The deep universe: lecture notes 1993
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| Format: | Conference Proceeding Book |
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| Language: | English |
| Published: |
Berlin [u.a.]
Springer
1995
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| Item Description: | Literaturangaben |
| Physical Description: | XIV, 526 S. graph. Darst. |
| ISBN: | 3540589139 |
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| 245 | 1 | 0 | |a The deep universe |b lecture notes 1993 |c Saas Fee Advanced Course 23. A. R. Sandage ; R. G. Kron ; M. S. Longair. Swiss Society for Astrophysics and Astronomy. Ed. by B. Binggeli ... |
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| adam_text | Contents
Practical Cosmology: Inventing the Past
By Allan Sandage
Preface
................................................... 1
1
Introduction to the Standard Model
..................... 3
1.1
Scope of the Subject
................................... 3
1.2
The Hall of Fame
...................................... 6
1.3
Example of Simplicity: The Luminosity Density of Shining
Baryons:
A Study in Methods
........................... 7
1.4
Experimental Geometry: Introduction to Curved Spaces
.... 8
1.5
The Four Standard Tests of Classical Cosmology
.......... 12
1.6
The Classical Standard Model
.......................... 13
2
The First Tests The Count-Magnitude Relation;
Theory and Practice I (The Early Phase
1920-1938) ..... 24
2.1
Theory of the Count-Magnitude Relation in Parametric
Form
................................................ 24
2.2
N(m, go) Is Degenerate to
z
in First Order While N(z, qo)
Is Not
............................................... 26
2.3
Hubble s
1926-1934
Galaxy Count Program
.............. 28
2.4
Hubble s Program to Find Space Curvature from Galaxy
Counts
............................................... 30
2.5
Why Hubble s Program Failed
.......................... 34
3
The Count—Magnitude Relation:
Theory and Practice
Π
(The Modern Attempts)
......... 41
3.1
The Realistic N(m) Test
............................... 41
3.2
The N{m) Data
....................................... 53
3.3
Calculation of the N(z,q0) Distribution
................... 58
3.4
Comparing the N(m, qo) and the N(z, go) Distributions for
Consistency
........................................... 64
4
The Second Test: Angular Size
=
f(z, q0)
................. 73
4.0
Introduction
.......................................... 73
4.1
The Very Local Redshift-Angular Diameter Test
.......... 73
4.2
General Theory of Angular Diameter
=
f(z,q0) Valid for
All Redshifts
.......................................... 75
4.3
Predictions for a Tired Light Model
.................... 78
VIII
4.4
The Difference Between Metric and Isophotal Diameters
.... 79
4.5
Samples of Angular Size-Redshift Data
.................. 80
4.6
Kellermann s Data on Compact Radio Sources
............ 87
5
The Third Test: The Redshift-Distance Relation
Based on the m(z, qo) Hubble Diagram
................... 91
5.0
Introduction
.......................................... 91
5.1
Expected Form
........................................ 91
5.2
The Early Observations
1927-1936 ...................... 97
5.3
The
Palomar
Program
1953-1980 ........................ 106
5.4
Expected Hubble m(qoj z) Diagram at Arbitrarily Large
Redshift
..............................................
Ill
5.5
The Observational Search for qo Via the Hubble Diagram
... 114
5.6
The Local Velocity Field
............................... 118
6
Is the Expansion Real?
.................................. 127
6.1
History
.............................................. 127
6.2
Preliminaries to the
Tolman
Surface Brightness Test
....... 129
6.3
Selective Effects for a Practical
Tolman
Test
.............. 137
6.4
Result of a
1991
Attempt at the
Tolman
Test
............. 142
7
The Fourth Test: Timing (Age of the Galaxy)
........... 147
7.1
Theory of the Test
..................................... 147
7.2
The Road to Understanding the
Н
-R
Diagram
............ 148
7.3
Absolute Magnitude of RR Lyrae Stars from Pulsation
Properties
............................................ 162
7.4
Age of the Galaxy and the Universe Using Globular
Clusters
.............................................. 166
8
Timing Test Continued (The Hubble Constant)
.......... 170
8.1
Historical Resume
..................................... 170
8.2
Crime, Chess, and the Philosophy of False Clues in Puzzles
. 172
8.3
Seven Astronomical Ways to Ho
......................... 175
8.4
Cepheid Distances to the Local Calibrators
............... 183
8.5
Six Methods to Obtain the Distance of the Virgo Cluster
... 184
8.6
The Value of Ho
...................................... 188
8.7
The Timing Test
...................................... 189
9
The Hubble Constant from Type
Ia Supernovae
......... 192
9.1
Introduction
.......................................... 192
9.2
The Hubble Diagram Circa
1994 ........................ 194
9.3
Absolute Calibration of M(max) for
SNe
la
............... 200
9.4
Ho and the
Cosmologica!
Timing Test
.................... 207
10
Observational Selection Bias
............................. 210
10.1
Observational Selection Bias in the Hubble Diagrams of
Sbl and
Sci
Galaxies
___.............................. 210
IX
10.2
The Spaenhauei Diagram
............................... 213
10.3
The SD Applied to Real Data
........................... 215
10.4
The
Malmquist
Mo
-
(M(rn)) Calculation
................ 217
10.5
The Hubble Constant Does Not Increase Outward
......... 223
10.6
Selection Bias in the Tully-Fisher Method
................ 225
10.7
The Hubble Constant from the TF Method Using a
Distance-Limited Field Galaxy Sample
................... 229
Evolution in the Galaxy Population
By Richard G. Kron
1
Foundations of Galaxy Evolution Models
................ 233
1.1
Introduction
.......................................... 233
1.2
Cosmology and Evolution
.............................. 233
1.3
Star Light
............................................ 236
1.4
The Star-Formation Rate and the Initial Mass Function
.... 238
2
Evolutionary Synthesis Models
.......................... 242
2.1
Evolutionary Synthesis Models
.......................... 242
2.2
Evolution of the Solar Neighborhood
..................... 244
2.3
Effect of the
IntersteĽar
Medium
........................ 247
2.4
Other Disk Galaxy Models
............................. 248
2.5
Single-Generation Models
.............................. 249
2.6
Summary
............................................. 250
3
Basic Statistics of Galaxies
.............................. 252
3.1
Giant Galaxies
........................................ 252
3.2
Dwarf Galaxies
........................................ 254
3.3
Distribution Functions
................................. 255
4
Computing Models for Faint-Galaxy Samples
............ 263
4.1
Effect of Redshift
...................................... 263
4.2
Model Input Parameters
............................... 264
4.3
Time Scales
.......................................... 265
4.4
Modeling the Count Distribution
........................ 266
4.5
Selection Effects
....................................... 268
4.6
Approximate Analytic Form for the fc-Correction
.......... 270
5
Distant Galaxy Observations in the Real World
......... 273
5.1
Detection Model
...................................... 273
5.2
Signal-to-Noise Ratio as a Function of Redshift
............ 275
5.3
Other Aspects of Faint-Object Detection
................. 278
β
Galaxy Profiles at High Redshift
........................ 281
6.1
Calculating Apparent Sizes and Surface Brightnesses
....... 281
6.2
Evolution and Cosmology
.............................. 284
6.3
Petrosian s Formulation
................................ 285
6.4
Selection by
Signał-to-Noise
Ratio
....................... 287
7
Reconciling Counts with the Redshift Distribution
...... 289
7.1
Statement of the Problem
.............................. 289
7.2
The Count Distribution
................................ 291
7.3
The Redshift Distribution.
.............................. 292
7.4
The Color Distribution
................................. 295
8
The Butcher-Oemler Effect
-
A Case Study
............. 299
8.1
A Collection of Concerns
............................... 300
8.2
A Rogue s Gallery
..................................... 301
8.3
Galaxy Morphological Types
............................ 303
9
Deep-Universe Programs for the Future
................. 307
9.1
Galaxy Rotation Curves at High Redshift
................ 307
9.2
Adaptive Optics Imaging of Distant Galaxies
............. 310
9.3
Detection of Distant
Supernovae
........................ 313
9.4
Jf-Band Imaging in Antarctica
.......................... 314
The Physics of Background Radiation
By Malcolm S. Longair
1
Observations of the Extragalactic Background Radiation
317
1.1
A Prospectus
......................................... 317
1.2
Recommended Reading
................................ 319
1.3
Observations of the Extragalactic Background Radiation
-
An Overview
......................................... 320
1.4
The Radio Background Radiation
....................... 323
1.5
The Cosmic Microwave Background Radiation
............ 327
1.6
The Infrared Background Radiation
..................... 331
1.7
The Optical Background Radiation
...................... 334
1.8
The Ultraviolet Background Radiation
................... 339
1.9
The X-ray Background Radiation
........................ 342
1.10
The 7-ray Background Radiation
........................ 343
1.11
Summary
............................................. 346
2
The Robertson-Walker Metric
........................... 350
2.1
The Isotropy of the Universe
............................ 350
2.2
The Homogeneity of the Universe and Hubble s Law
....... 356
2.3 Isotropie
Curved Spaces
................................ 360
2.4
The Robertson-Walker Metric
........................... 364
2.5
Observations in Cosmology
............................. 367
2.6
Conclusion
........................................... 374
XI
3
World Models
........................................... 376
3.1
Experimental and Observational Tests of General Relativity
376
3.2
The Einstein Field Equations
........................... 380
3.3
The Standard Dust Models
-
The Friedman World Models
. 381
3.4
Testing the Friedman Models
........................... 387
3.5
Radiation Dominated Universes
......................... 389
3.6
Inflationary Models
.................................... 391
4
Number Counts and the Background Radiation
.......... 396
4.1
Number Counts of Discrete Sources
...................... 396
4.2
The Background Radiation
............................. 400
4.3
The Effects of Evolution
-
The Case of the Radio
Background Emission
.................................. 402
4.4
The Background Radiation and the Source Counts
......... 405
4.5
Fluctuations in the Background Radiation due to Discrete
Sources
.............................................. 405
5
The Origin of the X-ray and Gamma-ray Backgrounds
... 412
5.1
The Origin of the Soft X-ray Background:
0.5-2
keV
....... 412
5.2
The X-ray Background Radiation:
2-100
keV
............. 415
5.3
The Gamma-ray Background
........................... 422
6
A Brief Thermal History of the Universe
................ 426
6.1
The Matter and Radiation Content of the Universe
........ 426
6.2
The Epoch of Recombination
........................... 427
6.3
The Epoch of Equality of Matter and Radiation
Inerţial
Mass Densities
........................................ 428
6.4
Early Epochs
......................................... 431
6.5
Nucleosynthesis in the Early Universe
.................... 432
7
The Origin of the Large-Scale Structure of the Universe
. 440
7.1
The Non-relativistic Wave Equation for the Growth of
Small Perturbations in the Expanding Universe
........... 441
7.2
The Jeans Instability
.................................. 443
7.3
The Jeans Instability in an Expanding Medium
........... 444
7.4
The Basic Problem
.................................... 451
7.5
The Evolution of Adiabatic Baryonic Fluctuations in the
Standard Hot Big Bang
................................ 452
7.6
Dissipation Processes in the Pre-Recombination Phases of
the Hot Big Bang
..................................... 455
7.7
Baryonic Pancake Theory
.............................. 456
7.8
Concluding Remarks
................................... 458
8
Dark Matter and Galaxy Formation
..................... 460
8.1
Introduction
.......................................... 460
8.2
Forms of Dark Matter
.................................. 461
8.3
Instabilities in the Presence of Dark Matter
............... 464
XII
8.4
The Evolution of Hot and Cold Dark Matter Perturbations
. 466
8.5
How Well Do the Models Work?
......................... 468
9
Fluctuations in the Cosmic Microwave Background
Radiation
................................................ 473
9.1
The
Ionisation
of the Intergalactic Gas Through the Epoch
of Recombination
...................................... 473
9.2
Fluctuations in the Background Radiation due to
Large-Scale Density Perturbations
....................... 474
9.3
Comparison with Observations
.......................... 479
9.4
Other Sources of Fluctuations
........................... 481
10
The Intergalactic Gas
.................................... 484
10.1
The Background Emission of and Absorption by the
Intergalactic Gas
...................................... 484
10.2
The Gunn-Peterson Test
............................... 485
10.3
The
Collisione!
Excitation of the Intergalactic Gas
......... 487
10.4
Quasar Absorption Lines and the Diffuse Intergalactic
Fai
Ultraviolet Background Radiation
....................... 489
10.5
The Luke-Warm Intergalactic Gas
....................... 493
10.6
The Lyman Continuum Opacity of the Intergalactic Gas
... 496
11
Galaxy Formation and the Background Radiation
....... 500
11.1
When Were the Heavy Elements Formed?
................ 500
11.2
The Lilly and Cowie Argument
.......................... 500
11.3
Submillimetre Cosmology
............................... 504
11.4
The Millimetre Background Radiation and Galaxy
Formation
............................................ 507
11.5
Results and Conclusions
................................ 511
|
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| spelling | The deep universe lecture notes 1993 Saas Fee Advanced Course 23. A. R. Sandage ; R. G. Kron ; M. S. Longair. Swiss Society for Astrophysics and Astronomy. Ed. by B. Binggeli ... Berlin [u.a.] Springer 1995 XIV, 526 S. graph. Darst. txt rdacontent n rdamedia nc rdacarrier Literaturangaben Kosmologie (DE-588)4114294-9 gnd rswk-swf (DE-588)1071861417 Konferenzschrift 1993 Les Diablerets gnd-content Kosmologie (DE-588)4114294-9 s DE-604 Sandage, Allan 1926-2010 Sonstige (DE-588)141345500 oth Kron, Richard G. Sonstige oth Longair, Malcolm 1941- Sonstige (DE-588)120637561 oth Binggeli, Bruno Sonstige oth Schweizerische Gesellschaft für Astrophysik und Astronomie Sonstige (DE-588)600073-3 oth Saas-Fee Advanced Course 23. 1993 Les Diablerets Sonstige (DE-588)2147573-8 oth Digitalisierung TU Muenchen application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=006845746&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
| spellingShingle | The deep universe lecture notes 1993 Kosmologie (DE-588)4114294-9 gnd |
| subject_GND | (DE-588)4114294-9 (DE-588)1071861417 |
| title | The deep universe lecture notes 1993 |
| title_auth | The deep universe lecture notes 1993 |
| title_exact_search | The deep universe lecture notes 1993 |
| title_full | The deep universe lecture notes 1993 Saas Fee Advanced Course 23. A. R. Sandage ; R. G. Kron ; M. S. Longair. Swiss Society for Astrophysics and Astronomy. Ed. by B. Binggeli ... |
| title_fullStr | The deep universe lecture notes 1993 Saas Fee Advanced Course 23. A. R. Sandage ; R. G. Kron ; M. S. Longair. Swiss Society for Astrophysics and Astronomy. Ed. by B. Binggeli ... |
| title_full_unstemmed | The deep universe lecture notes 1993 Saas Fee Advanced Course 23. A. R. Sandage ; R. G. Kron ; M. S. Longair. Swiss Society for Astrophysics and Astronomy. Ed. by B. Binggeli ... |
| title_short | The deep universe |
| title_sort | the deep universe lecture notes 1993 |
| title_sub | lecture notes 1993 |
| topic | Kosmologie (DE-588)4114294-9 gnd |
| topic_facet | Kosmologie Konferenzschrift 1993 Les Diablerets |
| url | http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=006845746&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA |
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