Cosmology's century: an inside history of our modern understanding of the Universe
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Buch |
| Sprache: | English |
| Veröffentlicht: |
Princeton ; Oxford
Princeton University Press
[2020]
|
| Schlagworte: | |
| Online-Zugang: | Inhaltsverzeichnis |
| Beschreibung: | Hier auch später erschienene, unveränderte Nachdrucke |
| Beschreibung: | xvii, 403 Seiten Illustrationen, Diagramme 24 cm |
| ISBN: | 9780691196022 9780691234472 |
Internformat
MARC
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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 xvii, 403 Seiten |b Illustrationen, Diagramme |c 24 cm | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b n |2 rdamedia | ||
| 338 | |b nc |2 rdacarrier | ||
| 500 | |a Hier auch später erschienene, unveränderte Nachdrucke | ||
| 648 | 7 | |a Geschichte 1917-2003 |2 gnd |9 rswk-swf | |
| 650 | 4 | |a bicssc / Astrophysics | |
| 650 | 4 | |a bicssc / History of science | |
| 650 | 4 | |a bisacsh / SCIENCE / Physics / Astrophysics | |
| 650 | 4 | |a bisacsh / SCIENCE / History | |
| 650 | 4 | |a Cosmology - History | |
| 650 | 0 | 7 | |a Kosmologie |0 (DE-588)4114294-9 |2 gnd |9 rswk-swf |
| 689 | 0 | 0 | |a Kosmologie |0 (DE-588)4114294-9 |D s |
| 689 | 0 | 1 | |a Geschichte 1917-2003 |A z |
| 689 | 0 | |5 DE-604 | |
| 776 | 0 | 8 | |i Erscheint auch als |n Online-Ausgabe |z 978-0-691-20166-5 |
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Datensatz im Suchindex
| _version_ | 1804181445674008576 |
|---|---|
| adam_text | CONTENTS
PREFACE
ANDACKNOWLEDGMENTS
XIII
CHAPTER
I
INTRODUCTION
1
I. I THE
SCIENCE
AND
PHILOSOPHY
OF
COSMOLOGY
2
1.2 AN
OVERVIEW
6
CHAPTER
2
THE
HOMOGENEOUS
UNIVERSE
12
2.1 EINSTEIN S
COSMOLOGICAL
PRINCIPLE
12
2.2 EARLY
EVIDENCE
OF
INHOMOGENEITY
16
2.3 EARLY
EVIDENCE
OF
HOMOGENEITY:
ISOTROPY
18
2.4 EARLY
EVIDENCE
OF
HOMOGENEITY:
COUNTS
AND
REDSHIFTS
22
2.5
THE
UNIVERSE
AS A
STATIONARY
RANDOM
PROCESS
25
2.6 A
FRACTAL
UNIVERSE 31
2.7
CONCLUDING
REMARKS 34
CHAPTER
3
COSMOLOGICAL
MODELS
3.1
DISCOVERY
OF
THE
RELATIVISTIC
36
EXPANDING
UNIVERSE
36
3.2
THE
RELATIVISTIC
BIG BANG COSMOLOGY
45
3.3
THE
STEADY-STATE
COSMOLOGY
50
3.4
EMPIRICALASSESSMENTS
OF
THE
STEADY-STATE COSMOLOGY
51
3.5
NONEMPIRICALASSESSMENTS
OF
THE
BIG BANG MODEL
56
3.5.1 EARLY THINKING
56
[VII]
$
B1IOTHEK
DEUTSCHES
MUSEUM
HLUENCHE A
[VIII]
CONTENTS
3.5.2
COSMOLOGICAL
INFLATION
3.5.3
BIASING
3.6
EMPIRICALASSESSMENTS
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
62
66
69
71
74
77
82
105
3.7
CONCLUDING
REMARKS
111
CHAPTER
4
FOSSILS: MICROWAVE
RADIATION
AND
LIGHT
ELEMENTS
114
4.1
THERMAL
RADIATION IN
AN
EXPANDING
UNIVERSE
115
4.2
GAMOW
SCENARIO
122
4.2.1
GAMOW S
1948
PAPERS
123
4.2.2
PREDICTING
THE
PRESENT CMB
TEMPERATURE
130
4.2.3
THE ALPHER,
BETHE,
AND
GAMOW
PAPER
133
4.3
HELIUM
AND
DEUTERIUM
FROM
THE
HOT BIG
BANG
139
4.3.1
RECOGNITION
OF
FOSSIL
HELIUM
139
4.3.2
HELIUM IN
A
COLD
UNIVERSE
143
4.3.3 DEVELOPMENTS IN
1964
AND
1965
146
4.4 SOURCES
OFMICROWAVE
RADIATION
151
4.4.1
INTERSTELLAR CYANOGEN
153
4.4.2
DETECTION
AT
BELL LABORATORIES
156
4.4.3
ZEL DOVICH S GROUP
158
CONTENTS
[1X]
4.4.4
DICKE S
GROUP
4.4.5
RECOGNITION
OF
THE
CMB
4.5 MEASURING
THE
CMB INTENSITY
160
162
SPECTRUM 164
4.5.1
THE
SITUATION
IN
THE
1970S
164
4.5.2
ALTERNATIVE
INTERPRETATIONS
166
4.5.3
THE
SUBMILLIMETER
ANOMALIES 169
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?
171
174
182
CHAPTER
5
HOW COSMIC
STRUCTURE
GREW
184
5.1
THE
GRAVITATIONAL
INSTABILITY
PICTURE 186
5.1.1
LEMAITRE S
SOLUTION
193
5.1.2
LIFSHITZ S
PERTURBATION
ANALYSES
198
5.1.3
NONGRAVITATIONAL
INTERACTION
OF
BARYONS
AND
THE
CMB 202
5.1.4
THE
JEANS
MASS 208
5.2 SCENARIOS
210
5.2.1
CHAOS
AND
ORDER 210
5.2.2
PRIMEVAL
TURBULENCE
213
5.2.3
GRAVITATIONAL ORIGIN
OF
GALAXY ROTATION
216
5.2.4
EXPLOSIONS
221
5.2.5 SPONTANEOUSLY
BROKEN
HOMOGENEITY
223
5.2.6 INITIAL
CONDITIONS
229
5.2.7 BOTTOM-UP
OR
TOP-DOWN
STRUCTURE
FORMATION
233
5.3 CONCLUDING REMARKS
236
[X]
CONTENTS
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 3115
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
239
240
245
247
248
255
257
258
260
260
265
272
276
279
280
A
NEUTRINO REST
MASS
285
7.2
COLD
DARK
MATTER
289
7.2.1 WHAT
HAPPENED IN
1977
290
7.2.2
THE SITUATION IN
THE
EARLY
1980S
295
7.2.3
THE SEARCH
FOR
DARK MATTER
DETECTION
297
CHAPTER
8
THE AGE
OF
ABUNDANCE
OF
COSMOLOGICAL
MODELS
300
8.1
WHY
IS
THE
CMB SO
SMOOTH?
301
8.2 THE
COUNTEREXAMPLE:
CDM
302
8.3 CDM
AND
STRUCTURE
FORMATION
307
8.4 VARIATIONS
ON
THE
THEME
311
8.4.1
TCDM
312
8.4.2
DDM
AND
MDM
313
CONTENTS
[XI]
8.4.3
ACDM
AND TCDM
8.4.4
OTHER THOUGHTS
8.5 HOW
MIGHT
ITALL FIT
TOGETHER?
314
315
316
CHAPTER
9
THE
1998-2003
REVOLUTION 323
9.1
THEREDSHIFT-MAGNITUDETEST
323
9.2 THE
CMB
TEMPERATUREANISOTROPY
332
9.3
WHAT
HAPPENED
AT
THE
TURN
OF
THE
CENTURY
335
9.4
THE
FUTURE
OF
PHYSICAL
COSMOLOGY
340
CHAPTER
10
THE WAYS
OF
RESEARCH
343
10.1 TECHNOLOGY
343
10.2 HUMAN
BEHAVIOR
344
10.3 ROADS
NOT
TAKEN
345
10.4 THE
SOCIAL
CONSTRUCTION
OF
SCIENCE
348
REFERENCES
355
INDEX
399
|
| adam_txt |
CONTENTS
PREFACE
ANDACKNOWLEDGMENTS
"
XIII
CHAPTER
I
INTRODUCTION
1
I. I THE
SCIENCE
AND
PHILOSOPHY
OF
COSMOLOGY
2
1.2 AN
OVERVIEW
6
CHAPTER
2
THE
HOMOGENEOUS
UNIVERSE
12
2.1 EINSTEIN'S
COSMOLOGICAL
PRINCIPLE
12
2.2 EARLY
EVIDENCE
OF
INHOMOGENEITY
16
2.3 EARLY
EVIDENCE
OF
HOMOGENEITY:
ISOTROPY
18
2.4 EARLY
EVIDENCE
OF
HOMOGENEITY:
COUNTS
AND
REDSHIFTS
22
2.5
THE
UNIVERSE
AS A
STATIONARY
RANDOM
PROCESS
25
2.6 A
FRACTAL
UNIVERSE 31
2.7
CONCLUDING
REMARKS 34
CHAPTER
3
COSMOLOGICAL
MODELS
3.1
DISCOVERY
OF
THE
RELATIVISTIC
36
EXPANDING
UNIVERSE
36
3.2
THE
RELATIVISTIC
BIG BANG COSMOLOGY
45
3.3
THE
STEADY-STATE
COSMOLOGY
50
3.4
EMPIRICALASSESSMENTS
OF
THE
STEADY-STATE COSMOLOGY
51
3.5
NONEMPIRICALASSESSMENTS
OF
THE
BIG BANG MODEL
56
3.5.1 EARLY THINKING
56
[VII]
$
B1IOTHEK
DEUTSCHES
MUSEUM
'
HLUENCHE'A
[VIII]
CONTENTS
3.5.2
COSMOLOGICAL
INFLATION
3.5.3
BIASING
3.6
EMPIRICALASSESSMENTS
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
62
66
69
71
74
77
82
105
3.7
CONCLUDING
REMARKS
111
CHAPTER
4
FOSSILS: MICROWAVE
RADIATION
AND
LIGHT
ELEMENTS
114
4.1
THERMAL
RADIATION IN
AN
EXPANDING
UNIVERSE
115
4.2
GAMOW'
SCENARIO
122
4.2.1
GAMOW'S
1948
PAPERS
123
4.2.2
PREDICTING
THE
PRESENT CMB
TEMPERATURE
130
4.2.3
THE ALPHER,
BETHE,
AND
GAMOW
PAPER
133
4.3
HELIUM
AND
DEUTERIUM
FROM
THE
HOT BIG
BANG
139
4.3.1
RECOGNITION
OF
FOSSIL
HELIUM
139
4.3.2
HELIUM IN
A
COLD
UNIVERSE
143
4.3.3 DEVELOPMENTS IN
1964
AND
1965
146
4.4 SOURCES
OFMICROWAVE
RADIATION
151
4.4.1
INTERSTELLAR CYANOGEN
153
4.4.2
DETECTION
AT
BELL LABORATORIES
156
4.4.3
ZEL'DOVICH'S GROUP
158
CONTENTS
[1X]
4.4.4
DICKE'S
GROUP
4.4.5
RECOGNITION
OF
THE
CMB
4.5 MEASURING
THE
CMB INTENSITY
160
162
SPECTRUM 164
4.5.1
THE
SITUATION
IN
THE
1970S
164
4.5.2
ALTERNATIVE
INTERPRETATIONS
166
4.5.3
THE
SUBMILLIMETER
ANOMALIES 169
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?
171
174
182
CHAPTER
5
HOW COSMIC
STRUCTURE
GREW
184
5.1
THE
GRAVITATIONAL
INSTABILITY
PICTURE 186
5.1.1
LEMAITRE'S
SOLUTION
193
5.1.2
LIFSHITZ'S
PERTURBATION
ANALYSES
198
5.1.3
NONGRAVITATIONAL
INTERACTION
OF
BARYONS
AND
THE
CMB 202
5.1.4
THE
JEANS
MASS 208
5.2 SCENARIOS
210
5.2.1
CHAOS
AND
ORDER 210
5.2.2
PRIMEVAL
TURBULENCE
213
5.2.3
GRAVITATIONAL ORIGIN
OF
GALAXY ROTATION
216
5.2.4
EXPLOSIONS
221
5.2.5 SPONTANEOUSLY
BROKEN
HOMOGENEITY
223
5.2.6 INITIAL
CONDITIONS
229
5.2.7 BOTTOM-UP
OR
TOP-DOWN
STRUCTURE
FORMATION
233
5.3 CONCLUDING REMARKS
236
[X]
CONTENTS
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 3115
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
239
240
245
247
248
255
257
258
260
260
265
272
276
279
280
A
NEUTRINO REST
MASS
285
7.2
COLD
DARK
MATTER
289
7.2.1 WHAT
HAPPENED IN
1977
290
7.2.2
THE SITUATION IN
THE
EARLY
1980S
295
7.2.3
THE SEARCH
FOR
DARK MATTER
DETECTION
297
CHAPTER
8
THE AGE
OF
ABUNDANCE
OF
COSMOLOGICAL
MODELS
300
8.1
WHY
IS
THE
CMB SO
SMOOTH?
301
8.2 THE
COUNTEREXAMPLE:
CDM
302
8.3 CDM
AND
STRUCTURE
FORMATION
307
8.4 VARIATIONS
ON
THE
THEME
311
8.4.1
TCDM
312
8.4.2
DDM
AND
MDM
313
CONTENTS
[XI]
8.4.3
ACDM
AND TCDM
8.4.4
OTHER THOUGHTS
8.5 HOW
MIGHT
ITALL FIT
TOGETHER?
314
315
316
CHAPTER
9
THE
1998-2003
REVOLUTION 323
9.1
THEREDSHIFT-MAGNITUDETEST
323
9.2 THE
CMB
TEMPERATUREANISOTROPY
332
9.3
WHAT
HAPPENED
AT
THE
TURN
OF
THE
CENTURY
335
9.4
THE
FUTURE
OF
PHYSICAL
COSMOLOGY
340
CHAPTER
10
THE WAYS
OF
RESEARCH
343
10.1 TECHNOLOGY
343
10.2 HUMAN
BEHAVIOR
344
10.3 ROADS
NOT
TAKEN
345
10.4 THE
SOCIAL
CONSTRUCTION
OF
SCIENCE
348
REFERENCES
"
355
INDEX
"
399 |
| any_adam_object | 1 |
| any_adam_object_boolean | 1 |
| author | Peebles, P. J. E. 1935- |
| author_GND | (DE-588)140955194 |
| author_facet | Peebles, P. J. E. 1935- |
| author_role | aut |
| author_sort | Peebles, P. J. E. 1935- |
| author_variant | p j e p pje pjep |
| building | Verbundindex |
| bvnumber | BV046711804 |
| classification_rvk | UB 2484 |
| ctrlnum | (OCoLC)1164609634 (DE-599)BVBBV046711804 |
| discipline | Physik |
| discipline_str_mv | Physik |
| era | Geschichte 1917-2003 gnd |
| era_facet | Geschichte 1917-2003 |
| format | Book |
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| id | DE-604.BV046711804 |
| illustrated | Illustrated |
| index_date | 2024-07-03T14:31:03Z |
| indexdate | 2024-07-10T08:51:46Z |
| institution | BVB |
| isbn | 9780691196022 9780691234472 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-032122188 |
| oclc_num | 1164609634 |
| open_access_boolean | |
| owner | DE-29T DE-706 DE-12 DE-19 DE-BY-UBM DE-210 DE-355 DE-BY-UBR |
| owner_facet | DE-29T DE-706 DE-12 DE-19 DE-BY-UBM DE-210 DE-355 DE-BY-UBR |
| physical | xvii, 403 Seiten Illustrationen, Diagramme 24 cm |
| 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 xvii, 403 Seiten Illustrationen, Diagramme 24 cm txt rdacontent n rdamedia nc rdacarrier Hier auch später erschienene, unveränderte Nachdrucke Geschichte 1917-2003 gnd rswk-swf bicssc / Astrophysics bicssc / History of science bisacsh / SCIENCE / Physics / Astrophysics bisacsh / SCIENCE / History Cosmology - History Kosmologie (DE-588)4114294-9 gnd rswk-swf Kosmologie (DE-588)4114294-9 s Geschichte 1917-2003 z DE-604 Erscheint auch als Online-Ausgabe 978-0-691-20166-5 Digitalisierung Deutsches Museum application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=032122188&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
| spellingShingle | Peebles, P. J. E. 1935- Cosmology's century an inside history of our modern understanding of the Universe bicssc / Astrophysics bicssc / History of science bisacsh / SCIENCE / Physics / Astrophysics bisacsh / SCIENCE / History Cosmology - History 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 | bicssc / Astrophysics bicssc / History of science bisacsh / SCIENCE / Physics / Astrophysics bisacsh / SCIENCE / History Cosmology - History Kosmologie (DE-588)4114294-9 gnd |
| topic_facet | bicssc / Astrophysics bicssc / History of science bisacsh / SCIENCE / Physics / Astrophysics bisacsh / SCIENCE / History Cosmology - History Kosmologie |
| url | http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=032122188&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA |
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