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...
Gespeichert in:
Beteilige Person: | |
---|---|
Format: | Elektronisch E-Book |
Sprache: | Englisch |
Veröffentlicht: |
Cambridge
Cambridge University Press
1997
|
Schlagwörter: | |
Links: | https://doi.org/10.1017/CBO9780511721694 https://doi.org/10.1017/CBO9780511721694 https://doi.org/10.1017/CBO9780511721694 |
Zusammenfassung: | 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 |
Beschreibung: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
Umfang: | 1 online resource (xvi, 317 pages) |
ISBN: | 9780511721694 |
DOI: | 10.1017/CBO9780511721694 |
Internformat
MARC
LEADER | 00000nam a2200000zc 4500 | ||
---|---|---|---|
001 | BV043945762 | ||
003 | DE-604 | ||
005 | 00000000000000.0 | ||
007 | cr|uuu---uuuuu | ||
008 | 161206s1997 xx o|||| 00||| eng d | ||
020 | |a 9780511721694 |c Online |9 978-0-511-72169-4 | ||
024 | 7 | |a 10.1017/CBO9780511721694 |2 doi | |
035 | |a (ZDB-20-CBO)CR9780511721694 | ||
035 | |a (OCoLC)992869287 | ||
035 | |a (DE-599)BVBBV043945762 | ||
040 | |a DE-604 |b ger |e rda | ||
041 | 0 | |a eng | |
049 | |a DE-12 |a DE-92 | ||
082 | 0 | |a 523.1/01/5118 |2 20 | |
084 | |a US 2000 |0 (DE-625)146681: |2 rvk | ||
100 | 1 | |a Krasiński, Andrzej |e Verfasser |4 aut | |
245 | 1 | 0 | |a Inhomogeneous cosmological models |c Andrzej Krasiński |
264 | 1 | |a Cambridge |b Cambridge University Press |c 1997 | |
300 | |a 1 online resource (xvi, 317 pages) | ||
336 | |b txt |2 rdacontent | ||
337 | |b c |2 rdamedia | ||
338 | |b cr |2 rdacarrier | ||
500 | |a Title from publisher's bibliographic system (viewed on 05 Oct 2015) | ||
505 | 8 | |a 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 | |
520 | |a 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 | ||
650 | 4 | |a Mathematisches Modell | |
650 | 4 | |a Cosmology / Mathematical models | |
650 | 4 | |a Relativity (Physics) / Mathematical models | |
650 | 0 | 7 | |a Weltall |0 (DE-588)4079154-3 |2 gnd |9 rswk-swf |
650 | 0 | 7 | |a Mathematisches Modell |0 (DE-588)4114528-8 |2 gnd |9 rswk-swf |
650 | 0 | 7 | |a Kosmologisches Modell |0 (DE-588)4330709-7 |2 gnd |9 rswk-swf |
650 | 0 | 7 | |a Inhomogenes Medium |0 (DE-588)4228459-4 |2 gnd |9 rswk-swf |
689 | 0 | 0 | |a Weltall |0 (DE-588)4079154-3 |D s |
689 | 0 | 1 | |a Mathematisches Modell |0 (DE-588)4114528-8 |D s |
689 | 0 | |8 1\p |5 DE-604 | |
689 | 1 | 0 | |a Kosmologisches Modell |0 (DE-588)4330709-7 |D s |
689 | 1 | 1 | |a Inhomogenes Medium |0 (DE-588)4228459-4 |D s |
689 | 1 | |8 2\p |5 DE-604 | |
776 | 0 | 8 | |i Erscheint auch als |n Druckausgabe |z 978-0-521-03017-5 |
776 | 0 | 8 | |i Erscheint auch als |n Druckausgabe |z 978-0-521-48180-9 |
856 | 4 | 0 | |u https://doi.org/10.1017/CBO9780511721694 |x Verlag |z URL des Erstveröffentlichers |3 Volltext |
912 | |a ZDB-20-CBO | ||
883 | 1 | |8 1\p |a cgwrk |d 20201028 |q DE-101 |u https://d-nb.info/provenance/plan#cgwrk | |
883 | 1 | |8 2\p |a cgwrk |d 20201028 |q DE-101 |u https://d-nb.info/provenance/plan#cgwrk | |
943 | 1 | |a oai:aleph.bib-bvb.de:BVB01-029354733 | |
966 | e | |u https://doi.org/10.1017/CBO9780511721694 |l DE-12 |p ZDB-20-CBO |q BSB_PDA_CBO |x Verlag |3 Volltext | |
966 | e | |u https://doi.org/10.1017/CBO9780511721694 |l DE-92 |p ZDB-20-CBO |q FHN_PDA_CBO |x Verlag |3 Volltext |
Datensatz im Suchindex
_version_ | 1818982577708466176 |
---|---|
any_adam_object | |
author | Krasiński, Andrzej |
author_facet | Krasiński, Andrzej |
author_role | aut |
author_sort | Krasiński, Andrzej |
author_variant | a k ak |
building | Verbundindex |
bvnumber | BV043945762 |
classification_rvk | US 2000 |
collection | ZDB-20-CBO |
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 |
ctrlnum | (ZDB-20-CBO)CR9780511721694 (OCoLC)992869287 (DE-599)BVBBV043945762 |
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 |
dewey-sort | 3523.1 11 45118 |
dewey-tens | 520 - Astronomy and allied sciences |
discipline | Physik |
doi_str_mv | 10.1017/CBO9780511721694 |
format | Electronic eBook |
fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>04092nam a2200589zc 4500</leader><controlfield tag="001">BV043945762</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">00000000000000.0</controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">161206s1997 xx o|||| 00||| eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9780511721694</subfield><subfield code="c">Online</subfield><subfield code="9">978-0-511-72169-4</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1017/CBO9780511721694</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ZDB-20-CBO)CR9780511721694</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)992869287</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV043945762</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-12</subfield><subfield code="a">DE-92</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">523.1/01/5118</subfield><subfield code="2">20</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">US 2000</subfield><subfield code="0">(DE-625)146681:</subfield><subfield code="2">rvk</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Krasiński, Andrzej</subfield><subfield code="e">Verfasser</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Inhomogeneous cosmological models</subfield><subfield code="c">Andrzej Krasiński</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Cambridge</subfield><subfield code="b">Cambridge University Press</subfield><subfield code="c">1997</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 online resource (xvi, 317 pages)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Title from publisher's bibliographic system (viewed on 05 Oct 2015)</subfield></datafield><datafield tag="505" ind1="8" ind2=" "><subfield code="a">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</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">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</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Mathematisches Modell</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Cosmology / Mathematical models</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Relativity (Physics) / Mathematical models</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Weltall</subfield><subfield code="0">(DE-588)4079154-3</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Mathematisches Modell</subfield><subfield code="0">(DE-588)4114528-8</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Kosmologisches Modell</subfield><subfield code="0">(DE-588)4330709-7</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Inhomogenes Medium</subfield><subfield code="0">(DE-588)4228459-4</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="689" ind1="0" ind2="0"><subfield code="a">Weltall</subfield><subfield code="0">(DE-588)4079154-3</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2="1"><subfield code="a">Mathematisches Modell</subfield><subfield code="0">(DE-588)4114528-8</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2=" "><subfield code="8">1\p</subfield><subfield code="5">DE-604</subfield></datafield><datafield tag="689" ind1="1" ind2="0"><subfield code="a">Kosmologisches Modell</subfield><subfield code="0">(DE-588)4330709-7</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="1" ind2="1"><subfield code="a">Inhomogenes Medium</subfield><subfield code="0">(DE-588)4228459-4</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="1" ind2=" "><subfield code="8">2\p</subfield><subfield code="5">DE-604</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druckausgabe</subfield><subfield code="z">978-0-521-03017-5</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druckausgabe</subfield><subfield code="z">978-0-521-48180-9</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1017/CBO9780511721694</subfield><subfield code="x">Verlag</subfield><subfield code="z">URL des Erstveröffentlichers</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-20-CBO</subfield></datafield><datafield tag="883" ind1="1" ind2=" "><subfield code="8">1\p</subfield><subfield code="a">cgwrk</subfield><subfield code="d">20201028</subfield><subfield code="q">DE-101</subfield><subfield code="u">https://d-nb.info/provenance/plan#cgwrk</subfield></datafield><datafield tag="883" ind1="1" ind2=" "><subfield code="8">2\p</subfield><subfield code="a">cgwrk</subfield><subfield code="d">20201028</subfield><subfield code="q">DE-101</subfield><subfield code="u">https://d-nb.info/provenance/plan#cgwrk</subfield></datafield><datafield tag="943" ind1="1" ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-029354733</subfield></datafield><datafield tag="966" ind1="e" ind2=" "><subfield code="u">https://doi.org/10.1017/CBO9780511721694</subfield><subfield code="l">DE-12</subfield><subfield code="p">ZDB-20-CBO</subfield><subfield code="q">BSB_PDA_CBO</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="966" ind1="e" ind2=" "><subfield code="u">https://doi.org/10.1017/CBO9780511721694</subfield><subfield code="l">DE-92</subfield><subfield code="p">ZDB-20-CBO</subfield><subfield code="q">FHN_PDA_CBO</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield></record></collection> |
id | DE-604.BV043945762 |
illustrated | Not Illustrated |
indexdate | 2024-12-20T17:49:26Z |
institution | BVB |
isbn | 9780511721694 |
language | English |
oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-029354733 |
oclc_num | 992869287 |
open_access_boolean | |
owner | DE-12 DE-92 |
owner_facet | DE-12 DE-92 |
physical | 1 online resource (xvi, 317 pages) |
psigel | ZDB-20-CBO ZDB-20-CBO BSB_PDA_CBO ZDB-20-CBO FHN_PDA_CBO |
publishDate | 1997 |
publishDateSearch | 1997 |
publishDateSort | 1997 |
publisher | Cambridge University Press |
record_format | marc |
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 |