.png){kind=logo}
Stock image for illustration purposes only - book cover, edition or condition may vary.
Computational Methods for Astrophysical Fluid Flow
Leveque, Randall J.; Mihalas, Dimitri; Dorfi, E.A.; Muller, Ewald
€ 131.63
FREE Delivery in Ireland
Description for Computational Methods for Astrophysical Fluid Flow
Hardcover. An examination of modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications. Emphasis is placed on high-resolution shock-capturing finite-volume schemes based on Riemann solvers, and radiation hydrodynamics and applications are explored. Editor(s): Steiner, Oskar; Gautschy, A. Series: Saas-Fee Advanced Course. Num Pages: 510 pages, 212 black & white illustrations, 6 colour illustrations, 2 black & white tables, biograph. BIC Classification: PDE; PHDF; PHVB. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 241 x 162 x 40. Weight in Grams: 1024.
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.
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.
Product Details
Format
Hardback
Publication date
1998
Publisher
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Germany
Number of pages
522
Condition
New
Series
Saas-Fee Advanced Course
Number of Pages
510
Place of Publication
Berlin, Germany
ISBN
9783540644484
SKU
V9783540644484
Shipping Time
Usually ships in 15 to 20 working days
Ref
99-15
Reviews for Computational Methods for Astrophysical Fluid Flow
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