3D Simulations of Core-Collapse SNe

Details 3D Simulations of Core-Collapse SNe 3D Simulations of Core-Collapse SNe

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1294..266j&link_type=abstract

THE FIRST STARS AND GALAXIES: CHALLENGES FOR THE NEXT DECADE. AIP Conference Proceedings, Volume 1294, pp. 266-267 (2010).

Physics

Supernovae, Hydrodynamics, Nucleosynthesis, Supernovae, Hydrodynamics, Origin, Formation, And Abundances Of The Elements

Scientific paper

Simulations of Rayleigh-Taylor (RT) induced mixing in spherically
symmetric core-collapse supernova (SN) explosions are performed in both
2D and 3D. When the only intial perturbation is that arising from the
grid, the final state of the 2D and 3D simulations are essentially the
same for a variety of presupernova progenitor models.

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