Capturing Stellar Core Hydrodynamic Instabilities in Core-Collapse Supernovae

Details Capturing Stellar Core Hydrodynamic Instabilities in Core-Collapse Supernovae Capturing Stellar Core Hydrodynamic Instabilities in Core-Collapse Supernovae

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005oicc.conf..123b&link_type=abstract

OPEN ISSUES IN CORE COLLAPSE SUPERNOVA THEORY . Held 22-24 June 2004 in National Institute for Nuclear Theory, University of Was

Physics

Nuclear Physics

Nuclear Theory

1

Scientific paper

Current efforts to model the multidimensional dynamics of core-collapse supernovae show effects of strong turbulence during the post-bounce phase. This motion may be seeded by convection driven by neutrino heating below the accretion shock, but this shock itself is capable of generating such turbulence through the spherical accretion shock instability (SASI). Here we review recent studies of the SASI and discuss its role in core-collapse supernovae.

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