Abstract
Exact analytic solutions are derived for radiation in time-dependent relativistic flows. The flows are spherically-symmetric homologous explosions or implosions of matter with a grey extinction coefficient. The solutions are suitable for testing numerical transfer codes, and this is illustrated for a fully relativistic Monte Carlo code.
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APA
Lucy, L. B. (2005). Similarity solutions for radiation in time-dependent relativistic flows. Astronomy and Astrophysics, 429(1), 31–37. https://doi.org/10.1051/0004-6361:20041890
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