- ISBN: 9780444530073 | 044453007X
- Cover: Hardcover
- Copyright: 9/12/2007
Organizers | p. ix |
Lecturers | p. xi |
Participants | p. xiii |
Preface | p. xvii |
Long Lectures | p. 1 |
Gravitational waves | p. 3 |
Introduction | p. 7 |
Linearization of Einstein equations | p. 8 |
Einstein equations and gauge symmetry | p. 9 |
Wave equation | p. 11 |
Transverse-traceless gauge | p. 12 |
Interaction of gravitational waves with point particles | p. 13 |
Newtonian and relativistic description of tidal gravity | p. 13 |
Description in the transverse-traceless gauge | p. 14 |
Description in the free-falling frame | p. 15 |
Key ideas underlying gravitational-wave detectors | p. 16 |
Effective stress-energy tensor of gravitational waves | p. 18 |
Generation of gravitational waves | p. 21 |
Sources in slow motion, weak-field and negligible self-gravity | p. 21 |
Sources in slow motion and weak-field, but non-negligible self-gravity | p. 23 |
Radiated energy, angular momentum and linear momentum | p. 24 |
Application to binary systems | p. 25 |
Inspiral waveforms at leading Newtonian order | p. 25 |
Inspiral waveform including post-Newtonian corrections | p. 28 |
Merger and ring-down waveforms | p. 30 |
Templates for data analysis | p. 32 |
Other astrophysical sources | p. 36 |
Pulsars | p. 36 |
Supernovae | p. 39 |
Cosmological sources | p. 39 |
Phenomenological bounds | p. 40 |
Gravitational waves produced by causal mechanisms | p. 41 |
Gravitational waves produced by cosmic and fundamental strings | p. 44 |
Gravitational waves produced during inflation | p. 45 |
References | p. 48 |
Baryogenesis | p. 53 |
Observational evidence for the BAU | p. 57 |
Sakharov's conditions for baryogenesis | p. 60 |
B violation | p. 61 |
Loss of thermal equilibrium | p. 62 |
C, CP violation | p. 63 |
Examples of CP violation | p. 65 |
More history | p. 68 |
Example: GUT baryogenesis | p. 69 |
Washout processes | p. 73 |
B and CP violation in the standard model | p. 76 |
CP violation in the SM | p. 80 |
Electroweak phase transition and electroweak baryogenesis | p. 82 |
Strength of the phase transition | p. 85 |
EWPT in the MSSM | p. 91 |
A model of electroweak baryogenesis: 2HDM | p. 95 |
EDM constraints | p. 103 |
EWBG in the MSSM | p. 104 |
Other mechanisms; Leptogenesis | p. 108 |
References | p. 112 |
String cosmology | p. 117 |
Dark energy | p. 121 |
The problem of scales | p. 121 |
The string theory landscape | p. 121 |
The Bousso-Polchinski (Brown-Teitelboim) mechanism | p. 124 |
Caveats to the landscape approach | p. 130 |
Inflation | p. 130 |
Brane-antibrane inflation | p. 131 |
Warped compactification | p. 136 |
Warped brane-antibrane inflation | p. 140 |
The [eta] problem | p. 141 |
Solutions (?) to the [eta] problem | p. 146 |
Confrontation with experiment | p. 153 |
References | p. 159 |
Physics of the early universe and inflation | p. 165 |
Preamble | p. 169 |
Concise history of the early universe | p. 169 |
Big Bang: answered questions | p. 169 |
Big Bang: unanswered questions | p. 175 |
Inflation | p. 181 |
Inflation: answered questions | p. 181 |
Models of inflation | p. 185 |
Inflaton family portrait | p. 189 |
Global geometry | p. 194 |
Generalities | p. 195 |
De Sitter and FRW geometries | p. 196 |
FRW geometry | p. 198 |
Single FRW domain from inflation | p. 199 |
Scalar field fluctuations in de Sitter geometry | p. 202 |
Multiple FRW domains from inflation and fractal geometry in the future | p. 207 |
Generation of fluctuations from inflation | p. 211 |
Cosmic piano | p. 211 |
Generation of the scalar metrics fluctuations | p. 213 |
Generation of the tensor metrics fluctuations | p. 214 |
Probing models with fluctuations | p. 215 |
Preheating after inflation | p. 219 |
Heating the universe after inflation | p. 219 |
Pair creation by an electric field | p. 221 |
Linear resonant preheating | p. 222 |
Non-linear dynamics of resonant preheating | p. 223 |
Inflaton fragmentation | p. 226 |
Tachyonic preheating | p. 228 |
Gravitational waves from preheating | p. 228 |
References | p. 230 |
Cosmic microwave background anisotropies up to second order | p. 233 |
Preamble | p. 237 |
Introduction | p. 237 |
Perturbing gravity | p. 240 |
The collisionless Boltzmann equation for photons | p. 242 |
Collision term | p. 246 |
The collision integral | p. 246 |
Computation of different contributions to the collision term | p. 250 |
Final expression for the collision term | p. 255 |
The Brightness equation | p. 256 |
First order | p. 256 |
Second order | p. 257 |
Hierarchy equations for multipole moments | p. 260 |
Integral solution of the second-order Boltzmann equation | p. 263 |
The Boltzmann equation for baryons and cold dark matter | p. 265 |
Energy continuity equations | p. 267 |
Momentum continuity equations | p. 269 |
Linear solution of the Boltzmann equations | p. 274 |
Linear solutions in the limit of tight coupling | p. 275 |
Perturbation modes with k [double less-than sign] k[subscript eq] | p. 277 |
Perturbation modes with k [double greater-than sign] k[subscript eq] | p. 278 |
Conclusions | p. 278 |
Einstein's equations | p. 279 |
The metric tensor | p. 280 |
The connection coefficients | p. 280 |
Einstein tensor | p. 280 |
Energy-momentum tensor | p. 281 |
First-order solutions of Einstein's equations in various eras | p. 283 |
Matter-dominated era | p. 283 |
Radiation-dominated era | p. 283 |
References | p. 284 |
Physics beyond the standard model and dark matter | p. 287 |
Introduction | p. 291 |
Particle physics and cosmology | p. 291 |
Next threshold | p. 293 |
Why beyond the standard model | p. 295 |
Empirical reasons | p. 295 |
Philosophical and aesthetic reasons | p. 296 |
Positron analogue | p. 299 |
Hierarchy problem | p. 302 |
Examples of physics beyond the standard model | p. 302 |
Supersymmetry | p. 303 |
Composite Higgs | p. 305 |
Extra dimensions | p. 306 |
Evidence for dark matter | p. 310 |
What dark matter is not | p. 312 |
MACHOs | p. 313 |
Neutrinos | p. 314 |
CHAMPs and SIMPs | p. 316 |
WIMP dark matter | p. 316 |
WIMP | p. 316 |
Boltzmann equation | p. 318 |
Analytic approximation | p. 320 |
Numerical integration | p. 321 |
The new minimal standard model | p. 322 |
Direct detection experiments | p. 324 |
Popular WIMPs | p. 326 |
Indirect detection experiments | p. 328 |
Dark horse candidates | p. 328 |
Gravitino | p. 328 |
Axion | p. 330 |
Other candidates | p. 332 |
Cosmic coincidence | p. 332 |
Conclusions | p. 334 |
Gravitational lensing | p. 334 |
Deflection angle | p. 334 |
Amplification in microlensing | p. 338 |
MACHO search | p. 340 |
Strong lensing | p. 342 |
References | p. 343 |
Short Topical Lectures | p. 349 |
Effective field theories and gravitational radiation | p. 351 |
Lecture I | p. 355 |
Introduction and motivation | p. 355 |
Effective field theories: a review | p. 358 |
Lecture II | p. 370 |
The binary inspiral as an EFT calculation | p. 370 |
The EFT for isolated compact objects | p. 371 |
Calculating observables | p. 374 |
Integrating out the orbital scale | p. 381 |
Radiation | p. 386 |
Finite size effects | p. 390 |
Conclusions | p. 392 |
Redundant operators | p. 393 |
References | p. 395 |
Holographic cosmology | p. 397 |
Introduction | p. 401 |
Framework | p. 401 |
Anti-de Sitter cosmologies | p. 403 |
Dual field theory evolution | p. 405 |
Discussion | p. 409 |
References | p. 410 |
Neutrino physics and cosmology | p. 411 |
Introduction | p. 415 |
The cosmic neutrino background | p. 415 |
Relic neutrino production and decoupling | p. 415 |
Background evolution | p. 418 |
Neutrinos and Primordial Nucleosynthesis | p. 419 |
Extra radiation and the effective number of neutrinos | p. 420 |
Massive neutrinos | p. 421 |
Flavour oscillations and neutrino masses | p. 421 |
Neutrinos as dark matter | p. 423 |
Effects of neutrino masses on cosmology | p. 424 |
Brief description of cosmological observables | p. 425 |
Neutrino free-streaming | p. 425 |
Impact of massive neutrinos on the matter power spectrum | p. 427 |
Impact of massive neutrinos on the CMB anisotropy spectrum | p. 429 |
Current bounds on neutrino masses | p. 430 |
CMB anisotropies | p. 430 |
Galaxy redshift surveys | p. 431 |
Lyman-[alpha] forest | p. 432 |
Summary and discussion of current bounds | p. 432 |
Future sensitivities on neutrino masses from cosmology | p. 434 |
Conclusions | p. 435 |
References | p. 436 |
Cosmic microwave background: observational status | p. 437 |
Introduction | p. 441 |
CMB temperature anisotropies: the "early" days | p. 442 |
WMAP first release | p. 443 |
Polarization of the CMB - discovery and first measurements | p. 445 |
WMAP three year release | p. 447 |
Conclusion | p. 450 |
References | p. 450 |
Structure formation with numerical simulations | p. 453 |
Introduction | p. 457 |
The hierarchical scenario | p. 457 |
Computational cosmology | p. 458 |
Internal structure of dark matter haloes | p. 460 |
The halo model | p. 463 |
Galaxy formation physics | p. 464 |
The Mare Nostrum simulation | p. 466 |
Conclusion | p. 469 |
References | p. 469 |
Giving mass to the graviton | p. 471 |
Introduction | p. 475 |
Theoretical obstructions to massive gravity | p. 477 |
Constructing the massive gravity models | p. 482 |
Linear perturbations | p. 486 |
Some phenomenological implications | p. 489 |
Newton's potential | p. 489 |
Cosmological evolution | p. 493 |
Experimental signatures | p. 494 |
Summary and outlook | p. 496 |
References | p. 498 |
Working Group Reports | p. 501 |
Dark matter on the smallest scales | p. 503 |
Introduction | p. 503 |
The dark matter problem | p. 504 |
Dark matter candidates | p. 505 |
Small scale structure | p. 506 |
Detectability and future work | p. 507 |
References | p. 509 |
Scalar gravity: post-Newtonian corrections via an effective field theory approach | p. 511 |
Introduction | p. 511 |
Scalar gravity | p. 511 |
NRGR | p. 512 |
Einstein-Infeld-Hoffmann | p. 513 |
Discussion - Conclusions | p. 515 |
Dark Matter in minimal trinification | p. 517 |
Introduction | p. 517 |
Trinification in a nutshell | p. 518 |
A simple case | p. 519 |
Light and darkness of trinification | p. 520 |
A Dark Matter candidate | p. 521 |
Relative abundance | p. 521 |
Decay time | p. 522 |
Conclusion and discussion | p. 523 |
References | p. 524 |
Trans-Planckian physics from cosmology | p. 525 |
Introduction | p. 525 |
Standard approach | p. 526 |
Trans-Planckian behavior: non-linear dispersion relation | p. 527 |
References | p. 529 |
A pedagogical primer on preheating | p. 531 |
Introduction | p. 531 |
Inflation and its end | p. 532 |
A simple model of preheating | p. 532 |
Gravitational fluctuations | p. 534 |
References | p. 535 |
Braneworld graviton interactions in early universe phase transitions | p. 537 |
Braneworld cosmology | p. 537 |
Brane inflation and the Electroweak phase transition | p. 538 |
Gravitons | p. 539 |
References | p. 541 |
Individual Seminars | p. 543 |
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