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Titlebook: Global Structure and Evolution in General Relativity; Proceedings of the F Spiros Cotsakis,Gary W. Gibbons Conference proceedings 1996 Spri

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書目名稱Global Structure and Evolution in General Relativity
副標(biāo)題Proceedings of the F
編輯Spiros Cotsakis,Gary W. Gibbons
視頻videohttp://file.papertrans.cn/387/386610/386610.mp4
叢書名稱Lecture Notes in Physics
圖書封面Titlebook: Global Structure and Evolution in General Relativity; Proceedings of the F Spiros Cotsakis,Gary W. Gibbons Conference proceedings 1996 Spri
描述The five lectures presented in this volume address very timely mathematical problems in relativity and cosmology. .Part I. is devoted to the initial value and evolution problems of the Einstein equations. Especially it deals with the Einstein-Yang-Mills-Boltzmann system, fluid models with finite or infinite conductivity, global evolution of a new (two-phase) model for gravitational collapse and the structure of maximal, asymptotically flat, vacuum solutions of the constraint equations which have the additional property of containing trapped surfaces. .Part II. focuses on geometrical-topological problems in relativity and cosmology: on the role of cosmic censorship for the global structure of the Einstein-Maxwell equations and on the mathematical structure of quantum conformal superspace.
出版日期Conference proceedings 1996
關(guān)鍵詞Gravitation; Gravity; black hole; cosmology; general relativity; relativity; theory of relativity
版次1
doihttps://doi.org/10.1007/BFb0103443
isbn_softcover978-3-662-14072-7
isbn_ebook978-3-540-49361-7Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer-Verlag Berlin Heidelberg 1996
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The structure of quantum conformal superspace,is motivated by questions involving reduction of the canonical Hamiltonian formulation of general relativity to a non-degenerate Hamiltonian formulation, and to questions involving both linearization stability and quantization of the gravitational field. We show that if the degree of symmetry of . i
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Einleitung Forschungsziel und Methoden,s and a hard phase corresponding to matter at supranuclear densities. The model contains a rich variety of features, such as interfaces across which the entropy jumps, stable static solutions corresponding to neutron stars, as well as black holes and singularities. We study the global dynamics of th
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https://doi.org/10.1007/978-3-322-97195-1is motivated by questions involving reduction of the canonical Hamiltonian formulation of general relativity to a non-degenerate Hamiltonian formulation, and to questions involving both linearization stability and quantization of the gravitational field. We show that if the degree of symmetry of . i
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Relativistic fluids and gravitational collapse,he entropy jumps, stable static solutions corresponding to neutron stars, as well as black holes and singularities. We study the global dynamics of this model in the spherically symmetric case, in the hope of providing insight into the dynamics of real astrophysical situations.
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0075-8450 topological problems in relativity and cosmology: on the role of cosmic censorship for the global structure of the Einstein-Maxwell equations and on the mathematical structure of quantum conformal superspace.978-3-662-14072-7978-3-540-49361-7Series ISSN 0075-8450 Series E-ISSN 1616-6361
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