initial Peak
50%
Gravitational Redshift
50%
Multigroup
50%
Solid Angle
50%
General Relativity
50%
Inelastic Scattering
50%
Nucleosynthesis
50%
Wide-angle
50%
Explosion Energy
50%
Non-rotating
50%
Annular Region
50%
R-process
50%
Gravitational Mass
50%
Ejecta Mass
50%
Many-body Interactions
50%
Terminal Dynamics
50%
Proton Rich
50%
Initial Perturbation
50%
Proto-neutron Star
50%
Debris Field
50%
Physics
Core-Collapse Supernovae
100%
Ejecta
100%
Supernovae
66%
Nucleon
33%
Advection
33%
Nuclear Fusion
33%
Neutron Stars
33%
General Relativity
33%
Inelastic Scattering
33%
Spatial Distribution
33%
Hydrodynamics
33%