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04508cam a2200481Ki 4500
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20210114162426
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200204s2020 njua fo 000 0 eng d
▼a 9780691201665
▼q electronic book
▼a 0691201668
▼q electronic book
▼z 9780691196022
▼q hardcover
▼a 2324244
▼b (N$T)
▼a (OCoLC)1152229023
▼a 22573/ctvssj6jx
▼b JSTOR
▼a UKAHL
▼b eng
▼e rda
▼c UKAHL
▼d OCLCO
▼d EBLCP
▼d JSTOR
▼d N$T
▼d YDX
▼d YDXIT
▼d 248023
▼a QB981
▼b .P44 2020
▼a 523.1
▼2 23
▼a Peebles, P. J. E.
▼q (Phillip James Edwin),
▼e author.
▼a Cosmology's century:
▼b an inside history of our modern understanding of the Universe /:
▼c P.J.E. Peebles.
▼a Princeton:
▼b Princeton University Press,
▼c 2020.
▼a 1 online resource:
▼b illustrations.
▼a text
▼b txt
▼2 rdacontent
▼a computer
▼b c
▼2 rdamedia
▼a online resource
▼b cr
▼2 rdacarrier
▼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
▼a 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
▼a 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
▼a 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
▼a 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
▼a Master record variable field(s) change: 050
▼a Cosmology
▼x History.
▼a Electronic books.
▼a Electronic books.
▼3 EBSCOhost
▼u http://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&db=nlabk&AN=2324244
▼a YBP Library Services
▼b YANK
▼n 16584683
▼a ProQuest Ebook Central
▼b EBLB
▼n EBL6214864
▼a Askews and Holts Library Services
▼b ASKH
▼n AH37347566
▼a EBSCOhost
▼b EBSC
▼n 2324244
▼a 강리원
▼a eBook
▼a 92
▼b N$T
| 자료유형 : | eBook |
|---|---|
| ISBN : | 9780691201665 |
| ISBN : | 0691201668 |
| ISBN : | |
| 개인저자 : | Peebles, P. J. E. (Phillip James Edwin), author. |
| 서명/저자사항 : | Cosmology's century: an inside history of our modern understanding of the Universe /: P.J.E. Peebles. |
| 발행사항 : | Princeton: Princeton University Press, 2020. |
| 형태사항 : | 1 online resource: illustrations. |
| 내용주기 : | 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 |
| 내용주기 : | 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 |
| 내용주기 : | 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 |
| 내용주기 : | 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 |
| 내용주기 : | 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 |
| 일반주제명 : | Cosmology -- History. -- |
| 언어 | 영어 |
| URL : |
|---|
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