1973
DOI: 10.1063/1.3128097
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Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity

Abstract: A leading physicist delves into relativity and experimental applications Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity offers a Nobel laureate's perspectives on the wealth of data technological developments have brought to expand upon Einstein's theory. Unique in basing relativity on the Principle of Equivalence of Gravitation and Inertia over Riemannian geometry, this book explores relativity experiments and observational cosmology to provide a sound foundation upo… Show more

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Cited by 923 publications
(907 citation statements)
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“…Let us briefly review some general properties of black holes [6,7,8,9,10]. Black holes are objects which result as end points of gravitational collapse of matter.…”
Section: Black Holes and The Information Puzzlementioning
confidence: 99%
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“…Let us briefly review some general properties of black holes [6,7,8,9,10]. Black holes are objects which result as end points of gravitational collapse of matter.…”
Section: Black Holes and The Information Puzzlementioning
confidence: 99%
“…There are many singular classical solutions of general relativity (for standard textbooks on classical general relativity, see, e.g., [6,7,8,9,10]), including the Schwarzschild black hole and the Big Bang model of cosmology. Black holes and their higher dimensional analogues (black branes) also appear as solutions of low energy string theory.…”
Section: Quantum Theory and General Relativitymentioning
confidence: 99%
“…We believe that the Universe is homogeneous and isotropic [9]. This statement implies that the space-time can be parametrized by the Friedmann-Lemaître-Robertson-Walker (FLRW) metric which, inserted into the Einstein equations yield the Friedmann equations [9].…”
Section: Introductionmentioning
confidence: 99%
“…This statement implies that the space-time can be parametrized by the Friedmann-Lemaître-Robertson-Walker (FLRW) metric which, inserted into the Einstein equations yield the Friedmann equations [9]. From these latter we can derive the following time evolution equation [2,3,11]:…”
Section: Introductionmentioning
confidence: 99%
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