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9780521793766

An Introduction to Cosmology

by
  • ISBN13:

    9780521793766

  • ISBN10:

    0521793769

  • Edition: 3rd
  • Format: Paperback
  • Copyright: 2002-02-04
  • Publisher: Cambridge University Press

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Summary

The third edition of this successful textbook is fully updated and includes important recent developments in cosmology. It begins with an introduction to cosmology and general relativity, and goes on to cover the mathematical models of standard cosmology. The physical aspects of cosmology, including primordial nucleosynthesis, the astroparticle physics of inflation, and the current ideas on structure formation are discussed. Alternative models of cosmology are reviewed, including the model of Quasi-Steady State Cosmology, which has recently been proposed as an alternative to Big Bang Cosmology. The final chapters discuss observational cosmology, and debate theory versus observational methods. The book includes 400 problems and numerous worked examples. This introductory textbook describes modern cosmology at a level suitable for advanced undergraduates and graduates who are familiar with mathematical methods and basic theoretical physics. It is intended for use on courses in theoretical physics, astrophysics or applied mathematics that include modern cosmology.

Author Biography

Jayant Narlikar graduated from Banaras Hindu University, India, in 1957. He then studied mathematics at Cambridge University, graduating with the highest honours and the Tyson Medal for Astronomy. He continued in Cambridge, obtaining first a Ph.D. and then the Sc.D. degree of Cambridge University. Professor Narlikar was a founder staff member of the Institute of Theoretical Astronomy in Cambridge in 1966 and later, in 1988, set up and became director of the Inter-University Centre for Astronomy and Astrophysics in Pune, India. He has received world-wide acclaim for his research in gravitation and cosmology

Table of Contents

Foreword xi
Preface to the first edition xii
Preface to the second edition xv
Preface to the third edition xvi
The large-scale structure of the universe
1(37)
Astronomy and cosmology
1(1)
From Herschel to Hubble
2(7)
Types of galaxy
9(9)
Radio sources
18(3)
Quasars
21(1)
Structures on the largest scale
22(5)
Coordinates and catalogues of astronomical objects
27(2)
The expansion of the universe
29(4)
Radiation backgrounds
33(1)
Theoretical models of the Universe
34(4)
Exercises
36(2)
The general theory of relativity
38(56)
Space, time and gravitation
38(3)
Vectors and tensors
41(8)
Covariant differentiation
49(4)
Riemannian geometry
53(2)
Spacetime curvature
55(3)
Geodesics
58(3)
The principle of equivalence
61(4)
The action principle and the energy tensors
65(5)
Gravitational equations
70(4)
The Schwarzschild solution
74(3)
Experimental tests of general relativity
77(17)
Exercises
87(7)
From relativity to cosmology
94(31)
The historical background
94(2)
Newtonian cosmology
96(3)
The Einstein universe
99(5)
The expanding universe
104(2)
Simplifying assumptions of cosmology
106(6)
The redshift
112(2)
Apparent brightness
114(4)
Hubble's law
118(1)
Angular size
119(2)
Surface brightness
121(1)
Source counts
121(4)
Exercises
122(3)
The Friedmann models
125(37)
Introduction
125(2)
The Einstein field equations simplified for cosmology
127(2)
Energy tensors of the universe
129(5)
The Friedmann models
134(9)
The luminosity distance
143(3)
Horizons and the Hubble radius
146(2)
The angular-size-redshift relation
148(2)
Source counts
150(2)
The radiation background from sources
152(2)
Cosmological models with the λ-term
154(4)
Concluding remarks
158(4)
Exercises
159(3)
Relics of the big bang
162(32)
The radiation-dominated universe
162(3)
Thermodynamics of the early universe
165(7)
Primordial neutrinos
172(3)
The neutron-to-proton ration
175(4)
The synthesis of light nuclei
179(6)
The microwave background
185(5)
Concluding remarks
190(4)
Exercises
190(4)
The very early universe
194(43)
Cosmology and particle physics
194(4)
The survival of massive particles
198(5)
Grand unified theories and baryogenesis
203(12)
Some problems of Friedmann cosmology
215(5)
The inflationary universe
220(7)
Primordial black holes
227(3)
Quantum cosmology
230(1)
Conclusion
231(6)
Exercises
234(3)
The formation of large-scale structures in the universe
237(41)
A key problem in cosmology
237(1)
The Jeans mass in the expanding universe
238(8)
Growth in the post-recombination era
246(4)
Observational constraints
250(6)
Density and mass fluctuations
256(2)
Inputs from the inflationary phase
258(5)
The role of dark matter
263(7)
The non-linear regime
270(8)
Exercises
274(4)
Alternative cosmologies
278(39)
Alternatives to Friedmann cosmologies
278(1)
Mach's principle
279(4)
The Brans-Dicke theory of gravity
283(3)
Cosmological solutions of the Brans-Dicke equations
286(4)
The Hoyle-Narlikar cosmologies
290(8)
Gravitational equations of NH theory
298(5)
The large-numbers hypothesis
303(2)
The two metrics
305(3)
Cosmological models based on the LNH
308(4)
Concluding remarks
312(5)
Exercises
312(5)
Cosmologies with creation of matter
317(51)
Introduction
317(1)
The steady-state theory
318(7)
Observable parameters of the steady-state cosmology
325(2)
Physical and astrophysical considerations
327(2)
The quasi-steady-state cosmology
329(5)
Planck particles
334(1)
The cosmological constant
335(2)
The creation of matter
337(6)
Cosmological models
343(4)
The quasi-steady-state solution
347(2)
The astrophysical picture
349(1)
The origin of the light nuclei
350(2)
The microwave background
352(8)
Large-scale structure
360(2)
Concluding remarks
362(6)
Exercises
364(4)
Local observational tests of cosmological significance
368(68)
Introduction
368(2)
The measurement of Hubble's constant
370(17)
The anisotropy of local large-scale velocity fields
387(5)
The distribution and density of matter in our neighbourhood
392(15)
The age of the universe
407(5)
The abundances of light nuclei
412(4)
The evidence for antimatter
416(2)
The microwave background
418(18)
Exercises
430(6)
Observations of distant parts of the universe
436(52)
The past light cone
436(2)
The redshift-magnitude relation
438(11)
Number counts of extragalactic objects
449(10)
The variation of angular size with distance
459(6)
The surface-brightness test
465(1)
Quasars as probes of the history of the universe
465(10)
Observational constraints on cosmological parameters
475(6)
The variation of fundamental constants
481(7)
Exercises
485(3)
A critical overview of cosmology
488(23)
Cosmology as a science
488(1)
Observational constraints on the QSSC
489(5)
The case for standard cosmology
494(1)
The case against standard cosmology
495(2)
The outlook for the future
497(3)
Concluding remarks
500(11)
Exercises
509(2)
Table of constants 511(3)
Glossary of symbols and abbreviations 514(1)
Bibliography 515(18)
Index 533

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