Overview

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.

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9783540644484

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From the reviews <br> Gives detailed web addresses and information where such codes can be downloaded (...). In conclusion, I feel the book gives and excellent account of present-day astrophysical hydrodynamics. <br> A. Brandenburg, The Observatory, 1999

From the reviews Gives detailed web addresses and information where such codes can be downloaded (...). In conclusion, I feel the book gives and excellent account of present-day astrophysical hydrodynamics. A. Brandenburg, The Observatory, 1999

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