Multigroup radiative transfer in supernova shock breakout models

Details Multigroup radiative transfer in supernova shock breakout models Multigroup radiative transfer in supernova shock breakout models

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011astl...37..194b&link_type=abstract

Astronomy Letters, Volume 37, Issue 3, pp.194-209

Astronomy and Astrophysics

Astronomy

Supernovae, Shock Waves, X-Ray Transients

Scientific paper

The physical peculiarities of supernova shock breakout are discussed. A number of models for various types of supernovae have been constructed based on multigroup radiative transfer by taking these peculiarities into account. The results of numerical simulations and the influence of the effects of photon scattering by electrons and the thermalization depth on them are considered. It is shown under which conditions the appearance of hard X-ray emission is possible at shock breakout. It is pointed out what refinements are necessary in the computational algorithms for radiative transfer and hydrodynamics.

Affiliated with

Also associated with

No associations

Rating

Multigroup radiative transfer in supernova shock breakout models does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Multigroup radiative transfer in supernova shock breakout models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multigroup radiative transfer in supernova shock breakout models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-861102