Modern cosmology:
Saved in:
| Main Author: | |
|---|---|
| Format: | Electronic eBook |
| Language: | English |
| Published: |
San Diego, California
Academic Press, An Imprint of Elsevier
[2003]
|
| Subjects: | |
| Online Access: | FAW01 UBM01 Volltext |
| Item Description: | Includes bibliographical references (pages 426-434) and index "Modern Cosmology begins with an introduction to the smooth, homogeneous universe described by a Friedman-Robertson-Walker metric, including careful treatments of dark energy, big bang nucleosynthesis, recombination, and dark matter. From this starting point, the reader is introduced to perturbations about an FRW universe: their evolution with the Einstein-Boltzmann equations, their generation by primordial inflation, and their observational consequences. These consequences include the anisotropy spectrum of the cosmic microwave background (CMB) featuring acoustic peaks and polarization, the matter power spectrum with baryonic wiggles, and their detection via photometric galaxy surveys, redshift distortions, cluster abundances, and weak lensing. The book concludes with a long chapter on data analysis. Modern Cosmology is the first book to explain in detail the structure of the acoustic peaks in the CMB, the E/B decomposition in polarization which may allow for detection of primordial gravity waves, and the modern analysis techniques used on increasingly large cosmological data sets. Readers will gain the tools needed to work in cosmology and learn how modern observations are rapidly revolutionizing our picture of the universe. * Provides foundations, calculations, and interpretations which illuminate current thinking in cosmology * Covers the major advances in cosmology over the past decade * Includes over 100 unique, pedagogical figures"--Provided by publisher |
| Physical Description: | 1 Online-Ressource (xiii, 440 pages) |
| ISBN: | 008051197X 1281036242 9780080511979 9781281036247 |
Staff View
MARC
| LEADER | 00000nmm a2200000zc 4500 | ||
|---|---|---|---|
| 001 | BV042311012 | ||
| 003 | DE-604 | ||
| 005 | 20160926 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 150129s2003 |||| o||u| ||||||eng d | ||
| 020 | |a 008051197X |c electronic book |9 0-08-051197-X | ||
| 020 | |a 1281036242 |9 1-281-03624-2 | ||
| 020 | |a 9780080511979 |c electronic book |9 978-0-08-051197-9 | ||
| 020 | |a 9781281036247 |9 978-1-281-03624-7 | ||
| 035 | |a (OCoLC)731735144 | ||
| 035 | |a (DE-599)BVBBV042311012 | ||
| 040 | |a DE-604 |b ger |e aacr | ||
| 041 | 0 | |a eng | |
| 049 | |a DE-1046 |a DE-19 | ||
| 082 | 0 | |a 523.1 |2 22 | |
| 084 | |a US 2000 |0 (DE-625)146681: |2 rvk | ||
| 100 | 1 | |a Dodelson, Scott |e Verfasser |4 aut | |
| 245 | 1 | 0 | |a Modern cosmology |c Scott Dodelson |
| 264 | 1 | |a San Diego, California |b Academic Press, An Imprint of Elsevier |c [2003] | |
| 300 | |a 1 Online-Ressource (xiii, 440 pages) | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 500 | |a Includes bibliographical references (pages 426-434) and index | ||
| 500 | |a "Modern Cosmology begins with an introduction to the smooth, homogeneous universe described by a Friedman-Robertson-Walker metric, including careful treatments of dark energy, big bang nucleosynthesis, recombination, and dark matter. From this starting point, the reader is introduced to perturbations about an FRW universe: their evolution with the Einstein-Boltzmann equations, their generation by primordial inflation, and their observational consequences. These consequences include the anisotropy spectrum of the cosmic microwave background (CMB) featuring acoustic peaks and polarization, the matter power spectrum with baryonic wiggles, and their detection via photometric galaxy surveys, redshift distortions, cluster abundances, and weak lensing. The book concludes with a long chapter on data analysis. Modern Cosmology is the first book to explain in detail the structure of the acoustic peaks in the CMB, the E/B decomposition in polarization which may allow for detection of primordial gravity waves, and the modern analysis techniques used on increasingly large cosmological data sets. Readers will gain the tools needed to work in cosmology and learn how modern observations are rapidly revolutionizing our picture of the universe. * Provides foundations, calculations, and interpretations which illuminate current thinking in cosmology * Covers the major advances in cosmology over the past decade * Includes over 100 unique, pedagogical figures"--Provided by publisher | ||
| 650 | 7 | |a Kosmologie |2 gtt | |
| 650 | 7 | |a SCIENCE / Cosmology |2 bisacsh | |
| 650 | 7 | |a Cosmology |2 fast | |
| 650 | 4 | |a Cosmology | |
| 650 | 0 | 7 | |a Kosmologie |0 (DE-588)4114294-9 |2 gnd |9 rswk-swf |
| 655 | 7 | |8 1\p |0 (DE-588)4123623-3 |a Lehrbuch |2 gnd-content | |
| 689 | 0 | 0 | |a Kosmologie |0 (DE-588)4114294-9 |D s |
| 689 | 0 | |8 2\p |5 DE-604 | |
| 776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe, Hardcover |z 0-12-219141-2 |
| 776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe, Hardcover |z 978-0-12-219141-1 |
| 856 | 4 | 0 | |u http://www.sciencedirect.com/science/book/9780122191411 |x Verlag |3 Volltext |
| 912 | |a ZDB-33-ESD | ||
| 940 | 1 | |q FLA_PDA_ESD | |
| 999 | |a oai:aleph.bib-bvb.de:BVB01-027748004 | ||
| 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 | |
| 966 | e | |u http://www.sciencedirect.com/science/book/9780122191411 |l FAW01 |p ZDB-33-ESD |q FAW_PDA_ESD |x Verlag |3 Volltext | |
| 966 | e | |u http://www.sciencedirect.com/science/book/9780122191411 |l UBM01 |p ZDB-33-ESD |q UBM_PDA_ESD_Kauf |x Verlag |3 Volltext | |
Record in the Search Index
| _version_ | 1804152900353523712 |
|---|---|
| any_adam_object | |
| author | Dodelson, Scott |
| author_facet | Dodelson, Scott |
| author_role | aut |
| author_sort | Dodelson, Scott |
| author_variant | s d sd |
| building | Verbundindex |
| bvnumber | BV042311012 |
| classification_rvk | US 2000 |
| collection | ZDB-33-ESD |
| ctrlnum | (OCoLC)731735144 (DE-599)BVBBV042311012 |
| dewey-full | 523.1 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.1 |
| dewey-search | 523.1 |
| dewey-sort | 3523.1 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>03640nmm a2200541zc 4500</leader><controlfield tag="001">BV042311012</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">20160926 </controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">150129s2003 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">008051197X</subfield><subfield code="c">electronic book</subfield><subfield code="9">0-08-051197-X</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">1281036242</subfield><subfield code="9">1-281-03624-2</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9780080511979</subfield><subfield code="c">electronic book</subfield><subfield code="9">978-0-08-051197-9</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9781281036247</subfield><subfield code="9">978-1-281-03624-7</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)731735144</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV042311012</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">aacr</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-1046</subfield><subfield code="a">DE-19</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">523.1</subfield><subfield code="2">22</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">Dodelson, Scott</subfield><subfield code="e">Verfasser</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Modern cosmology</subfield><subfield code="c">Scott Dodelson</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">San Diego, California</subfield><subfield code="b">Academic Press, An Imprint of Elsevier</subfield><subfield code="c">[2003]</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (xiii, 440 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">Includes bibliographical references (pages 426-434) and index</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">"Modern Cosmology begins with an introduction to the smooth, homogeneous universe described by a Friedman-Robertson-Walker metric, including careful treatments of dark energy, big bang nucleosynthesis, recombination, and dark matter. From this starting point, the reader is introduced to perturbations about an FRW universe: their evolution with the Einstein-Boltzmann equations, their generation by primordial inflation, and their observational consequences. These consequences include the anisotropy spectrum of the cosmic microwave background (CMB) featuring acoustic peaks and polarization, the matter power spectrum with baryonic wiggles, and their detection via photometric galaxy surveys, redshift distortions, cluster abundances, and weak lensing. The book concludes with a long chapter on data analysis. Modern Cosmology is the first book to explain in detail the structure of the acoustic peaks in the CMB, the E/B decomposition in polarization which may allow for detection of primordial gravity waves, and the modern analysis techniques used on increasingly large cosmological data sets. Readers will gain the tools needed to work in cosmology and learn how modern observations are rapidly revolutionizing our picture of the universe. * Provides foundations, calculations, and interpretations which illuminate current thinking in cosmology * Covers the major advances in cosmology over the past decade * Includes over 100 unique, pedagogical figures"--Provided by publisher</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Kosmologie</subfield><subfield code="2">gtt</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">SCIENCE / Cosmology</subfield><subfield code="2">bisacsh</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Cosmology</subfield><subfield code="2">fast</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Cosmology</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Kosmologie</subfield><subfield code="0">(DE-588)4114294-9</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="655" ind1=" " ind2="7"><subfield code="8">1\p</subfield><subfield code="0">(DE-588)4123623-3</subfield><subfield code="a">Lehrbuch</subfield><subfield code="2">gnd-content</subfield></datafield><datafield tag="689" ind1="0" ind2="0"><subfield code="a">Kosmologie</subfield><subfield code="0">(DE-588)4114294-9</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" 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">Druck-Ausgabe, Hardcover</subfield><subfield code="z">0-12-219141-2</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druck-Ausgabe, Hardcover</subfield><subfield code="z">978-0-12-219141-1</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://www.sciencedirect.com/science/book/9780122191411</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-33-ESD</subfield></datafield><datafield tag="940" ind1="1" ind2=" "><subfield code="q">FLA_PDA_ESD</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-027748004</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="966" ind1="e" ind2=" "><subfield code="u">http://www.sciencedirect.com/science/book/9780122191411</subfield><subfield code="l">FAW01</subfield><subfield code="p">ZDB-33-ESD</subfield><subfield code="q">FAW_PDA_ESD</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="966" ind1="e" ind2=" "><subfield code="u">http://www.sciencedirect.com/science/book/9780122191411</subfield><subfield code="l">UBM01</subfield><subfield code="p">ZDB-33-ESD</subfield><subfield code="q">UBM_PDA_ESD_Kauf</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield></record></collection> |
| genre | 1\p (DE-588)4123623-3 Lehrbuch gnd-content |
| genre_facet | Lehrbuch |
| id | DE-604.BV042311012 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:18:03Z |
| institution | BVB |
| isbn | 008051197X 1281036242 9780080511979 9781281036247 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027748004 |
| oclc_num | 731735144 |
| open_access_boolean | |
| owner | DE-1046 DE-19 DE-BY-UBM |
| owner_facet | DE-1046 DE-19 DE-BY-UBM |
| physical | 1 Online-Ressource (xiii, 440 pages) |
| psigel | ZDB-33-ESD FLA_PDA_ESD ZDB-33-ESD FAW_PDA_ESD ZDB-33-ESD UBM_PDA_ESD_Kauf |
| publishDate | 2003 |
| publishDateSearch | 2003 |
| publishDateSort | 2003 |
| publisher | Academic Press, An Imprint of Elsevier |
| record_format | marc |
| spelling | Dodelson, Scott Verfasser aut Modern cosmology Scott Dodelson San Diego, California Academic Press, An Imprint of Elsevier [2003] 1 Online-Ressource (xiii, 440 pages) txt rdacontent c rdamedia cr rdacarrier Includes bibliographical references (pages 426-434) and index "Modern Cosmology begins with an introduction to the smooth, homogeneous universe described by a Friedman-Robertson-Walker metric, including careful treatments of dark energy, big bang nucleosynthesis, recombination, and dark matter. From this starting point, the reader is introduced to perturbations about an FRW universe: their evolution with the Einstein-Boltzmann equations, their generation by primordial inflation, and their observational consequences. These consequences include the anisotropy spectrum of the cosmic microwave background (CMB) featuring acoustic peaks and polarization, the matter power spectrum with baryonic wiggles, and their detection via photometric galaxy surveys, redshift distortions, cluster abundances, and weak lensing. The book concludes with a long chapter on data analysis. Modern Cosmology is the first book to explain in detail the structure of the acoustic peaks in the CMB, the E/B decomposition in polarization which may allow for detection of primordial gravity waves, and the modern analysis techniques used on increasingly large cosmological data sets. Readers will gain the tools needed to work in cosmology and learn how modern observations are rapidly revolutionizing our picture of the universe. * Provides foundations, calculations, and interpretations which illuminate current thinking in cosmology * Covers the major advances in cosmology over the past decade * Includes over 100 unique, pedagogical figures"--Provided by publisher Kosmologie gtt SCIENCE / Cosmology bisacsh Cosmology fast Cosmology Kosmologie (DE-588)4114294-9 gnd rswk-swf 1\p (DE-588)4123623-3 Lehrbuch gnd-content Kosmologie (DE-588)4114294-9 s 2\p DE-604 Erscheint auch als Druck-Ausgabe, Hardcover 0-12-219141-2 Erscheint auch als Druck-Ausgabe, Hardcover 978-0-12-219141-1 http://www.sciencedirect.com/science/book/9780122191411 Verlag 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 | Dodelson, Scott Modern cosmology Kosmologie gtt SCIENCE / Cosmology bisacsh Cosmology fast Cosmology Kosmologie (DE-588)4114294-9 gnd |
| subject_GND | (DE-588)4114294-9 (DE-588)4123623-3 |
| title | Modern cosmology |
| title_auth | Modern cosmology |
| title_exact_search | Modern cosmology |
| title_full | Modern cosmology Scott Dodelson |
| title_fullStr | Modern cosmology Scott Dodelson |
| title_full_unstemmed | Modern cosmology Scott Dodelson |
| title_short | Modern cosmology |
| title_sort | modern cosmology |
| topic | Kosmologie gtt SCIENCE / Cosmology bisacsh Cosmology fast Cosmology Kosmologie (DE-588)4114294-9 gnd |
| topic_facet | Kosmologie SCIENCE / Cosmology Cosmology Lehrbuch |
| url | http://www.sciencedirect.com/science/book/9780122191411 |
| work_keys_str_mv | AT dodelsonscott moderncosmology |