Published by Oxford University Press, 2008
ISBN 10: 0199205671 ISBN 13: 9780199205677
Language: English
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hardcover. Condition: Good. Connecting readers with great books since 1972! Used textbooks may not include companion materials such as access codes, etc. May have some wear or writing/highlighting. We ship orders daily and Customer Service is our top priority!
Published by Oxford University Press, 2008
ISBN 10: 0199205671 ISBN 13: 9780199205677
Language: English
Seller: GreatBookPrices, Columbia, MD, U.S.A.
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Published by Oxford University Press, 2008
ISBN 10: 0199205671 ISBN 13: 9780199205677
Language: English
Seller: Ria Christie Collections, Uxbridge, United Kingdom
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Published by Oxford University Press, 2008
ISBN 10: 0199205671 ISBN 13: 9780199205677
Language: English
Seller: GreatBookPricesUK, Woodford Green, United Kingdom
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Published by Oxford University Press, 2008
ISBN 10: 0199205671 ISBN 13: 9780199205677
Language: English
Seller: GreatBookPrices, Columbia, MD, U.S.A.
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Published by Oxford University Press, 2008
ISBN 10: 0199205671 ISBN 13: 9780199205677
Language: English
Seller: GreatBookPricesUK, Woodford Green, United Kingdom
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Add to basketHardcover. Condition: Brand New. 1st edition. 448 pages. 9.50x6.50x1.25 inches. In Stock.
Published by Oxford University Press, Oxford, 2008
ISBN 10: 0199205671 ISBN 13: 9780199205677
Language: English
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Add to basketHardcover. Condition: new. Hardcover. This book introduces the modern field of 3+1 numerical relativity. The book has been written in a way as to be as self-contained as possible, and only assumes a basic knowledge of special relativity. Starting from a brief introduction to general relativity, it discusses the different concepts and tools necessary for the fully consistent numerical simulation of relativistic astrophysical systems, with strong and dynamical gravitational fields. Among the topicsdiscussed in detail are the following: the initial data problem, hyperbolic reductions of the field equations, gauge conditions, the evolution of black hole space-times, relativistic hydrodynamics,gravitational wave extraction and numerical methods. There is also a final chapter with examples of some simple numerical space-times. The book is aimed at both graduate students and researchers in physics and astrophysics, and at those interested in relativistic astrophysics. This book is a self-contained introduction to the field of numerical relativity. Starting from basic general relativity, it introduces all the concepts and tools necessary for the fully relativistic simulation of astrophysical systems with strong and dynamical gravitational fields. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability.
Published by Oxford University Press, 2012
ISBN 10: 0199656150 ISBN 13: 9780199656158
Language: English
Seller: Toscana Books, AUSTIN, TX, U.S.A.
Paperback. Condition: new. Excellent Condition.Excels in customer satisfaction, prompt replies, and quality checks.
Published by Oxford University Press, 2008
ISBN 10: 0199205671 ISBN 13: 9780199205677
Language: English
Seller: OM Books, Sevilla, SE, Spain
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Published by Oxford University Press, 2008
ISBN 10: 0199205671 ISBN 13: 9780199205677
Language: English
Seller: PBShop.store US, Wood Dale, IL, U.S.A.
HRD. Condition: New. New Book. Shipped from UK. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000.
Published by Oxford University Press, 2008
ISBN 10: 0199205671 ISBN 13: 9780199205677
Language: English
Seller: PBShop.store UK, Fairford, GLOS, United Kingdom
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Add to basketHRD. Condition: New. New Book. Delivered from our UK warehouse in 4 to 14 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000.
Published by Oxford University Press, 2008
ISBN 10: 0199205671 ISBN 13: 9780199205677
Language: English
Seller: moluna, Greven, Germany
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Add to basketGebunden. Condition: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. This book is a self-contained introduction to the field of numerical relativity. Starting from basic general relativity, it introduces all the concepts and tools necessary for the fully relativistic simulation of astrophysical systems with strong and dynami.