New open-source approaches to the modeling of stellar collapse and the formation of black holes

Details New open-source approaches to the modeling of stellar collapse and the formation of black holes New open-source approaches to the modeling of stellar collapse and the formation of black holes

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ap%26ss.336..151o&link_type=abstract

Astrophysics and Space Science, Volume 336, Issue 1, pp.151-156

Astronomy and Astrophysics

Astrophysics

Stellar Collapse, Black Holes, Supernovae

Scientific paper

We present new approaches to the simulation of stellar collapse, the formation of black holes, and explosive core-collapse supernova nucleosynthesis that build upon open-source codes and microphysics. We discuss the new spherically-symmetric general-relativistic (GR) collapse code GR1D that is endowed with an approximate 1.5D treatment of rotation, comes with multiple nuclear equations of state, and handles neutrinos with a multi-species leakage scheme. Results from a first set of spinning black hole formation simulations are presented. We go on to discuss the derivative code GR1D+ N which is tuned for calculations of explosive nucleosynthesis and includes a NSE/non-NSE equation of state treatment, and a nuclear reaction network. We present sample results showing GR1D+ N's performance in reproducing previous results with thermal-bomb-driven explosions. Finally, we introduce the 3 + 1 GR Zelmani core collapse simulation package and present first results obtained in its application to the 3D modeling of failing core-collapse supernovae.

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