Numerical simulations of core-collapse supernovae imposing steady shock approximation

Details Numerical simulations of core-collapse supernovae imposing steady shock approximation Numerical simulations of core-collapse supernovae imposing steady shock approximation

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jphcs..31..155w&link_type=abstract

Journal of Physics: Conference Series, Volume 31, Issue 1, pp. 155-156 (2006).

Physics

Scientific paper

We carried out one-dinensional long-term numerical simulations of core-collapse supernovae imposing steady shock approximation. As a result of a computation, we found core does not explode and shock wave stalls within several hundreds milliseconds from bounce. However, we execute long-term numerical simulation until 3.5 seconds from bounce with short CPU time using Personal Computer.

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