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Monte Carlo Radiative Transfer Simulations: Applications to Astrophysical Outflows and Explosionsтезисы доклада
Информация о цитировании статьи получена из
Web of Science
Дата последнего поиска статьи во внешних источниках: 29 мая 2015 г.
- Авторы: Sim S.A., Kromer M., Röpke F.K., Sorokina E.I., Blinnikov S.I., Kasen D., Hillebrandt W.
- Сборник: Numerical Modeling of Space Plasma Flows, Astronum-2009
- Серия: Astronomical Society of the Pacific Conference Series
- Том: 429
- Тезисы
- Год издания: 2010
- Место издания: San Francisco
- Первая страница: 148
- Последняя страница: 153
- Аннотация: The theory of radiative transfer provides the link between the physical conditions in an astrophysical object and the observable radiation which it emits. Thus accurately modelling radiative transfer is often a necessary part of testing theoretical models by comparison with observations. We describe a new radiative transfer code which employs Monte Carlo methods for the numerical simulation of radiation transport in expanding media. We discuss the application of this code to the calculation of synthetic spectra and light curves for a Type Ia supernova explosion model and describe the sensitivity of the results to certain approximations made in the simulations.
- Добавил в систему: Сорокина Елена Ильинична