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9780750308106

Modern Cosmology

by ;
  • ISBN13:

    9780750308106

  • ISBN10:

    0750308109

  • Format: Hardcover
  • Copyright: 2001-12-01
  • Publisher: CRC Press

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Supplemental Materials

What is included with this book?

Summary

Based on lectures given to postgraduate students, this volume gathers contributions from a number of international scientists currently working in various research fields in cosmology. Of interest to students, researchers in relativity, gravitation, cosmology, and astrophysics.

Table of Contents

Preface xiii
The physics of the early universe (an overview)
1(8)
Silvio Bonometto
The physics of the early universe: an overview
1(8)
The middle-age cosmology
2(2)
Inflationary theories
4(2)
Links between cosmology and particale physics
6(1)
Basic questions and tentative answers
7(2)
An introduction to the physics of cosmology
9(99)
John A Peacock
Aspects of general relativity
9(4)
The equivalence principle
11(1)
Applications of gravitational time dilation
12(1)
The energy-momentum tensor
13(3)
Relativistic fluid mechanics
14(2)
The field equations
16(3)
Newtonian limit
16(1)
Pressure as a source of gravity
17(1)
Energy density of the vacuum
17(2)
The Friedmann models
19(13)
Cosmological coordinates
19(2)
The redshift
21(1)
Dynamics of the expansion
22(2)
Solutions to the Friedmann equation
24(3)
Horizons
27(1)
Observations in cosmology
27(2)
The meaning of an expanding universe
29(3)
Inflationary cosmology
32(15)
Inflation field dynamics
34(2)
Ending inflation
36(2)
Relic fluctuations from inflation
38(2)
Gravity waves and tilt
40(2)
Evidence for vacuum energy at late times
42(1)
Cosmic coincidence
43(4)
Dynamics of structure formation
47(11)
Linear perturbations
47(3)
Dynamical effects of radiation
50(3)
The peculiar velocity field
53(1)
Transfer functions
54(3)
The spherical model
57(1)
Quantifying large-scale structure
58(28)
Fourier analysis of density fluctuations
59(2)
The CDM model
61(2)
Karhunen-Loeve and all that
63(5)
Projection on the sky
68(4)
Nonlinear clustering: a problem for CDM?
72(2)
Real-space and redshift-space clustering
74(2)
The state of the art in LSS
76(5)
Galaxy formation and biased clustering
81(5)
Cosmic background fluctuations
86(22)
The hot big bang and the microwave background
86(2)
Mechanisms for primary fluctuations
88(2)
The temperature power spectrum
90(3)
Large-scale fluctuations and CMB power spectrum
93(2)
Predictions of CMB anisotropies
95(2)
Geometrical degeneracy
97(3)
Small-scale data and outlook
100(4)
References
104(4)
Cosmological models
108(51)
George F R Ellis
Introduction
108(4)
Spacetime
109(1)
Field equations
109(1)
Matter description
110(1)
Cosmology
111(1)
1+3 covariant description: variables
112(3)
Average 4-velocity of matter
112(1)
Kinematic quantities
113(1)
Matter tensor
114(1)
Electromagnetic field
114(1)
Weyl tensor
115(1)
1+3 Covariant description: equations
115(6)
Energy-momentum conservation equations
115(1)
Ricci identities
116(3)
Bianchi identities
119(1)
Implications
120(1)
Shear-free dust
120(1)
Tetrad description
121(3)
General tetrad formalism
121(2)
Tetrad formalism in cosmology
123(1)
Complete set
124(1)
Models and symmetries
124(6)
Symmetries of cosmologies
124(3)
Classification of cosmological symmetries
127(3)
Friedmann-Lemaitre models
130(2)
Phase planes and evolutionary paths
131(1)
Spatial topology
131(1)
Growth of inhomogeneity
132(1)
Bianchi universes (s = 3)
132(7)
Constructing Bianchi universes
133(1)
Dynamical systems approach
134(4)
Isotropization properties
138(1)
Observations and horizons
139(7)
Observational variables and relations: FL models
139(2)
Particle horizons and visual horizons
141(1)
Small universes
141(1)
Observations in anisotropic and inhomogeneous models
142(1)
Proof of almost-FL geometry
143(3)
Importance of consistency checks
146(1)
Explaining homogeneity and structure
146(8)
Showing initial conditions are irrelevant
147(3)
The explanation of initial conditions
150(3)
The irremovable problem
153(1)
Conclusion
154(5)
References
154(5)
Inflationary cosmology and creation of matter in the universe
159(27)
Andrei D Linde
Introduction
159(1)
Brief history of inflation
160(4)
Chaotic inflation
161(3)
Quantum fluctuations in the inflationary universe
164(4)
Quantum fluctuations and density perturbations
168(1)
From the big bang theory to the theory of eternal inflation
169(3)
(P)reheating after inflation
172(11)
Conclusions
183(3)
References
183(3)
Dark matter and particle physics
186(25)
Antonio Masiero
Silvia Pascoli
Introduction
186(2)
The SM of particle physics
188(4)
The Higgs mechanism and vector boson masses
189(2)
Fermion masses
191(1)
Successes and difficulties of the SM
192(1)
The dark matter problem: experimental evidence
192(2)
Lepton number violation and neutrinos as HDM candidates
194(4)
Experimental limits on neutrion masses
194(1)
Neutrino masses in the SM and beyond
195(1)
Thermal history of neutrinos
196(1)
HDM and structure formation
197(1)
Low-energy SUSY and DM
198(5)
Neutralinos as the LSP in SUSY models
198(1)
Neutralinos in the minimal supersymmetric SM
199(1)
Thermal history of neutralinos and ΩCDM
200(2)
CDM models and structure formation
202(1)
Warm dark matter
203(1)
Thermal history of light gravitinos and WDM models
203(1)
Dark energy, ACDM and xCDM or QCDM
204(7)
ACDM models
205(1)
Scalar field cosmology and quintessence
206(1)
References
207(4)
Supergravity and cosmology
211(8)
Renata Kallosh
M/string theory and supergravity
211(1)
Superconformal symmetry, supergravity and cosmology
212(3)
Gravitino production after inflation
215(1)
Super-Higgs effect in cosmology
216(1)
Mp → ∞ limit
217(2)
References
218(1)
The cosmic microwave background
219(45)
Arthur Kosowsky
A brief historical perspective
220(2)
Physics of temperature fluctuations
222(7)
Causes of temperature fluctuations
223(1)
A formal description
224(2)
Tight coupling
226(1)
Free-streaming
227(1)
Diffusion damping
227(1)
The resulting power spectrum
228(1)
Physics of polarization fluctuations
229(5)
Stokes parameters
230(1)
Thomson scattering and the quadrupolar source
231(1)
Harmonic expansions and power spectra
232(2)
Acoustic oscillations
234(5)
An oscillator equation
235(1)
Initial conditions
236(1)
Coherent oscillations
237(1)
The effect of baryons
238(1)
Cosmological models and constraints
239(12)
A space of models
239(2)
Physical quantities
241(1)
Power spectrum degeneracies
242(2)
Idealized experiments
244(3)
Current constraints and upcoming experiments
247(4)
Model-independent cosmological constraints
251(7)
Flatness
252(2)
Coherent acoustic oscillations
254(1)
Adiabatic primordial perturbations
254(1)
Gaussian primordial perturbations
255(1)
Tensor or vector perturbations
255(2)
Reionization redshift
257(1)
Magnetic fields
257(1)
The topology of the universe
257(1)
Finale: testing inflationary cosmology
258(6)
References
261(3)
Dark matter search with innovative techniques
264(18)
Andrea Giuliani
CDM direct detection
264(7)
Status of the DM problem
264(1)
Neutralinos
265(1)
The galactic halo
266(1)
Strategies for WIMP direct detection
267(4)
Phonon-mediated particle detection
271(2)
Basic principles
272(1)
The energy absorber
272(1)
Phonon sensors
273(1)
Innovative techniques based on phonon-mediated devices
273(6)
Basic principles of double readout detectors
273(1)
CDMS, EDELWEISS and CRESST experiments
274(2)
Discussion of the CDMS results
276(3)
Other innovative techniques
279(3)
References
280(2)
Signature for signals from the dark universe The DAMA Collaboration
282(14)
Introduction
282(3)
The highly radiopure ~100 kg Nal (T) set-up
285(1)
Investigation of the WIMP annual modulation signature
286(6)
Results of the model-independent approach
286(1)
Main points on the investigation of possible systematics in the new DAMA/Nal-3 and 4 running periods
287(3)
Results of a model-dependent analysis
290(2)
DAMA annual modulation result versus CDMS exclusion plot
292(2)
Conclusion
294(2)
References
295(1)
Neutrino oscillations: a phenomenological overview
296(16)
GianLuigi Fogli
Introduction
296(1)
Three-neutrino mixing and oscillations
297(1)
Analysis of the atmospheric data
298(4)
Analysis of the solar data
302(7)
Total rates and expectations
302(3)
Two-flavour oscillations in vacuum
305(1)
Two-flavour oscillations in matter
305(3)
Three-flavour oscillations in matter
308(1)
Conclusions
309(3)
References
311(1)
Highlights in modern observational cosmology
312(32)
Piero Rosati
Synopsis
312(1)
The cosmological fremework
312(9)
Friedmann cosmological background
313(1)
Observables in cosmology
314(3)
Applications
317(4)
Galaxy surveys
321(13)
Overview
321(1)
Survey strategies and selection methods
322(3)
Galaxy counts and evolution
325(3)
Colour selection techniques
328(3)
Star formation history in the universe
331(3)
Cluster surveys
334(10)
Clusters as cosmological probes
334(3)
Cluster search methods
337(2)
Determining Ωm and ΩΛ
339(3)
References
342(2)
Clustering in the universe: from highly nonlinear structures to homogeneity
344(23)
Luigi Guzzo
Introduction
344(1)
The clustering of galaxies
344(3)
Our distorted view of the galaxy distribution
347(6)
Is the universe fractal?
353(6)
Scaling laws
353(2)
Observational evidences
355(2)
Scaling in Fourier space
357(2)
Do we really see homogeneity? Variance on ~1000h-1 Mpc scales
359(4)
The REFLEX cluster survey
359(2)
'Peaks and valleys' in the power spectrum
361(2)
Conclusions
363(4)
References
364(3)
The debate on galaxy space distribution: an overview
367(11)
Marco Montuori
Luciano Pietronero
Introduction
367(1)
The standard approach of clustering correlation
367(1)
Criticisms of the standard approach
368(1)
Mass-length relation and conditional density
369(1)
Homogeneous and fractal structure
369(1)
ξ (r) for a fractal structure
369(1)
Galaxy surveys
370(2)
Angular samples
371(1)
Redshift samples
371(1)
Γ (r) analysis
372(2)
Interpretation of standard results
374(4)
References
376(2)
Gravitational lensing
378(42)
Philippe Jetzer
Introduction
378(3)
Historical remarks
379(2)
Lens equation
381(9)
Point-like lenses
381(2)
Thin lens approximation
383(1)
Lens equation
384(2)
Remarks on the lens equation
386(4)
Simple lens models
390(8)
Axially symmetric lenses
390(3)
Schwarzschild lens
393(2)
Singular isothermal sphere
395(1)
Generalization of the singular isothermal sphere
396(1)
Extended source
397(1)
Two point-mass lens
398(1)
Galactic microlensing
398(8)
Introduction
398(8)
The lens equation in cosmology
406(3)
Hubble constant from time delays
409(1)
Galaxy clusters as lenses
409(11)
Weak lensing
413(3)
Comparison with results from x-ray observations
416(1)
References
417(3)
Numerical simulations in cosmology
420(54)
Anatoly Klypin
Synopsis
420(1)
Methods
421(18)
Introduction
421(2)
Equations of evolution of fluctuations in an expanding universe
423(2)
Initial conditions
425(4)
Codes
429(4)
Effects of resolution
433(4)
Halo identification
437(2)
Spatial and velocity biases
439(12)
Introduction
439(1)
Oh, bias, bias
440(2)
Spatial bias
442(5)
Velocity bias
447(4)
Conclusions
451(1)
Dark matter halos
451(23)
Introduction
451(3)
Dark matter halos: the NFW and the Moore et al profiles
454(3)
Properties of dark matter halos
457(5)
Halo profiles: convergence study
462(9)
References
471(3)
Index 474

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