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Titlebook: Quantum Cosmology; A Fundamental Descri Martin Bojowald Book 2011 Springer Science+Business Media, LLC 2011 big bang physics.bouncing cosmo

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發(fā)表于 2025-3-21 16:31:33 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Quantum Cosmology
副標(biāo)題A Fundamental Descri
編輯Martin Bojowald
視頻videohttp://file.papertrans.cn/782/781125/781125.mp4
概述Bridges the gap between quantum gravity research and cosmology.Discusses concepts and philosophical implications of the universe before the big bang.The author is credited for establishing loop quantu
叢書名稱Lecture Notes in Physics
圖書封面Titlebook: Quantum Cosmology; A Fundamental Descri Martin Bojowald Book 2011 Springer Science+Business Media, LLC 2011 big bang physics.bouncing cosmo
描述.Consequences of quantum gravity on grander scales are expected to be enormous: only such a theory can show how black holes really behave and where our universe came from. Applications of loop quantum gravity to cosmology have especially by now shed much light on cosmic evolution of a universe in a fundamental, microscopic description. Modern techniques are explained in this book which demonstrate how the universe could have come from a non-singular phase before the big bang, how equations for the evolution of structure can be derived, but also what fundamental limitations remain to our knowledge of the universe before the big bang..The following topics will be covered in this book:.Hamiltonian cosmology: a general basic treatment of isotropy, perturbations and their role for observations; useful in general cosmology..Effective equations: an efficient way to evaluate equations of quantum gravity, which is also useful in other areas of physics where quantum theory is involved..Loop quantization: a new formalism for the atomic picture of space-time; usually presented at a sophisticated mathematical level, but evaluated here from an intuitive physical side..The book will start with ph
出版日期Book 2011
關(guān)鍵詞big bang physics; bouncing cosmologies; difference equations; early universe cosmology; effective equati
版次1
doihttps://doi.org/10.1007/978-1-4419-8276-6
isbn_softcover978-1-4614-3017-9
isbn_ebook978-1-4419-8276-6Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer Science+Business Media, LLC 2011
The information of publication is updating

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Dynamics: Changing Atoms of Space–Timeels. Now, these spatial structures have to fit into a consistent quantum space–time which in a certain sense reduces to a solution of Einstein’s equation in a semiclassical or low-curvature limit. Only completing this most challenging step will make the theory one of quantum gravity, rather than of spatial quantum geometry.
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Midisuperspace Models: Black Hole Collapselest inhomogenous model is that of spherical symmetry, which provides interesting ways to test the formalism as well as applications in the context of black holes. In the vacuum case the model has a finite number of dynamical degrees of freedom, but the infinitely many kinematical ones already allow one to test field theoretic aspects.
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Quantum Cosmology978-1-4419-8276-6Series ISSN 0075-8450 Series E-ISSN 1616-6361
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Harmonic Cosmology: The Universe Before the Big Bang and How Much We Can Know About ItTo understand the strong quantum phase that is expected to be realized in a small and highly curved universe around the big bang,big bang we return to the solvable modelsolvable model of loop quantum cosmology developed in ..
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