Inhomogeneous cosmological models:
This volume provides a comprehensive survey of our understanding of the universe based on the exact solutions of the theory of relativity. More precisely, it describes those models that fit with astronomical observations of galaxy clusters, cosmic voids and other key features of our universe. This a...
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| Main Author: | |
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| Format: | Electronic eBook |
| Language: | English |
| Published: |
Cambridge
Cambridge University Press
1997
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| Subjects: | |
| Online Access: | BSB01 FHN01 Volltext |
| Summary: | This volume provides a comprehensive survey of our understanding of the universe based on the exact solutions of the theory of relativity. More precisely, it describes those models that fit with astronomical observations of galaxy clusters, cosmic voids and other key features of our universe. This authoritative account achieves two important goals. First, it collects together all independently derived cosmological solutions since the birth of relativity in 1915 to 1997, and clearly shows how they are interrelated. Secondly, it presents a coherent overview of the physical properties of these inhomogeneous models. It demonstrates, for instance, that the formation of voids and the interaction of the cosmic microwave background radiation with matter in the universe can be explained by exact solutions of the Einstein equations, without the need for approximations. This book will be of particular interest to graduates and researchers in gravity, relativity and theoretical cosmology as well as historians of science |
| Item Description: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
| Physical Description: | 1 online resource (xvi, 317 pages) |
| ISBN: | 9780511721694 |
| DOI: | 10.1017/CBO9780511721694 |
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| contents | 1. Preliminaries -- 2. The Szekeres-Szafron family of solutions -- 3. Physics and cosmology in an inhomogeneous Universe -- 4. The Stephani-Barnes family of solutions -- 5. Solution with null radiation -- 6. Solutions with a "stiff fluid"/scalar field source -- 7. Other solutions -- 8. Averaging out inhomogeneities of geometry and matter in cosmological models -- 9. Comments -- App. A. Dictionary of abbreviations used in the text and in the diagrams -- App. B. Why should one consider inhomogeneous models of the Universe? -- App. C. Memorable statements about the cosmological principle -- App. D. How was this review compiled? -- App. E. Historical milestones |
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| dewey-full | 523.1/01/5118 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.1/01/5118 |
| dewey-search | 523.1/01/5118 |
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| discipline | Physik |
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| id | DE-604.BV043945762 |
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| indexdate | 2024-07-10T07:39:24Z |
| institution | BVB |
| isbn | 9780511721694 |
| language | English |
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| spelling | Krasiński, Andrzej Verfasser aut Inhomogeneous cosmological models Andrzej Krasiński Cambridge Cambridge University Press 1997 1 online resource (xvi, 317 pages) txt rdacontent c rdamedia cr rdacarrier Title from publisher's bibliographic system (viewed on 05 Oct 2015) 1. Preliminaries -- 2. The Szekeres-Szafron family of solutions -- 3. Physics and cosmology in an inhomogeneous Universe -- 4. The Stephani-Barnes family of solutions -- 5. Solution with null radiation -- 6. Solutions with a "stiff fluid"/scalar field source -- 7. Other solutions -- 8. Averaging out inhomogeneities of geometry and matter in cosmological models -- 9. Comments -- App. A. Dictionary of abbreviations used in the text and in the diagrams -- App. B. Why should one consider inhomogeneous models of the Universe? -- App. C. Memorable statements about the cosmological principle -- App. D. How was this review compiled? -- App. E. Historical milestones This volume provides a comprehensive survey of our understanding of the universe based on the exact solutions of the theory of relativity. More precisely, it describes those models that fit with astronomical observations of galaxy clusters, cosmic voids and other key features of our universe. This authoritative account achieves two important goals. First, it collects together all independently derived cosmological solutions since the birth of relativity in 1915 to 1997, and clearly shows how they are interrelated. Secondly, it presents a coherent overview of the physical properties of these inhomogeneous models. It demonstrates, for instance, that the formation of voids and the interaction of the cosmic microwave background radiation with matter in the universe can be explained by exact solutions of the Einstein equations, without the need for approximations. This book will be of particular interest to graduates and researchers in gravity, relativity and theoretical cosmology as well as historians of science Mathematisches Modell Cosmology / Mathematical models Relativity (Physics) / Mathematical models Weltall (DE-588)4079154-3 gnd rswk-swf Mathematisches Modell (DE-588)4114528-8 gnd rswk-swf Kosmologisches Modell (DE-588)4330709-7 gnd rswk-swf Inhomogenes Medium (DE-588)4228459-4 gnd rswk-swf Weltall (DE-588)4079154-3 s Mathematisches Modell (DE-588)4114528-8 s 1\p DE-604 Kosmologisches Modell (DE-588)4330709-7 s Inhomogenes Medium (DE-588)4228459-4 s 2\p DE-604 Erscheint auch als Druckausgabe 978-0-521-03017-5 Erscheint auch als Druckausgabe 978-0-521-48180-9 https://doi.org/10.1017/CBO9780511721694 Verlag URL des Erstveröffentlichers Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 2\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Krasiński, Andrzej Inhomogeneous cosmological models 1. Preliminaries -- 2. The Szekeres-Szafron family of solutions -- 3. Physics and cosmology in an inhomogeneous Universe -- 4. The Stephani-Barnes family of solutions -- 5. Solution with null radiation -- 6. Solutions with a "stiff fluid"/scalar field source -- 7. Other solutions -- 8. Averaging out inhomogeneities of geometry and matter in cosmological models -- 9. Comments -- App. A. Dictionary of abbreviations used in the text and in the diagrams -- App. B. Why should one consider inhomogeneous models of the Universe? -- App. C. Memorable statements about the cosmological principle -- App. D. How was this review compiled? -- App. E. Historical milestones Mathematisches Modell Cosmology / Mathematical models Relativity (Physics) / Mathematical models Weltall (DE-588)4079154-3 gnd Mathematisches Modell (DE-588)4114528-8 gnd Kosmologisches Modell (DE-588)4330709-7 gnd Inhomogenes Medium (DE-588)4228459-4 gnd |
| subject_GND | (DE-588)4079154-3 (DE-588)4114528-8 (DE-588)4330709-7 (DE-588)4228459-4 |
| title | Inhomogeneous cosmological models |
| title_auth | Inhomogeneous cosmological models |
| title_exact_search | Inhomogeneous cosmological models |
| title_full | Inhomogeneous cosmological models Andrzej Krasiński |
| title_fullStr | Inhomogeneous cosmological models Andrzej Krasiński |
| title_full_unstemmed | Inhomogeneous cosmological models Andrzej Krasiński |
| title_short | Inhomogeneous cosmological models |
| title_sort | inhomogeneous cosmological models |
| topic | Mathematisches Modell Cosmology / Mathematical models Relativity (Physics) / Mathematical models Weltall (DE-588)4079154-3 gnd Mathematisches Modell (DE-588)4114528-8 gnd Kosmologisches Modell (DE-588)4330709-7 gnd Inhomogenes Medium (DE-588)4228459-4 gnd |
| topic_facet | Mathematisches Modell Cosmology / Mathematical models Relativity (Physics) / Mathematical models Weltall Kosmologisches Modell Inhomogenes Medium |
| url | https://doi.org/10.1017/CBO9780511721694 |
| work_keys_str_mv | AT krasinskiandrzej inhomogeneouscosmologicalmodels |