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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.
Published by: Springer
Publication Date: 1998-08-19
Format: Hardcover
ISBN-13: 9783540644484
DOI: 10.1007/3-540-31632-9
Dimensions: 235.0cm x155.0cm
Pages: 510.0