Monte Carlo Simulations of Radiative and Neutrino Transport under Astrophysical Conditions


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Аннотация

Monte Carlo simulations are utilized to model radiative and neutrino transfer in astrophysics. An algorithm that can be used to study radiative transport in astrophysical plasma based on simulations of photon trajectories in a medium is described. Formation of the hard X-ray spectrum of the Galactic microquasar SS 433 is considered in detail as an example. Specific requirements for applying such simulations to neutrino transport in a densemedium and algorithmic differences compared to its application to photon transport are discussed.

Авторлар туралы

Yu. Krivosheyev

Space Research Institute

Хат алмасуға жауапты Автор.
Email: krivosheev@iki.rssi.ru
Ресей, Moscow, 117997

G. Bisnovatyi-Kogan

Space Research Institute; Moscow Engineering and Physics Institute

Email: krivosheev@iki.rssi.ru
Ресей, Moscow, 117997; Moscow, 115409

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