Computational Methods for Astrophysical Fluid Flow

Name: Computational Methods for Astrophysical Fluid Flow
Brand: Springer-Verlag Berlin and Heidelberg GmbH & Co. KG
SKU: 9783642084126
Price: 425.21 PLN
Availability: InStock

Saas-Fee Advanced Course 27. Lecture Notes 1997 Swiss Society for Astrophysics and Astronomy

Autor: Randall J. LeVeque, Dimitri Mihalas, E.A. Dorfi, Ewald Müller

Język:

Oprawa: Miękka

Wydawca: Springer-Verlag Berlin and Heidelberg GmbH & Co. KG

Dostępność: Dostępna u dostawcy

Wysyłamy za 5-8 dni

425.21 zł

This book leads directly to the most modern numerical techniques for compressible fluid flow, with s...

Informacje o książce

Autor

Randall J. LeVeque, Dimitri Mihalas, E.A. Dorfi, Ewald Müller

Język

Angielski

Oprawa

Książka - Miękka

Data wydania

2010

strony

510

EAN

9783642084126

ISBN

3642084125

Enbook ID

01653423

Wydawca

Springer-Verlag Berlin and Heidelberg GmbH & Co. KG

Waga

881

Wymiary

155 x 235 x 21

Pełny opis

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.Four lectures lead the reader from basic numerical methods for solving hyperbolic partial differential equations to the application of complex simulation codes to selected astrophysical problems. The text highlights the powerful capabilities, the use, and the pitfalls of computational astrophysics. Difficult topics pertaining to astrophysical problem solving, such as gravitation, magnetic fields, reactive flow, and relativity, are addressed. Two lectures are devoted to radiation hydrodynamics. They treat the derivation of the basic equations and numerical methods. This book will be useful to students and researchers in astrophysics and applied mathematics.

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Computational Methods for Astrophysical Fluid Flow

Saas-Fee Advanced Course 27. Lecture Notes 1997 Swiss Society for Astrophysics and Astronomy

Informacje o książce

Pełny opis

Możesz być zainteresowany

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