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Titlebook: General Relativity and Relativistic Astrophysics; Norbert Straumann Textbook 19881st edition Springer-Verlag Berlin Heidelberg 1988 Accret

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书目名称General Relativity and Relativistic Astrophysics
编辑Norbert Straumann
视频video
丛书名称Theoretical and Mathematical Physics
图书封面Titlebook: General Relativity and Relativistic Astrophysics;  Norbert Straumann Textbook 19881st edition Springer-Verlag Berlin Heidelberg 1988 Accret
描述In 1979 I gave graduate courses at the University of Zurich and lectured in the ‘Troisieme Cycle de la Suisse Romande‘ (a consortium offour uni­ versities in the french-speaking part of Switzerland), and these lectures were the basis of the ‘Springer Lecture Notes in Physics‘, Volume 150, published in 1981. This text appeared in German, because there have been few modern expositions of the general theory of relativity in the mother tongue of its only begetter. Soon after the book appeared, W. Thirring asked me to prepare an English edition for the ‘Texts and Mono­ graphs in Physics‘. Fortunately E. Borie agreed to translate the original German text into English. An excellent collaboration allowed me to re­ vise and add to the contents of the book. I have updated and improved the original text and have added a number of new sections, mostly on astrophysical topics. In particular, in collaboration with M. Camenzind I have included a chapter on spherical and disk accretion onto compact objects. This book divides into three parts. Part I develops the mathematical tools used in the general theory of relativity. Since I wanted to keep this part short, but reasonably self-contained, I hav
出版日期Textbook 19881st edition
关键词Accretion; Astrophysik; Differentialgeometrie; Relativity; Relativitätstheorie; astrophysics; general rela
版次1
doihttps://doi.org/10.1007/978-3-642-84439-3
isbn_ebook978-3-642-84439-3Series ISSN 1864-5879 Series E-ISSN 1864-5887
issn_series 1864-5879
copyrightSpringer-Verlag Berlin Heidelberg 1988
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https://doi.org/10.1007/978-94-011-0327-5rong x-ray sources. For an understanding of sources like CygX-1, it is important to construct models for the flow of gas onto a black hole and the properties of the radiation which is produced in this process.
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The Post-Newtonian Approximation system but also for more exotic objects like the binary pulsar PSR 1913 + 16. In such situations, it suffices to study the effects predicted by general relativity in a consistent post-Newtonian approximation, i.e. at a level of approximation in which gravitational radiation plays no rôle.
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