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Titlebook: Einstein’s Field Equations and Their Physical Implications; Selected Essays in H Bernd G. Schmidt Conference proceedings 2000 Springer-Verl

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0075-8450 structure of Einstein‘s field equations and they show how to extract their physical content from them by mathematically exact methods. The essays are devoted to exact solutions and to the Cauchy problem of the field equations as well as to post-Newtonian approximations that have direct physical imp
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https://doi.org/10.1007/978-1-4684-5631-8ndependent degrees of freedom”. Very loosely speaking, the spacetime geometry should be uniquely determined by the matter content of the model under consideration. In a similar way, for a given matter model (such as that of a perfect fluid), there should be a one-to-one correspondence between Newtonian solutions and general relativistic ones.
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Post-Newtonian Gravitational Radiation,hen there are no symmetry in the problem (as is the case in the problem of the gravitational dynamics of separated bodies). Therefore, one is often obliged, in general relativity, to resort to approximation methods.
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0075-8450 lications. Further topics concern quantum gravity and optics in gravitational fields..The book addresses researchers in relativity and differential geometry but can also be used as additional reading material for graduate students.    .978-3-642-08637-3978-3-540-46580-5Series ISSN 0075-8450 Series E-ISSN 1616-6361
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The Cauchy Problem for the Einstein Equations,quations which are hyperbolic is examined in detail and some new results on that subject are presented. Relevant background from the theory of partial differential equations is also explained at some length.
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Conference proceedings 2000hy problem of the field equations as well as to post-Newtonian approximations that have direct physical implications. Further topics concern quantum gravity and optics in gravitational fields..The book addresses researchers in relativity and differential geometry but can also be used as additional reading material for graduate students.    .
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https://doi.org/10.1007/978-3-531-90489-4hen there are no symmetry in the problem (as is the case in the problem of the gravitational dynamics of separated bodies). Therefore, one is often obliged, in general relativity, to resort to approximation methods.
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