Simulations of multigroup relativistic radiative transfer for shock waves in supernovae

Details Simulations of multigroup relativistic radiative transfer for shock waves in supernovae Simulations of multigroup relativistic radiative transfer for shock waves in supernovae

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010astl...36..109t&link_type=abstract

Astronomy Letters, Volume 36, Issue 2, pp.109-115

Astronomy and Astrophysics

Astronomy

5

Supernovae, Radiative Transfer

Scientific paper

The results of numerical simulations of light curves and spectra and the influence of special relativity effects at the epoch of supernova shock breakout are considered. The algorithm of the RADA code used in the simulations is described. Prospects for using the numerical simulation results to analyze and interpret available and future data from the SWIFT and LOBSTER space observatories are discussed.

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