Modern cosmology:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
San Diego, California
Academic Press, An Imprint of Elsevier
[2003]
|
| Schlagworte: | |
| Beschreibung: | Print version record |
| Beschreibung: | 1 online resource (xiii, 440 pages) illustrations |
| ISBN: | 9780080511979 008051197X 9781281036247 1281036242 |
Internformat
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| 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] | |
| 264 | 4 | |c 2003 | |
| 300 | |a 1 online resource (xiii, 440 pages) |b illustrations | ||
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| 505 | 8 | |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" | |
| 650 | 7 | |a SCIENCE / Cosmology |2 bisacsh | |
| 650 | 7 | |a Cosmology |2 fast | |
| 650 | 7 | |a Kosmologie |2 gtt | |
| 650 | 4 | |a Cosmology | |
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| 776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe |a Dodelson, Scott |t Modern cosmology |d San Diego, Calif. : Academic Press, 2003 |z 0122191412 |z 9780122191411 |
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| 883 | 1 | |8 2\p |a cgwrk |d 20201028 |q DE-101 |u https://d-nb.info/provenance/plan#cgwrk | |
Datensatz im Suchindex
| _version_ | 1804179158767501312 |
|---|---|
| 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 | BV045341738 |
| collection | ZDB-4-ENC |
| contents | "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" |
| ctrlnum | (ZDB-4-ENC)ocn162129438 (OCoLC)162129438 (DE-599)BVBBV045341738 |
| 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 |
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| illustrated | Illustrated |
| indexdate | 2024-07-10T08:15:25Z |
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| isbn | 9780080511979 008051197X 9781281036247 1281036242 |
| language | English |
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| spelling | Dodelson, Scott Verfasser aut Modern cosmology Scott Dodelson San Diego, California Academic Press, An Imprint of Elsevier [2003] 2003 1 online resource (xiii, 440 pages) illustrations txt rdacontent c rdamedia cr rdacarrier Print version record "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" SCIENCE / Cosmology bisacsh Cosmology fast Kosmologie gtt 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 Dodelson, Scott Modern cosmology San Diego, Calif. : Academic Press, 2003 0122191412 9780122191411 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 "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" SCIENCE / Cosmology bisacsh Cosmology fast Kosmologie gtt 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 | SCIENCE / Cosmology bisacsh Cosmology fast Kosmologie gtt Cosmology Kosmologie (DE-588)4114294-9 gnd |
| topic_facet | SCIENCE / Cosmology Cosmology Kosmologie Lehrbuch |
| work_keys_str_mv | AT dodelsonscott moderncosmology |