Journal
COMPUTER PHYSICS COMMUNICATIONS
Volume 182, Issue 1, Pages 254-256Publisher
ELSEVIER SCIENCE BV
DOI: 10.1016/j.cpc.2010.06.032
Keywords
Stellar evolution; Massive star; Pair-instability supernovae
Funding
- DOE [DOE-FC02-01ER41176, DOE-FC02-06ER41438, DE-FC02-09ER41618]
- US Department of Energy [DE-FG02-87ER40328]
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We present preliminary results from multidimensional numerical studies of pair-instability supernova (PSN) studying the fluid instabilities that occur in multiple spatial dimensions We use the new radiation-hydrodynamics code CASTRO and introduce a new mapping procedure that defines the initial conditions for the multidimensional runs in such a way that conservation of physical quantities is guaranteed at any level of resolution (C) 2010 Elsevier B V All rights reserved
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