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E. A. Dorfi, Randall J. LeVeque, Dimitri Mihalas, Ewald Müller
Saas-Fee Advanced Course 27, Lecture Notes
Computational Methods for Astrophysical Fluid Flow

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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

Scientists, graduate students

Springer Berlin, 1998, 508 S.
42,75 Euro
ISBN: 978-3-540-64448-4

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