Open Issues in Core-Collapse Supernovae - Progenitors and 3-DIMENSIONAL Simulations

Details Open Issues in Core-Collapse Supernovae - Progenitors and 3-DIMENSIONAL Simulations Open Issues in Core-Collapse Supernovae - Progenitors and 3-DIMENSIONAL Simulations

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005oicc.conf..136f&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

Scientific paper

Modeling core-collapse supernovae is truly a complex computational and physical problem, requiring a detailed knowledge of a wide variety of physics and the latest techniques in both transport algorithms and hydrodynamics. Just understanding the hydrodynamic flows in core-collapse requires a much more comprehensive set of tests than is usually applied to hydrodynamic codes. In this article, we discuss a number of computational tests (with both analytic and experimental solutions) that should be added to any suite of code tests checking the viability of a code to model core-collapse supernovae. We demonstrate the weaknesses and strengths of various codes on these tests.

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