Energy loss through optically thin radiative cooling plays an important part in the evolution of astrophysical gas dynamics and should therefore be considered a necessary element in any numerical simulation. Although the addition of this physical process to the equations of hydrodynamics is straight
β¦ LIBER β¦
Computational relativistic astrophysics with adaptive mesh refinement: Testbeds
β Scribed by Evans, Edwin; Iyer, Sai; Schnetter, Erik; Suen, Wai-Mo; Tao, Jian; Wolfmeyer, Randy; Zhang, Hui-Min
- Book ID
- 126463756
- Publisher
- The American Physical Society
- Year
- 2005
- Tongue
- English
- Weight
- 273 KB
- Volume
- 71
- Category
- Article
- ISSN
- 1550-7998
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