Cosmology's century: an inside history of our modern understanding of the Universe
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Princeton ; Oxford
Princeton University Press
2020
|
| Schlagworte: | |
| Online-Zugang: | TUM01 |
| Beschreibung: | Description based on publisher supplied metadata and other sources |
| Beschreibung: | 1 Online-Ressource (xvii, 403 Seiten) Illustrationen, Diagramme |
| ISBN: | 9780691201665 |
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| 100 | 1 | |a Peebles, P. J. E. |d 1935- |e Verfasser |0 (DE-588)140955194 |4 aut | |
| 245 | 1 | 0 | |a Cosmology's century |b an inside history of our modern understanding of the Universe |c P.J.E. Peebles |
| 264 | 1 | |a Princeton ; Oxford |b Princeton University Press |c 2020 | |
| 264 | 4 | |c © 2020 | |
| 300 | |a 1 Online-Ressource (xvii, 403 Seiten) |b Illustrationen, Diagramme | ||
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| 505 | 8 | |a Cover -- Contents -- Preface and Acknowledgments -- CHAPTER 1. Introduction -- 1.1 The Science and Philosophy of Cosmology -- 1.2 An Overview -- CHAPTER 2. The Homogeneous Universe -- 2.1 Einstein's Cosmological Principle -- 2.2 Early Evidence of Inhomogeneity -- 2.3 Early Evidence of Homogeneity: Isotropy -- 2.4 Early Evidence of Homogeneity: Counts and Redshifts -- 2.5 The Universe as a Stationary Random Process -- 2.6 A Fractal Universe -- 2.7 Concluding Remarks -- CHAPTER 3. Cosmological Models -- 3.1 Discovery of the Relativistic Expanding Universe -- 3.2 The Relativistic Big Bang Cosmology -- 3.3 The Steady-State Cosmology -- 3.4 Empirical Assessments of the Steady-State Cosmology -- 3.5 Nonempirical Assessments of the Big Bang Model -- 3.5.1 Early Thinking -- 3.5.2 Cosmological Inflation -- 3.5.3 Biasing -- 3.6 Empirical Assessments of the Big Bang Model -- 3.6.1 Time Scales -- 3.6.2 Cosmological Tests in the 1970s -- 3.6.3 Mass Density Measurements: Introduction -- 3.6.4 Mass Density Measurements: Hubble to the Revolution -- 3.6.5 Mass Density Measurements: Assessments -- 3.7 Concluding Remarks -- CHAPTER 4. Fossils: Microwave Radiation and Light Elements -- 4.1 Thermal Radiation in an Expanding Universe -- 4.2 Gamow's Scenario -- 4.2.1 Gamow's 1948 Papers -- 4.2.2 Predicting the Present CMB Temperature -- 4.2.3 The Alpher, Bethe, and Gamow Paper -- 4.3 Helium and Deuterium from the Hot Big Bang -- 4.3.1 Recognition of Fossil Helium -- 4.3.2 Helium in a Cold Universe -- 4.3.3 Developments in 1964 and 1965 -- 4.4 Sources of Microwave Radiation -- 4.4.1 Interstellar Cyanogen -- 4.4.2 Detection at Bell Laboratories -- 4.4.3 Zel'dovich's Group -- 4.4.4 Dicke's Group -- 4.4.5 Recognition of the CMB -- 4.5 Measuring the CMB Intensity Spectrum -- 4.5.1 The Situation in the 1970s -- 4.5.2 Alternative Interpretations | |
| 505 | 8 | |a 4.5.3 The Submillimeter Anomalies -- 4.5.4 Establishing the CMB Thermal Spectrum -- 4.6 Nucleosynthesis and the Baryon Mass Density -- 4.7 Why Was the Hot Big Bang Cosmology Reinvented? -- CHAPTER 5. How Cosmic Structure Grew -- 5.1 The Gravitational Instability Picture -- 5.1.1 Lemaître's Solution -- 5.1.2 Lifshitz's Perturbation Analyses -- 5.1.3 Nongravitational Interaction of Baryons and the CMB -- 5.1.4 The Jeans Mass -- 5.2 Scenarios -- 5.2.1 Chaos and Order -- 5.2.2 Primeval Turbulence -- 5.2.3 Gravitational Origin of Galaxy Rotation -- 5.2.4 Explosions -- 5.2.5 Spontaneously Broken Homogeneity -- 5.2.6 Initial Conditions -- 5.2.7 Bottom-Up or Top-Down Structure Formation -- 5.3 Concluding Remarks -- CHAPTER 6. Subluminal Mass -- 6.1 Clusters of Galaxies -- 6.2 Groups of Galaxies -- 6.3 Galaxy Rotation Curves -- 6.3.1 The Andromeda Nebula -- 6.3.2 NGC 311525 -- 6.3.3 NGC 300 -- 6.3.4 NGC 2403 -- 6.3.5 The Burbidges's Program -- 6.3.6 Challenges -- 6.4 Stabilizing Spiral Galaxies -- 6.5 Recognizing Subluminal Matter -- 6.6 What Is the Nature of the Subluminal Matter? -- CHAPTER 7. Nonbaryonic Dark Matter -- 7.1 Hot Dark Matter -- 7.1.1 Apparent Detection of a Neutrino Rest Mass -- 7.2 Cold Dark Matter -- 7.2.1 What Happened in 1977 -- 7.2.2 The Situation in the Early 1980s -- 7.2.3 The Search for Dark Matter Detection -- CHAPTER 8. The Age of Abundance of Cosmological Models -- 8.1 Why Is the CMB So Smooth? -- 8.2 The Counterexample: CDM -- 8.3 CDM and Structure Formation -- 8.4 Variations on the Theme -- 8.4.1 TCDM -- 8.4.2 DDM and MDM -- 8.4.3 ΛCDM and τCDM -- 8.4.4 Other Thoughts -- 8.5 How Might It All Fit Together? -- CHAPTER 9. The 1998-2003 Revolution -- 9.1 The Redshift-Magnitude Test -- 9.2 The CMB Temperature Anisotropy -- 9.3 What Happened at the Turn of the Century -- 9.4 The Future of Physical Cosmology | |
| 505 | 8 | |a CHAPTER 10. The Ways of Research -- 10.1 Technology -- 10.2 Human Behavior -- 10.3 Roads Not Taken -- 10.4 The Social Construction of Science -- References -- Index -- Color Plates | |
| 648 | 7 | |a Geschichte 1917-2003 |2 gnd |9 rswk-swf | |
| 650 | 4 | |a Cosmology | |
| 650 | 0 | 7 | |a Kosmologie |0 (DE-588)4114294-9 |2 gnd |9 rswk-swf |
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| 689 | 0 | 1 | |a Geschichte 1917-2003 |A z |
| 689 | 0 | |5 DE-604 | |
| 776 | 0 | 8 | |i Erscheint auch als |a Peebles, P. J. E. |t Cosmology's Century |d Princeton : Princeton University Press,c2020 |n Druck-Ausgabe |z 978-0-691-19602-2 |
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Datensatz im Suchindex
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| author | Peebles, P. J. E. 1935- |
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| author_facet | Peebles, P. J. E. 1935- |
| author_role | aut |
| author_sort | Peebles, P. J. E. 1935- |
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| building | Verbundindex |
| bvnumber | BV047441691 |
| classification_rvk | UB 2484 |
| classification_tum | PHY 900 PHY 006 |
| collection | ZDB-30-PQE |
| contents | Cover -- Contents -- Preface and Acknowledgments -- CHAPTER 1. Introduction -- 1.1 The Science and Philosophy of Cosmology -- 1.2 An Overview -- CHAPTER 2. The Homogeneous Universe -- 2.1 Einstein's Cosmological Principle -- 2.2 Early Evidence of Inhomogeneity -- 2.3 Early Evidence of Homogeneity: Isotropy -- 2.4 Early Evidence of Homogeneity: Counts and Redshifts -- 2.5 The Universe as a Stationary Random Process -- 2.6 A Fractal Universe -- 2.7 Concluding Remarks -- CHAPTER 3. Cosmological Models -- 3.1 Discovery of the Relativistic Expanding Universe -- 3.2 The Relativistic Big Bang Cosmology -- 3.3 The Steady-State Cosmology -- 3.4 Empirical Assessments of the Steady-State Cosmology -- 3.5 Nonempirical Assessments of the Big Bang Model -- 3.5.1 Early Thinking -- 3.5.2 Cosmological Inflation -- 3.5.3 Biasing -- 3.6 Empirical Assessments of the Big Bang Model -- 3.6.1 Time Scales -- 3.6.2 Cosmological Tests in the 1970s -- 3.6.3 Mass Density Measurements: Introduction -- 3.6.4 Mass Density Measurements: Hubble to the Revolution -- 3.6.5 Mass Density Measurements: Assessments -- 3.7 Concluding Remarks -- CHAPTER 4. Fossils: Microwave Radiation and Light Elements -- 4.1 Thermal Radiation in an Expanding Universe -- 4.2 Gamow's Scenario -- 4.2.1 Gamow's 1948 Papers -- 4.2.2 Predicting the Present CMB Temperature -- 4.2.3 The Alpher, Bethe, and Gamow Paper -- 4.3 Helium and Deuterium from the Hot Big Bang -- 4.3.1 Recognition of Fossil Helium -- 4.3.2 Helium in a Cold Universe -- 4.3.3 Developments in 1964 and 1965 -- 4.4 Sources of Microwave Radiation -- 4.4.1 Interstellar Cyanogen -- 4.4.2 Detection at Bell Laboratories -- 4.4.3 Zel'dovich's Group -- 4.4.4 Dicke's Group -- 4.4.5 Recognition of the CMB -- 4.5 Measuring the CMB Intensity Spectrum -- 4.5.1 The Situation in the 1970s -- 4.5.2 Alternative Interpretations 4.5.3 The Submillimeter Anomalies -- 4.5.4 Establishing the CMB Thermal Spectrum -- 4.6 Nucleosynthesis and the Baryon Mass Density -- 4.7 Why Was the Hot Big Bang Cosmology Reinvented? -- CHAPTER 5. How Cosmic Structure Grew -- 5.1 The Gravitational Instability Picture -- 5.1.1 Lemaître's Solution -- 5.1.2 Lifshitz's Perturbation Analyses -- 5.1.3 Nongravitational Interaction of Baryons and the CMB -- 5.1.4 The Jeans Mass -- 5.2 Scenarios -- 5.2.1 Chaos and Order -- 5.2.2 Primeval Turbulence -- 5.2.3 Gravitational Origin of Galaxy Rotation -- 5.2.4 Explosions -- 5.2.5 Spontaneously Broken Homogeneity -- 5.2.6 Initial Conditions -- 5.2.7 Bottom-Up or Top-Down Structure Formation -- 5.3 Concluding Remarks -- CHAPTER 6. Subluminal Mass -- 6.1 Clusters of Galaxies -- 6.2 Groups of Galaxies -- 6.3 Galaxy Rotation Curves -- 6.3.1 The Andromeda Nebula -- 6.3.2 NGC 311525 -- 6.3.3 NGC 300 -- 6.3.4 NGC 2403 -- 6.3.5 The Burbidges's Program -- 6.3.6 Challenges -- 6.4 Stabilizing Spiral Galaxies -- 6.5 Recognizing Subluminal Matter -- 6.6 What Is the Nature of the Subluminal Matter? -- CHAPTER 7. Nonbaryonic Dark Matter -- 7.1 Hot Dark Matter -- 7.1.1 Apparent Detection of a Neutrino Rest Mass -- 7.2 Cold Dark Matter -- 7.2.1 What Happened in 1977 -- 7.2.2 The Situation in the Early 1980s -- 7.2.3 The Search for Dark Matter Detection -- CHAPTER 8. The Age of Abundance of Cosmological Models -- 8.1 Why Is the CMB So Smooth? -- 8.2 The Counterexample: CDM -- 8.3 CDM and Structure Formation -- 8.4 Variations on the Theme -- 8.4.1 TCDM -- 8.4.2 DDM and MDM -- 8.4.3 ΛCDM and τCDM -- 8.4.4 Other Thoughts -- 8.5 How Might It All Fit Together? -- CHAPTER 9. The 1998-2003 Revolution -- 9.1 The Redshift-Magnitude Test -- 9.2 The CMB Temperature Anisotropy -- 9.3 What Happened at the Turn of the Century -- 9.4 The Future of Physical Cosmology CHAPTER 10. The Ways of Research -- 10.1 Technology -- 10.2 Human Behavior -- 10.3 Roads Not Taken -- 10.4 The Social Construction of Science -- References -- Index -- Color Plates |
| ctrlnum | (ZDB-30-PQE)EBC6214864 (ZDB-30-PAD)EBC6214864 (ZDB-89-EBL)EBL6214864 (OCoLC)1152229023 (DE-599)BVBBV047441691 |
| 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 |
| discipline_str_mv | Physik |
| era | Geschichte 1917-2003 gnd |
| era_facet | Geschichte 1917-2003 |
| format | Electronic eBook |
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| id | DE-604.BV047441691 |
| illustrated | Not Illustrated |
| index_date | 2024-07-03T18:01:23Z |
| indexdate | 2024-07-10T09:12:15Z |
| institution | BVB |
| isbn | 9780691201665 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-032843843 |
| oclc_num | 1152229023 |
| open_access_boolean | |
| owner | DE-91 DE-BY-TUM |
| owner_facet | DE-91 DE-BY-TUM |
| physical | 1 Online-Ressource (xvii, 403 Seiten) Illustrationen, Diagramme |
| psigel | ZDB-30-PQE ZDB-30-PQE TUM_PDA_PQE_Kauf |
| publishDate | 2020 |
| publishDateSearch | 2020 |
| publishDateSort | 2020 |
| publisher | Princeton University Press |
| record_format | marc |
| spelling | Peebles, P. J. E. 1935- Verfasser (DE-588)140955194 aut Cosmology's century an inside history of our modern understanding of the Universe P.J.E. Peebles Princeton ; Oxford Princeton University Press 2020 © 2020 1 Online-Ressource (xvii, 403 Seiten) Illustrationen, Diagramme txt rdacontent c rdamedia cr rdacarrier Description based on publisher supplied metadata and other sources Cover -- Contents -- Preface and Acknowledgments -- CHAPTER 1. Introduction -- 1.1 The Science and Philosophy of Cosmology -- 1.2 An Overview -- CHAPTER 2. The Homogeneous Universe -- 2.1 Einstein's Cosmological Principle -- 2.2 Early Evidence of Inhomogeneity -- 2.3 Early Evidence of Homogeneity: Isotropy -- 2.4 Early Evidence of Homogeneity: Counts and Redshifts -- 2.5 The Universe as a Stationary Random Process -- 2.6 A Fractal Universe -- 2.7 Concluding Remarks -- CHAPTER 3. Cosmological Models -- 3.1 Discovery of the Relativistic Expanding Universe -- 3.2 The Relativistic Big Bang Cosmology -- 3.3 The Steady-State Cosmology -- 3.4 Empirical Assessments of the Steady-State Cosmology -- 3.5 Nonempirical Assessments of the Big Bang Model -- 3.5.1 Early Thinking -- 3.5.2 Cosmological Inflation -- 3.5.3 Biasing -- 3.6 Empirical Assessments of the Big Bang Model -- 3.6.1 Time Scales -- 3.6.2 Cosmological Tests in the 1970s -- 3.6.3 Mass Density Measurements: Introduction -- 3.6.4 Mass Density Measurements: Hubble to the Revolution -- 3.6.5 Mass Density Measurements: Assessments -- 3.7 Concluding Remarks -- CHAPTER 4. Fossils: Microwave Radiation and Light Elements -- 4.1 Thermal Radiation in an Expanding Universe -- 4.2 Gamow's Scenario -- 4.2.1 Gamow's 1948 Papers -- 4.2.2 Predicting the Present CMB Temperature -- 4.2.3 The Alpher, Bethe, and Gamow Paper -- 4.3 Helium and Deuterium from the Hot Big Bang -- 4.3.1 Recognition of Fossil Helium -- 4.3.2 Helium in a Cold Universe -- 4.3.3 Developments in 1964 and 1965 -- 4.4 Sources of Microwave Radiation -- 4.4.1 Interstellar Cyanogen -- 4.4.2 Detection at Bell Laboratories -- 4.4.3 Zel'dovich's Group -- 4.4.4 Dicke's Group -- 4.4.5 Recognition of the CMB -- 4.5 Measuring the CMB Intensity Spectrum -- 4.5.1 The Situation in the 1970s -- 4.5.2 Alternative Interpretations 4.5.3 The Submillimeter Anomalies -- 4.5.4 Establishing the CMB Thermal Spectrum -- 4.6 Nucleosynthesis and the Baryon Mass Density -- 4.7 Why Was the Hot Big Bang Cosmology Reinvented? -- CHAPTER 5. How Cosmic Structure Grew -- 5.1 The Gravitational Instability Picture -- 5.1.1 Lemaître's Solution -- 5.1.2 Lifshitz's Perturbation Analyses -- 5.1.3 Nongravitational Interaction of Baryons and the CMB -- 5.1.4 The Jeans Mass -- 5.2 Scenarios -- 5.2.1 Chaos and Order -- 5.2.2 Primeval Turbulence -- 5.2.3 Gravitational Origin of Galaxy Rotation -- 5.2.4 Explosions -- 5.2.5 Spontaneously Broken Homogeneity -- 5.2.6 Initial Conditions -- 5.2.7 Bottom-Up or Top-Down Structure Formation -- 5.3 Concluding Remarks -- CHAPTER 6. Subluminal Mass -- 6.1 Clusters of Galaxies -- 6.2 Groups of Galaxies -- 6.3 Galaxy Rotation Curves -- 6.3.1 The Andromeda Nebula -- 6.3.2 NGC 311525 -- 6.3.3 NGC 300 -- 6.3.4 NGC 2403 -- 6.3.5 The Burbidges's Program -- 6.3.6 Challenges -- 6.4 Stabilizing Spiral Galaxies -- 6.5 Recognizing Subluminal Matter -- 6.6 What Is the Nature of the Subluminal Matter? -- CHAPTER 7. Nonbaryonic Dark Matter -- 7.1 Hot Dark Matter -- 7.1.1 Apparent Detection of a Neutrino Rest Mass -- 7.2 Cold Dark Matter -- 7.2.1 What Happened in 1977 -- 7.2.2 The Situation in the Early 1980s -- 7.2.3 The Search for Dark Matter Detection -- CHAPTER 8. The Age of Abundance of Cosmological Models -- 8.1 Why Is the CMB So Smooth? -- 8.2 The Counterexample: CDM -- 8.3 CDM and Structure Formation -- 8.4 Variations on the Theme -- 8.4.1 TCDM -- 8.4.2 DDM and MDM -- 8.4.3 ΛCDM and τCDM -- 8.4.4 Other Thoughts -- 8.5 How Might It All Fit Together? -- CHAPTER 9. The 1998-2003 Revolution -- 9.1 The Redshift-Magnitude Test -- 9.2 The CMB Temperature Anisotropy -- 9.3 What Happened at the Turn of the Century -- 9.4 The Future of Physical Cosmology CHAPTER 10. The Ways of Research -- 10.1 Technology -- 10.2 Human Behavior -- 10.3 Roads Not Taken -- 10.4 The Social Construction of Science -- References -- Index -- Color Plates Geschichte 1917-2003 gnd rswk-swf Cosmology Kosmologie (DE-588)4114294-9 gnd rswk-swf Kosmologie (DE-588)4114294-9 s Geschichte 1917-2003 z DE-604 Erscheint auch als Peebles, P. J. E. Cosmology's Century Princeton : Princeton University Press,c2020 Druck-Ausgabe 978-0-691-19602-2 |
| spellingShingle | Peebles, P. J. E. 1935- Cosmology's century an inside history of our modern understanding of the Universe Cover -- Contents -- Preface and Acknowledgments -- CHAPTER 1. Introduction -- 1.1 The Science and Philosophy of Cosmology -- 1.2 An Overview -- CHAPTER 2. The Homogeneous Universe -- 2.1 Einstein's Cosmological Principle -- 2.2 Early Evidence of Inhomogeneity -- 2.3 Early Evidence of Homogeneity: Isotropy -- 2.4 Early Evidence of Homogeneity: Counts and Redshifts -- 2.5 The Universe as a Stationary Random Process -- 2.6 A Fractal Universe -- 2.7 Concluding Remarks -- CHAPTER 3. Cosmological Models -- 3.1 Discovery of the Relativistic Expanding Universe -- 3.2 The Relativistic Big Bang Cosmology -- 3.3 The Steady-State Cosmology -- 3.4 Empirical Assessments of the Steady-State Cosmology -- 3.5 Nonempirical Assessments of the Big Bang Model -- 3.5.1 Early Thinking -- 3.5.2 Cosmological Inflation -- 3.5.3 Biasing -- 3.6 Empirical Assessments of the Big Bang Model -- 3.6.1 Time Scales -- 3.6.2 Cosmological Tests in the 1970s -- 3.6.3 Mass Density Measurements: Introduction -- 3.6.4 Mass Density Measurements: Hubble to the Revolution -- 3.6.5 Mass Density Measurements: Assessments -- 3.7 Concluding Remarks -- CHAPTER 4. Fossils: Microwave Radiation and Light Elements -- 4.1 Thermal Radiation in an Expanding Universe -- 4.2 Gamow's Scenario -- 4.2.1 Gamow's 1948 Papers -- 4.2.2 Predicting the Present CMB Temperature -- 4.2.3 The Alpher, Bethe, and Gamow Paper -- 4.3 Helium and Deuterium from the Hot Big Bang -- 4.3.1 Recognition of Fossil Helium -- 4.3.2 Helium in a Cold Universe -- 4.3.3 Developments in 1964 and 1965 -- 4.4 Sources of Microwave Radiation -- 4.4.1 Interstellar Cyanogen -- 4.4.2 Detection at Bell Laboratories -- 4.4.3 Zel'dovich's Group -- 4.4.4 Dicke's Group -- 4.4.5 Recognition of the CMB -- 4.5 Measuring the CMB Intensity Spectrum -- 4.5.1 The Situation in the 1970s -- 4.5.2 Alternative Interpretations 4.5.3 The Submillimeter Anomalies -- 4.5.4 Establishing the CMB Thermal Spectrum -- 4.6 Nucleosynthesis and the Baryon Mass Density -- 4.7 Why Was the Hot Big Bang Cosmology Reinvented? -- CHAPTER 5. How Cosmic Structure Grew -- 5.1 The Gravitational Instability Picture -- 5.1.1 Lemaître's Solution -- 5.1.2 Lifshitz's Perturbation Analyses -- 5.1.3 Nongravitational Interaction of Baryons and the CMB -- 5.1.4 The Jeans Mass -- 5.2 Scenarios -- 5.2.1 Chaos and Order -- 5.2.2 Primeval Turbulence -- 5.2.3 Gravitational Origin of Galaxy Rotation -- 5.2.4 Explosions -- 5.2.5 Spontaneously Broken Homogeneity -- 5.2.6 Initial Conditions -- 5.2.7 Bottom-Up or Top-Down Structure Formation -- 5.3 Concluding Remarks -- CHAPTER 6. Subluminal Mass -- 6.1 Clusters of Galaxies -- 6.2 Groups of Galaxies -- 6.3 Galaxy Rotation Curves -- 6.3.1 The Andromeda Nebula -- 6.3.2 NGC 311525 -- 6.3.3 NGC 300 -- 6.3.4 NGC 2403 -- 6.3.5 The Burbidges's Program -- 6.3.6 Challenges -- 6.4 Stabilizing Spiral Galaxies -- 6.5 Recognizing Subluminal Matter -- 6.6 What Is the Nature of the Subluminal Matter? -- CHAPTER 7. Nonbaryonic Dark Matter -- 7.1 Hot Dark Matter -- 7.1.1 Apparent Detection of a Neutrino Rest Mass -- 7.2 Cold Dark Matter -- 7.2.1 What Happened in 1977 -- 7.2.2 The Situation in the Early 1980s -- 7.2.3 The Search for Dark Matter Detection -- CHAPTER 8. The Age of Abundance of Cosmological Models -- 8.1 Why Is the CMB So Smooth? -- 8.2 The Counterexample: CDM -- 8.3 CDM and Structure Formation -- 8.4 Variations on the Theme -- 8.4.1 TCDM -- 8.4.2 DDM and MDM -- 8.4.3 ΛCDM and τCDM -- 8.4.4 Other Thoughts -- 8.5 How Might It All Fit Together? -- CHAPTER 9. The 1998-2003 Revolution -- 9.1 The Redshift-Magnitude Test -- 9.2 The CMB Temperature Anisotropy -- 9.3 What Happened at the Turn of the Century -- 9.4 The Future of Physical Cosmology CHAPTER 10. The Ways of Research -- 10.1 Technology -- 10.2 Human Behavior -- 10.3 Roads Not Taken -- 10.4 The Social Construction of Science -- References -- Index -- Color Plates Cosmology Kosmologie (DE-588)4114294-9 gnd |
| subject_GND | (DE-588)4114294-9 |
| title | Cosmology's century an inside history of our modern understanding of the Universe |
| title_auth | Cosmology's century an inside history of our modern understanding of the Universe |
| title_exact_search | Cosmology's century an inside history of our modern understanding of the Universe |
| title_exact_search_txtP | Cosmology's century an inside history of our modern understanding of the Universe |
| title_full | Cosmology's century an inside history of our modern understanding of the Universe P.J.E. Peebles |
| title_fullStr | Cosmology's century an inside history of our modern understanding of the Universe P.J.E. Peebles |
| title_full_unstemmed | Cosmology's century an inside history of our modern understanding of the Universe P.J.E. Peebles |
| title_short | Cosmology's century |
| title_sort | cosmology s century an inside history of our modern understanding of the universe |
| title_sub | an inside history of our modern understanding of the Universe |
| topic | Cosmology Kosmologie (DE-588)4114294-9 gnd |
| topic_facet | Cosmology Kosmologie |
| work_keys_str_mv | AT peeblespje cosmologyscenturyaninsidehistoryofourmodernunderstandingoftheuniverse |