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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.
Table of Contents
- Nonlinear Conservation Laws and Finite Volume Methods
- Radition Hydrodynamics
- Radiation Hydrodynamics: Numerical Aspects and Applications
- Simulation of Astrophysical Fluid Flow
Readership:
Scientists, graduate students
Springer Berlin, 1998, 508 S.
42,75 Euro
Hardcover
ISBN: 978-3-540-64448-4
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