The primordial universe: = L' univers primordial
Saved in:
| Format: | Conference Proceeding Book |
|---|---|
| Language: | English |
| Published: |
Berlin [u.a.]
Springer
2000
LesUlis [u.a.] EDP Sciences |
| Series: | Ecole d'Eté de Physique Théorique: Session
71 |
| Subjects: | |
| Online Access: | Inhaltsverzeichnis |
| Item Description: | Literaturangaben |
| Physical Description: | XXXVI, 628 S. Ill., graph. Darst. : 23 cm |
| ISBN: | 3540410465 2868834981 |
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| 245 | 1 | 0 | |a The primordial universe |b = L' univers primordial |c École de Physique des Houches - UJF & INPG-Grenoble, LesHouches, Session LXXI, 28 June - 23 July 1999. Ed. by P. Binétruy ... |
| 246 | 1 | 1 | |a L' univers primordial |
| 264 | 1 | |a Berlin [u.a.] |b Springer |c 2000 | |
| 264 | 1 | |a LesUlis [u.a.] |b EDP Sciences | |
| 300 | |a XXXVI, 628 S. |b Ill., graph. Darst. : 23 cm | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b n |2 rdamedia | ||
| 338 | |b nc |2 rdacarrier | ||
| 490 | 1 | |a Ecole d'Eté de Physique Théorique: Session |v 71 | |
| 500 | |a Literaturangaben | ||
| 650 | 4 | |a Kosmologie - Astrophysik - Elementarteilchenphysik - Kongress - LesHouches <1999> | |
| 650 | 0 | 7 | |a Kosmologie |0 (DE-588)4114294-9 |2 gnd |9 rswk-swf |
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| 655 | 7 | |0 (DE-588)1071861417 |a Konferenzschrift |y 1999 |z Les Houches |2 gnd-content | |
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| 700 | 1 | |a Binétruy, Pierre |e Sonstige |4 oth | |
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| 830 | 0 | |a Ecole d'Eté de Physique Théorique: Session |v 71 |w (DE-604)BV000022608 |9 71 | |
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Record in the Search Index
| _version_ | 1804128477866098688 |
|---|---|
| adam_text | CONTENTS
Lecturers
xi
Participants
xiii
Préface
xvii
Preface
xxi
Contents
xxv
Course
1.
The Universe at High
Redshiñ
by S. Lilly
1
1
Introduction
5
1.1
The formation of structure in the Universe
.............. 5
1.2
Methodologies, opportunities and limitations
............ 6
1.3
Outline of the lectures
......................... 7
2
The present-day Universe
8
2.1
Galaxies
................................. 8
2.1.1
Normal galaxies
........................ 8
2.1.2
Galaxy scaling relations
.................... 10
2.1.3
Low surface brightness galaxies
................ 11
2.1.4
Dwarf galaxies
......................... 12
2.1.5
Active galactic nuclei
..................... 13
2.1.6
Ultra-luminous galaxies
.................... 13
2.2
The luminosity function and the luminosity density
and extragalactic background light
.................. 13
2.3
The baryon budget
........................... 15
XXVI
3
The theoretical framework. I: Cosmology
16
3.1
The Robertson-Walker metric and the appearance of distant objects
16
3.2
R(t) and the solutions to the
Friedmann
equation
......... 17
3.3
Cosmological parameters and uncertainties
............. 19
3.4
The development of density fluctuations
............... 19
3.4.1
Linear growth
.......................... 19
3.4.2
Fluctuations in baryonic matter and radiation
........ 20
3.4.3
Modification of the primordial spectrum
........... 20
4
The theoretical framework. II: The non-linear regime
22
4.1
Non-linear collapse
........................... 22
4.2
Hierarchical clustering and dissipation models
............ 22
4.3
The Press-Schechter formalism
.................... 25
4.4
Biassed galaxy formation
....................... 26
4.5
Origin of angular momentum
..................... 26
4.6
The structure of dark matter haloes
................. 27
4.7
Feed-back processes
.......................... 27
4.8
Chemical evolution
........................... 28
4.9
Galaxy spectral synthesis models
................... 30
4.10
Semi-analytic models
.......................... 31
5
The formation and evolution of galaxies: The local view
31
5.1
Star formation in disk galaxies and starbursts
............ 31
5.2
Spheroids and the elliptical galaxies
................. 32
5.3
Ultra-luminous galaxies
........................ 33
6
Evolution at cosmologically significant redshifts
34
6.1
Redshifts
2 > 1............................. 34
6.1.1
Methodologies
......................... 34
6.1.2
The evolving population of galaxies
............. 34
6.1.3
The early-type galaxy population
............... 35
6.1.4
The importance or otherwise of mergers
........... 37
6.1.5
The evolution of galaxies in rich clusters
........... 37
6.1.6
Inside the galaxies
....................... 38
6.2
Redshifts
z
> 3............................. 38
6.2.1
Detection and identification
.................. 38
6.2.2
Luminosity function and properties
.............. 39
6.2.3
Clustering and biassing
.................... 41
6.2.4
The nature of the Lyman-break population
......... 42
6.3
The observational gap at
z
= 2................... 42
7
The luminosity density as
ƒ
(г)
43
8
The cosmic evolution of active galactic nuclei
45
9
Luminous objects at high redshifts: The hidden Universe
45
10 Neutral gas 47
10.1 Re-ionization
of the IGM
....................... 47
10.2
High column density systems
..................... 48
10.3
The Lyman a forest systems
..................... 49
10.4
Global evolution of the neutral Hydrogen content
.......... 49
11
The first stars
49
12
Summary
52
Course
2.
Cosmological Parameters and Galaxy Formation
by J. Silk
61
1
Introduction
63
2
Temperature
65
3
Age
65
4
Hubble s constant
65
5 Baryon
density parameter
66
6
Matter density parameter
67
7
Cosmological constant
68
8
Spatial curvature
69
9
Density fluctuations
70
10 Ab initio
galaxy formation
74
11
Cold dark matter: Where we are today
75
12
Resolving the CDM conundrum
77
13
An empirical approach to disk star formation
78
14
Testing models of galaxy formation
81
15
Summary
83
XXVIII
Course
3.
A Short Course on
Big Bang Nucleosynthesis
by K.A. Olive
87
1
Introduction
89
2
Theory
90
3
Data
90
4
Likelihood analyses
93
5
More data
95
6
More analysis
96
7
Chemical evolution
96
8
Constraints from BBN
97
Course
4.
The Cosmic Microwave Background:
From Detector Signals to Constraints on the Early
Universe Physics
by F.R. Bouchet, J.-L.
Puget
and J.M.
Lamarre
103
1
Introduction
107
2
The cosmic background
108
2.1
Components of the cosmic background
................108
2.2
Formation of the CMB, recombination
................112
2.3
The CMB spectrum
..........................112
3
CMB anisotropies
118
3.1
Primary anisotropies
.......................... 118
3.1.1
Fundamental physics and CMB anisotropies
......... 118
3.1.2
The components of the primary fluctuations
......... 119
3.1.3
Power spectrum of the fluctuations in an inflationary model
119
3.2
The secondary CMB anisotropies
................... 121
3.2.1
Gravitational effects
...................... 122
3.2.2
Effects of the
reionisation
................... 125
4
Astrophysical foregrounds
129
4.1
Physics of galactic foregrounds
....................129
4.1.1
Dust emission
..........................129
4.1.2
Free-free emission
.......................134
4.1.3
Synchrotron emission
.....................136
XXIX
4.2
Physics of the extragalactic sources foregrounds
........... 138
4.2.1
Infrared galaxies and radio sources
.............. 138
4.2.2
Sunyaev-Zeldovich effect
................... 146
4.3
Putting it all together
......................... 149
4.3.1
A simple sky model
...................... 149
4.3.2
Detector noise backgrounds
................. 152
4.3.3
Comparing contributions
................... 153
5
Observations of CMB anisotropies
154
5.1
From raw data to the physics of the early Universe
........ 154
5.2
Observational requirements
...................... 156
5.3
Reaching the ultimate sensitivity
................... 159
5.4
Present status of observations
..................... 162
5.5
Future satellite observations: MAP, Planck
............. 163
5.6
Description of the Planck High-Frequency Instrument
....... 165
5.6.1
Instrument concept
....................... 165
5.6.2
Sensitivity
............................ 167
5.6.3
Focal plane optics
....................... 169
5.6.4
Bolometric detectors
...................... 173
6
Extraction of systematic effects and map making
176
6.1
Maximum likelihood estimators
.................... 176
6.2
Using noise properties
......................... 178
6.2.1
Systematics
........................... 179
6.2.2
Priors
.............................. 179
6.3
Map making
............................... 180
6.3.1
COBE
map making
..................... 181
6.3.2
Signal-to-noise (Wiener) filtering
............... 183
6.4
Using redundancies
........................... 184
6.5
Low-frequency noise
.......................... 186
6.5.1
Simplest destriping
....................... 187
6.6
Contributions from emission in the far side-lobes of the beam
. . . 187
7
Maps analysis methods
190
7.1
Methods of component separation
.................. 190
7.2
Final map accuracy achievable
.................... 192
7.3
Numerical simulations
......................... 196
7.3.1
Simulations of the observations
................ 197
7.3.2
Analysing simulated observations
............... 198
7.4
Joining ends
............................... 202
7.4.1
Power spectrum estimation
.................. 202
7.4.2
Constraints on models
..................... 204
8
Conclusions
207
Appendix
208
xxx
A Formulating the component separation problem
208
A.I Physical model
.............................208
A.
2
The separation problem
........................209
В
Error forecasts assuming Wiener filtering
210
B.I Reconstruction errors of linear component separations
.......210
B.2 Specific case of Wiener filtering
....................212
Course
5.
Introduction to Supersymmetry:
Astrophysical and Phenomenological Constraints
by K.A. Olive
221
1
Introduction
223
1.1
Some preliminaries
........................... 223
1.2
The hierarchy problem
......................... 226
1.3
Supersymmetric operators and transformations
........... 227
2
The simplest models
232
2.1
The massless non-interacting Wess-Zumino model
.........232
2.2
Interactions for chiral
multiplets
...................234
2.3
Gauge
multiplets
............................236
2.4
Interactions
...............................238
2.5
Supersymmetry breaking
........................242
3
The minimal supersymmetric standard model
244
3.1
The Higgs sector
............................ 246
3.2
The sfermions
.............................. 248
3.3
Neutralinos
............................... 250
3.4
Charginos
................................ 251
3.5
More supersymmetry breaking
.................... 251
3.5.1
D-Breaking
........................... 252
3.5.2
F-Breaking
........................... 252
3.6
R-parity
................................. 253
4
The constrained MSSM and supergravity
255
4.1
RG evolution
.............................. 256
4.2
The constrained MSSM
........................ 259
4.3
Supergravity
.............................. 261
5
Cosmology
264
5.1
The Polonyi problem
..........................265
5.2
The
gravitino
problem
.........................267
5.3
Inflation
.................................268
5.4
Baryogenesis
..............................270
5.4.1
The Affleck-Dine mechanism
.................271
6
Dark matter and accelerator constraints
276
Course
6.
Dark Matter: Direct Detection
by B.
Chardin
295
1
Motivations for non-baryonic Dark Matter
297
2
Weakly Interacting Massive Particles (WIMPs)
301
2.1
Phenomenology
............................. 301
2.2
Experimental signatures
........................ 303
2.3
WIMP direct detection experiments without discrimination
.... 304
2.3.1
Germanium detectors
..................... 305
2.3.2
Scintillator detectors
...................... 307
2.3.3
Cryogenic experiments
..................... 307
2.3.4
The purest of all materials
................... 308
2.4
WIMP direct detection experiments with discrimination
...... 310
2.4.1
Nal
experiments
........................ 310
2.4.2
Cryogenic detectors
...................... 312
2.4.3
A first WIMP candidate?
................... 314
2.4.4
Critical discussion and annual modulation signature
.... 315
2.5
Other discrimination techniques
.................... 319
2.5.1
Liquid xenon detectors
..................... 319
2.5.2
SIMPLE and PICASSO
.................... 319
2.6
Detecting the recoil direction
..................... 320
2.7
Low-energy WIMPs trapped in the Solar System
.......... 322
2.8
WIMPs with dominant axial interactions.
Direct vs. indirect detection
...................... 323
2.9
Testing (a significant part of) the SUSY models
........... 324
2.9.1
Neutron background
...................... 325
2.9.2
Surface events
......................... 328
2.9.3
Main detector strategies
.................... 328
2.10
Conclusions
............................... 330
3
Axions
330
4
Conclusions and perspectives
334
Course
7.
Inñation
and Creation of Matter in the Universe
by
A. Linde
341
1
Introduction
343
2
Brief history of inflation
344
XXXII
3
Quantum
fluctuations
in the inflationary universe
349
4
Quantum fluctuations and density perturbations
352
5
Initial conditions for inflation
354
6
From the Big Bang theory to the theory of eternal inflation
359
7
Stochastic approach to inflation
361
8
(P)reheating after inflation
367
9
Phase transitions and inflation after preheating
378
10
Open inflation
383
11
Towards inflation in supergravity: Hybrid inflation
386
12
Pre-Big Bang
388
13
Brane
world
389
14
Conclusions
392
Course
8.
Cosmological Constant vs. Quintessence
by P.
Binétruy
397
1
Cosmological constant
399
2
The role of supersymmetry
401
3
Observational results
402
4
Quintessence
404
4.1
Runaway quintessence
.........................406
4.2
Pseudo-Goldstone boson
........................413
5
Quintessential problems
414
6
Extra spacetime dimensions
417
7
Conclusion
420
хххш
Course
9.
Gravitino
Production
and Super-Higgs Effect
in Cosmology
by R. Kallosh
423
1
Introduction
425
2
Super-Higgs effect in cosmology
427
3
Gravitino
equations in one chiral
multiplet
case
429
4
Gravitino
production
434
Course
10.
Physics of the Early Universe:
Baryogenesis; Defects; Initial Conditions
by
N.
Turok
439
1
Introduction
441
2
Eiectroweak baryogenesis
443
3 В
violation in the standard model
447
4
The eiectroweak phase transition or crossover
453
5 Baryon
production
454
6
Two-Higgs baryogenesis
454
7
Baryogenesis from transport
456
8
Classical force baryogenesis
457
9
Cosmic defects
463
10
Unification and symmetry breaking
463
11
Homotopy and topology
464
12
Existence of defects
465
13
Low-energy actions
467
14
Scaling
468
15
Π
in the sky
469
XXXIV
16
Precision calculations
471
17
Refutation
473
18
Instantons
and the beginning
477
19
Singular
instantons
482
20
The four form and
Λ
488
21
Conclusions
489
Course
11.
M-Theory and Cosmology
by T. Banks
495
1
Introduction
497
2
M-theory, branes, moduli and all that
501
2.1
The story of
M
.............................501
3
Eleven-dimensional supergravity
510
4
Forms, branes and
BPS
states
513
4.1
Differential forms and topologically
nontrivial
cycles
........513
4.2
SUSY algebras and
BPS
states
....................516
5
Branes and compactification
517
5.1
A tale of two tori
............................517
5.2
A heterotic interlude
..........................524
5.3
Enhanced gauge symmetries
......................526
5.4
Conclusions
...............................529
6
Quantum cosmology
530
6.1
Semiclassical cosmology and quantum gravity
............530
6.2
Extreme moduli
.............................537
6.3
The moduli space of M-Theory on rectangular tori
.........539
6.4
The
2/5
transformation
........................540
6.5
The boundaries of moduli space
....................542
6.6
Covering the moduli space
.......................544
6.7
Moduli spaces with less SUSY
.....................548
6.8
Chaotically avoiding SUSY
......................550
6.9
Against inflation
............................552
6.10
Conclusions
...............................555
xxxv
7
Moduli and inflation
556
7.1
Introduction
............................... 556
7.2
Moduli as inflatons?
.......................... 556
7.3
Radius stabilization
.......................... 564
7.4
SUSY breaking
............................. 567
7.5
The effects of a dynamical radius
................... 572
7.6
Generalizing
Hořava-
Witten......................
573
7.7
Conclusions
............................... 574
Course
12.
String Cosmology: The Pre-Big Bang Scenario
by G.
Veneziano
581
1
Introduction
583
2
Basic motivations and ideas
584
2.1
Why string cosmology?
........................ 584
2.2
Why /which inflation?
......................... 587
2.3
Superstring-inspired cosmology
.................... 588
2.4
Explicit solutions
............................ 591
2.5
Phase diagrams and Penrose-style overview
............. 592
3
How could it have started?
596
3.1
Generic asymptotically trivial past
.................. 596
3.2
The asymptotic past s effective action and different
(conformai)
frames
.................................. 597
3.3
Classical asymptotic symmetries: The importance of SUSY
.... 598
3.4
Dilaton-driven inflation as gravitational collapse
.......... 598
3.5
Fine-tuning issues
........................... 601
3.6
The spherically symmetric case
.................... 603
4
Phenomenological consequences
605
4.1
Cosmologica!
amplification of vacuum fluctuations:
General properties
........................... 605
4.2
Tensor perturbations: An observable cosmic gravitational radiation
background (CGRB)?
......................... 609
4.3
Dilaton perturbations
......................... 611
4.4
Gauge-field perturbations: Seeds for Bgai?
.............. 613
4.5
Axion
perturbations: Seeds for CMBA and LSS?
.......... 613
4.6
Heating up the Universe
........................ 615
5
How could it have stopped?
616
5.1
No-go theorems
............................. 617
5.2
Exit
ста
a non-local V
......................... 617
5.3
Exit via
Bij
............................... 617
5.4
Exit via quantum tunnelling
...................... 618
5.5
Higher-derivative corrections
.....................618
5.6
Loop corrections and back reaction
..................619
5.7
Entropy considerations
.........................620
6
Outlook
623
Seminars by participants
629
|
| any_adam_object | 1 |
| building | Verbundindex |
| bvnumber | BV013664824 |
| classification_rvk | UD 4847 |
| classification_tum | PHY 400f PHY 900f PHY 980f |
| ctrlnum | (OCoLC)247947663 (DE-599)BVBBV013664824 |
| discipline | Physik |
| format | Conference Proceeding Book |
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| genre | (DE-588)1071861417 Konferenzschrift 1999 Les Houches gnd-content |
| genre_facet | Konferenzschrift 1999 Les Houches |
| id | DE-604.BV013664824 |
| illustrated | Illustrated |
| indexdate | 2024-07-09T18:49:52Z |
| institution | BVB |
| institution_GND | (DE-588)10017225-8 |
| isbn | 3540410465 2868834981 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-009337846 |
| oclc_num | 247947663 |
| open_access_boolean | |
| owner | DE-91G DE-BY-TUM DE-29T DE-355 DE-BY-UBR DE-703 DE-19 DE-BY-UBM |
| owner_facet | DE-91G DE-BY-TUM DE-29T DE-355 DE-BY-UBR DE-703 DE-19 DE-BY-UBM |
| physical | XXXVI, 628 S. Ill., graph. Darst. : 23 cm |
| publishDate | 2000 |
| publishDateSearch | 2000 |
| publishDateSort | 2000 |
| publisher | Springer EDP Sciences |
| record_format | marc |
| series | Ecole d'Eté de Physique Théorique: Session |
| series2 | Ecole d'Eté de Physique Théorique: Session |
| spelling | The primordial universe = L' univers primordial École de Physique des Houches - UJF & INPG-Grenoble, LesHouches, Session LXXI, 28 June - 23 July 1999. Ed. by P. Binétruy ... L' univers primordial Berlin [u.a.] Springer 2000 LesUlis [u.a.] EDP Sciences XXXVI, 628 S. Ill., graph. Darst. : 23 cm txt rdacontent n rdamedia nc rdacarrier Ecole d'Eté de Physique Théorique: Session 71 Literaturangaben Kosmologie - Astrophysik - Elementarteilchenphysik - Kongress - LesHouches <1999> Kosmologie (DE-588)4114294-9 gnd rswk-swf Astrophysik (DE-588)4003326-0 gnd rswk-swf Elementarteilchenphysik (DE-588)4014414-8 gnd rswk-swf (DE-588)1071861417 Konferenzschrift 1999 Les Houches gnd-content Kosmologie (DE-588)4114294-9 s Astrophysik (DE-588)4003326-0 s Elementarteilchenphysik (DE-588)4014414-8 s DE-604 Binétruy, Pierre Sonstige oth Ecole d'Été de Physique Théorique 71 1999 Les Houches Sonstige (DE-588)10017225-8 oth Ecole d'Eté de Physique Théorique: Session 71 (DE-604)BV000022608 71 Digitalisierung TU Muenchen application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=009337846&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
| spellingShingle | The primordial universe = L' univers primordial Ecole d'Eté de Physique Théorique: Session Kosmologie - Astrophysik - Elementarteilchenphysik - Kongress - LesHouches <1999> Kosmologie (DE-588)4114294-9 gnd Astrophysik (DE-588)4003326-0 gnd Elementarteilchenphysik (DE-588)4014414-8 gnd |
| subject_GND | (DE-588)4114294-9 (DE-588)4003326-0 (DE-588)4014414-8 (DE-588)1071861417 |
| title | The primordial universe = L' univers primordial |
| title_alt | L' univers primordial |
| title_auth | The primordial universe = L' univers primordial |
| title_exact_search | The primordial universe = L' univers primordial |
| title_full | The primordial universe = L' univers primordial École de Physique des Houches - UJF & INPG-Grenoble, LesHouches, Session LXXI, 28 June - 23 July 1999. Ed. by P. Binétruy ... |
| title_fullStr | The primordial universe = L' univers primordial École de Physique des Houches - UJF & INPG-Grenoble, LesHouches, Session LXXI, 28 June - 23 July 1999. Ed. by P. Binétruy ... |
| title_full_unstemmed | The primordial universe = L' univers primordial École de Physique des Houches - UJF & INPG-Grenoble, LesHouches, Session LXXI, 28 June - 23 July 1999. Ed. by P. Binétruy ... |
| title_short | The primordial universe |
| title_sort | the primordial universe l univers primordial |
| title_sub | = L' univers primordial |
| topic | Kosmologie - Astrophysik - Elementarteilchenphysik - Kongress - LesHouches <1999> Kosmologie (DE-588)4114294-9 gnd Astrophysik (DE-588)4003326-0 gnd Elementarteilchenphysik (DE-588)4014414-8 gnd |
| topic_facet | Kosmologie - Astrophysik - Elementarteilchenphysik - Kongress - LesHouches <1999> Kosmologie Astrophysik Elementarteilchenphysik Konferenzschrift 1999 Les Houches |
| url | http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=009337846&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA |
| volume_link | (DE-604)BV000022608 |
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