Multigroup radiative transfer in supernova shock breakout modelsстатья
Информация о цитировании статьи получена из
Web of Science,
Scopus
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 18 июля 2013 г.
Аннотация: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.