Kód: 04333684
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 ... celý popis
Angličtina
Nákupem získáte 236 bodů
Anotace knihy
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. TOC:Nonlinear Conservation Laws and Finite Volume Methods.- Radition Hydrodynamics.- Radiation Hydrodynamics: Numerical Aspects and Applications.- Simulation of Astrophysical Fluid Flow.
Parametry knihy
Zařazení knihy Knihy v angličtině Mathematics & science Physics Classical mechanics
2357 Kč
Angličtina
Osobní odběr Praha, Brno a 46795 dalších
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