3D-Simulations of Type Ia Supernovae

Details 3D-Simulations of Type Ia Supernovae 3D-Simulations of Type Ia Supernovae

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.552..115h&link_type=abstract

Proceedings of the 5th INTEGRAL Workshop on the INTEGRAL Universe (ESA SP-552). 16-20 February 2004, Munich, Germany. Scientific

Physics

Scientific paper

A 3D Monte Carlo code has been built to simulate the gamma ray emissions during Type Ia supernova explosions in order to properly take into account departures from symmetry. A 3D Delayed Detonation (DDT) model has been used as input for the simulation results presented further ahead. Two calculations of gamma ray emission were carried out: one taking into account the whole structure of the DDT model, and the second one carving out a conical hole from the sphere, where its density is almost negligible. The hole represents the expected location of the secondary star. Key words: supernovae; gamma rays; 3D conical hole; radiation transfer.

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