소장자료
LDR | 07070cam a2200000 a | ||
001 | 0100723603▲ | ||
005 | 20230824171225▲ | ||
007 | ta ▲ | ||
008 | 221207t20222020njuaf b 001 0 eng c▲ | ||
020 | ▼a9780691234472▼q(pbk.)▲ | ||
020 | ▼a0691234477▼q(pbk.)▲ | ||
020 | ▼a9780691196022▼q(hbk.)▲ | ||
020 | ▼a0691196028▼q(hbk.)▲ | ||
035 | ▼a(KERIS)REF000020105931▲ | ||
040 | ▼aYDX▼beng▼cYDX▼dBDX▼dUKMGB▼dOCLCO▼dOCLCF▼dTOH▼dOCLCQ▼dERASA▼dCDX▼dCOH▼dPAU▼dWAU▼dOCLCO▼dOCLCQ▼dIL4J6▼dOCLCO▼dDLC▼d221016▲ | ||
042 | ▼apcc▲ | ||
050 | 0 | 0 | ▼aQB981▼b.P419 2020▲ |
082 | 0 | 4 | ▼a523.1▼223▲ |
090 | ▼a523.1▼bP373c▲ | ||
100 | 1 | ▼aPeebles, P. J. E.▼q(Phillip James Edwin),▼eauthor.▲ | |
245 | 1 | 0 | ▼aCosmology's century :▼ban inside history of our modern understanding of the universe /▼cP. J. E. Peebles.▲ |
260 | ▼aPrinceton ;▼aOxford :▼bPrinceton University Press,▼c[2020]▲ | ||
300 | ▼axvii, 403 p., viii p. of plates :▼bill. (some col.) ;▼c24 cm▲ | ||
504 | ▼aIncludes bibliographical references (p. 355-398) and index.▲ | ||
505 | 0 | 0 | ▼gChapter 1: Introduction. 1.1.▼tThe science and philosophy of cosmology ;▼g1.2. An overview ; --▼gChapter 2.▼tThe homogeneous universe▼g2.1.▼tEinstein's Cosmological principle ;▼g2.2.▼tEarly evidence of Inhomogeneity ;▼g2.3.▼tEarly evidence of homogeneity : isotropy ;▼g2.4.▼tEarly evidence of homogeneity : counts and redshifts ;▼g2.5.▼tThe universe as a stationary random process ;▼g2.6.▼tA fractal universe ;▼g2.7. Concluding remarks --▼gChapter 3:▼tCosmological Models.▼g3.1.▼tDiscovery of the relativistic expanding universe ;▼g3.2.▼tThe relativistic big bang cosmology ;▼g3.3.▼tThe steady-state cosmology ;▼g3.4.▼tEmpirical assessments of the steady-ttate cosmology ;▼g3.5.▼tNonempirical assessments of the big bang model ;▼g3.5.1▼tEarly thinking ;▼g3.5.2.▼tCosmological inflation ;▼g3.5.3.▼tBiasing ;▼g3.6.▼tEmpirical assessments of the big bang model ;▼g3.6.1.▼tTime scales ;▼g3.6.2.▼tCosmological tests in the 1970s ;▼g3.6.3.▼tMass density measurements : Introduction ;▼g3.6.4.▼tMass density measurements : Hubble to the revolution ;▼g3.6.5.▼tMass density measurements : assessments ;▼g3.7. Concluding remarks --▼gChapter 4:▼tFossils : microwave radiation and light elements:▼g4.1.▼tThermal radiation in an expanding universe ;▼g4.2.▼tGamow's scenario ;▼g4.2.1.▼tGamow's 1948 papers ;▼g4.2.2.▼tPredicting the present CMB temperature ;▼g4.2.3.▼tThe Alpher, Bethe and Gamow paper ;▼g4.3.▼tHelium and deuterium from the hot big bang ;▼g4.3.1.▼tRecognition of fossil helium ;▼g4.3.2.▼tHelium in a cold universe ;▼g4.3.3.▼tDevelopments in 1964-1965 ;▼g4.4.▼tSources of microwave radiation ;▼g4.4.1.▼tInterstellar cyanogen ;▼g4.4.2.▼tDetection at Bell Laboratories ;▼g4.4.3.▼tZel'dovich's Group ;▼g4.4.4.▼tDicke's Group ;▼g4.4.5.▼tRecognition of the CMB ;▼g4.5 Measuring the CMB intensity spectrum ;▼g4.5.1.▼tThe situation in the 1970s ;▼g4.5.2.▼tAlternative interpretations ;▼g4.5.3.▼tThe submillimeter anomalies ;▼g4.5.4.▼tEstablishing the CMB thermal spectrum ;▼g4.6 Nucleosynthesis and the Baryon Mass Density ;▼g4.7.▼tWhy Was the Hot Big Bang Cosmology reinvented? --▼gChapter 5 How cosmic structure grew ;▼g5.1.▼tThe gravitational instability picture ;▼g5.1.1.▼tLemaître's solution ;▼g5.1.2.▼tLifshitz's perturbation analyses ;▼g5.1.3.▼tNongravitational interaction of Baryons and the CMB ;▼g5.1.4.▼tThe Jeans Mass ;▼g5.2.▼tScenarios ;▼g5.2.1.▼tChaos and Order ;▼g5.2.2 Primeval turbulence ;▼g5.2.3.▼tGravitational origin of galaxy rotation ;▼g5.2.4.▼tExplosions ;▼g5.2.5 Spontaneously broken homogeneity ;▼g5.2.6.▼tInitial conditions ;▼g5.2.7.▼tBottom-up or top-down structure formation ;▼g5.3. Concluding remarks ; --▼gChapter 6:▼tSubliminal mass ;▼g6.1.▼tClusters of galaxies ;▼g6.2.▼tGroups of galaxies ;▼g6.3.▼tGalaxy rotation curves ;▼g6.3.1.▼tThe Andromeda nebula ;▼g6.3.2 NGC3115 ;▼g6.3.3.▼tNGC 300 ;▼g6.3.4 NGC 2403 ;▼t6.3.5.▼tThe Burbidges's Program ;▼g6.3.6 Challenges ;▼g6.4.▼tStabilizing spiral galaxies ;▼g6.5.▼tRecognizing Subluminal Matter ;▼g6.6 What is the nature of the subluminal matter? ; --▼gChapter 7.▼tNonbaryonic Dark Matter ;▼g7.1.▼tHot dark matter ;▼g7.1.1.▼tApparent Detection of a Neutrino Rest Mass ;▼g7.2.▼tCold dark matter ;▼g7.2.1.▼tWhat happened in 1977 ;▼g7.2.2.▼tThe situation in the early 1980s ;▼g7.2.3.▼tThe search for dark matter Detection ; --▼gChapter 8.▼tThe age of abundance of cosmological Models ;▼g8.1.▼tWhy is the CMB So Smooth? ;▼g8.2.▼tThe counterexample : CDM ;▼g8.3.▼tCDM and structure formation ;▼g8.4.▼tVariations on the theme ;▼t8.4.1.▼tTCDM ;▼g8.4.2.▼tDDM and MDM ;▼t8.4.3 ACDM and CDM ;▼t8.4.4.▼tOther thoughts ;▼g8.5.▼tHow might it all fit together? --▼gChapter 9.▼tThe 1998-2003 Revoution:▼g9.1.▼tThe Redshift-Magnitude Test ;▼g9.2 The CMB temperature anisotropy ;▼g9.3.▼tWhat happened at the turn of the century ;▼g9.4.▼tThe future of physical cosmology --▼gChapter 10.▼tThe ways of research:▼g10.1.▼ttechnology ;▼g10.2▼tHuman behavior ;▼g10.3 Roads Not Taken ;▼g10.4.▼tThe social construction of science.▲ |
520 | ▼a"From Nobel Prize-winning physicist P.J.E. Peebles, the story of cosmology from Einstein to today. Modern cosmology began a century ago with Albert Einstein's general theory of relativity and his notion of a homogenous, philosophically satisfying cosmos. Cosmology's Century is the story of how generations of scientists built on these thoughts and many new measurements to arrive at a well-tested physical theory of the structure and evolution of our expanding universe. In this landmark book, one of the world's most esteemed theoretical cosmologists offers an unparalleled personal perspective on how the field developed. P.J.E. Peebles was at the forefront of many of the greatest discoveries of the past century, making fundamental contributions to our understanding of the presence of helium and microwave radiation from the hot big bang, the measures of the distribution and motion of ordinary matter, and the new kind of dark matter that allows us to make sense of these results. Taking readers from the field's beginnings, Peebles describes how scientists working in independent directions found themselves converging on a theory of cosmic evolution interesting enough to warrant the rigorous testing it passes so well. He explores the major advances--some inspired by remarkable insights or perhaps just lucky guesses--as well as the wrong turns taken and the roads not explored. He shares recollections from major players in this story and provides a rare, inside look at how natural science is really done. A monumental work, Cosmology's Century also emphasizes where the present theory is incomplete, suggesting exciting directions for continuing research"--Amazon▲ | ||
650 | 0 | ▼aCosmology▼xHistory.▲ |
Cosmology's century : an inside history of our modern understanding of the universe
자료유형
국외단행본
서명/책임사항
Cosmology's century : an inside history of our modern understanding of the universe / P. J. E. Peebles.
개인저자
Peebles, P. J. E. (Phillip James Edwin)
발행사항
Princeton ; Oxford : Princeton University Press , [2020]
형태사항
xvii, 403 p., viii p. of plates : ill. (some col.) ; 24 cm
서지주기
Includes bibliographical references (p. 355-398) and index.
내용주기
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-ttate 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 1964-1965 ; 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 : Subliminal 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 NGC3115 ; 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 ACDM and CDM ; 8.4.4. Other thoughts ; 8.5. How might it all fit together? -- Chapter 9. The 1998-2003 Revoution : 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.
요약주기
"From Nobel Prize-winning physicist P.J.E. Peebles, the story of cosmology from Einstein to today. Modern cosmology began a century ago with Albert Einstein's general theory of relativity and his notion of a homogenous, philosophically satisfying cosmos. Cosmology's Century is the story of how generations of scientists built on these thoughts and many new measurements to arrive at a well-tested physical theory of the structure and evolution of our expanding universe. In this landmark book, one of the world's most esteemed theoretical cosmologists offers an unparalleled personal perspective on how the field developed. P.J.E. Peebles was at the forefront of many of the greatest discoveries of the past century, making fundamental contributions to our understanding of the presence of helium and microwave radiation from the hot big bang, the measures of the distribution and motion of ordinary matter, and the new kind of dark matter that allows us to make sense of these results. Taking readers from the field's beginnings, Peebles describes how scientists working in independent directions found themselves converging on a theory of cosmic evolution interesting enough to warrant the rigorous testing it passes so well. He explores the major advances--some inspired by remarkable insights or perhaps just lucky guesses--as well as the wrong turns taken and the roads not explored. He shares recollections from major players in this story and provides a rare, inside look at how natural science is really done. A monumental work, Cosmology's Century also emphasizes where the present theory is incomplete, suggesting exciting directions for continuing research"--Amazon
ISBN
9780691234472 0691234477 9780691196022 0691196028
청구기호
523.1 P373c
소장정보
예도서예약
서서가에없는책 신고
보보존서고신청
캠캠퍼스대출
우우선정리신청
배자료배달신청
문문자발송
출청구기호출력
학소장학술지 원문서비스
등록번호 | 청구기호 | 소장처 | 도서상태 | 반납예정일 | 서비스 |
---|
북토크
자유롭게 책을 읽고
느낀점을 적어주세요
글쓰기
느낀점을 적어주세요
청구기호 브라우징
관련 인기대출 도서