الوصف
This book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications. Emphasis is put on high-resolution shock-capturing finite-volume schemes based on Riemann solvers. The applications of such schemes, in particular the PPM method, are given and include large-scale simulations of supernova explosions by core collapse and thermonuclear burning and astrophysical jets. Parts two and three treat radiation hydrodynamics. The power of adaptive (moving) grids is demonstrated with a number of stellar-physical simulations showing very crispy shock-front structures.
تفاصيل الكتاب
تنسيق
غلاف ورقي
صفحات
524 صفحات
لغة
الإنجليزية
منشور
ديسمبر 15, 2010
الناشر
Springer
رقم ISBN-10
3642084125
رقم ISBN-13
9783642084126