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358:, the other two books neglect global analysis and cover in great detail perturbations. He believed Hawking and Ellis did a great job summarizing recent developments in the field (as of 1974) and that the intended audience is a doctoral student (or higher) with a strong mathematical background and prior exposure to general relativity. He argued that the core of the books consists of two chapters, Chapter 4 on the significance of spacetime curvature and Chapter 6 on causal structure, and that the most interesting application is the penultimate chapter on black holes. He noted that mathematical arguments are at times difficult to follow and suggested
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their physical meaning are explored. In particular, Hawking and Ellis show that singularities and black holes arise in a large class of plausible solutions. He warned that although this book is self-contained, it is more suitable for specialists rather than new students as it is heavy-going and contains no exercises. He noted that despite the authors' attempt at a rigorous treatment, certain technical terms, such as Lie groups, are used but never explained, and that modern coordinate-free methods are introduced, but not used effectively.
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at the
University of Oxford considered this book to be an authoritative treatise that could become a classic. He observed that the authors begin with axioms of geometry and physics then derive the consequences in a rigorous fashion. Various well-known exact solutions to Einstein's field equations and
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of
Princeton University recommended this book to anyone interested in the implications of general relativity for cosmology, the singularity theorems, and the physics of black holes, presented in an almost Euclidean fashion, though he acknowledged that this is not a textbook due to its lack of
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for reference. He also noticed a small number of errors, though none affect the general conclusions drawn by the authors. He thought that this book is a "model" presentation on the interplay between mathematics and physics that could become highly influential in the future.
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by
Charles Misner, Kip Thorne, and John Archibald Wheeler. He believed these three books can supplement each other and lead students to the forefront of research. Whereas Hawking and Ellis employ global analysis extensively but say relatively little about
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In the mid-1970s, advances in the technologies of astronomical observations – radio, infrared, and X-ray astronomy – opened up the
Universe of exploration. New tools became necessary. In this book, Hawking and Ellis attempt to establish the
190:. Whereas the tools for studying Euclidean geometry were a straightedge and a compass, those needed to investigate curved spacetime are test particles and light rays. According to the mathematical physicist
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The book, now considered a classic, has also appeared in paperback format and has been reprinted many times. A fiftieth anniversary edition was published by
Cambridge University Press in February 2023.
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Wheeler, John A. (March–April 1975). "The Large Scale
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The Future of
Theoretical Physics and Cosmology: Celebrating Stephen Hawking's Contributions to Physics
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was "the first book to provide a detailed description of the revolutionary
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Sachs, Rainer (April 1974). "The Large Scale
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Woodhouse, Nicholas (1974). "The Large Scale
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Gibbons, G. W.; Shellard, E. P. S.; Rankin, S. J. (23 October 2003).
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examples and exercises. He praised its 62 illustrative diagrams.
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557:. Department of Physics, University of California, Riverside
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from the University of California, Berkeley, observed that
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introduced by Penrose and Hawking in the early seventies."
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