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Cosmic Strings and Other Topological Defects [Kietas viršelis]

(University of Cambridge), (Tufts University, Massachusetts)
  • Formatas: Hardback, 537 pages, aukštis x plotis x storis: 254x179x35 mm, weight: 1115 g
  • Serija: Cambridge Monographs on Mathematical Physics
  • Išleidimo metai: 29-Sep-1994
  • Leidėjas: Cambridge University Press
  • ISBN-10: 0521391539
  • ISBN-13: 9780521391535
Kitos knygos pagal šią temą:
  • Formatas: Hardback, 537 pages, aukštis x plotis x storis: 254x179x35 mm, weight: 1115 g
  • Serija: Cambridge Monographs on Mathematical Physics
  • Išleidimo metai: 29-Sep-1994
  • Leidėjas: Cambridge University Press
  • ISBN-10: 0521391539
  • ISBN-13: 9780521391535
Kitos knygos pagal šią temą:
Now in paperback, this book is the first comprehensive and coherent introduction to the role of cosmic strings and other topological defects in the universe. This study has been one of the major driving forces in cosmology over the last decade, and lies at the fruitful intersection of particle physics and cosmology. After an introduction to standard cosmological theory and the theory of phase transitions in the early universe, the book then describes, in turn, the properties, formation, and cosmological implications of cosmic strings, monopoles, domain walls and textures. The book concludes with a chapter considering the role of topological defects in inflationary universe models. Ample introductory material is included to make the book accessible to the wide audience of particle physicists, astrophysicists and cosmologists for whom this topic is of immediate interest.

Recenzijos

" a unique survey of one of the most fascinating and rapidly developing topics in which the theory of particles and astrophysics are combined in an intriguing way." Yuri N. Obukhov, General Relativity and Gravitation

Daugiau informacijos

Comprehensive introduction to the role of cosmic strings and other topological defects in the universe.
Preface xvii
Paperback preface xxi
Introduction
1(22)
Topological defects
1(4)
A brief history
2(2)
Overview
4(1)
Units and notation
5(1)
The standard cosmology
6(17)
The homogeneous expanding universe
6(2)
The Einstein equations
8(3)
Thermal history of the universe
11(2)
Primordial nucleosynthesis
13(2)
The microwave background radiation
15(1)
The growth of density fluctuations
16(5)
Shortcomings of the standard cosmology
21(2)
Phase transitions in the early universe
23(31)
Spontaneous symmetry breaking
23(14)
Simple models
23(3)
Non-abelian gauge theories
26(4)
Symmetry breaking in SU(2) models
30(5)
Grand unification: An SO(10) example
35(2)
The effective potential
37(2)
Cosmological phase transitions
39(9)
Symmetry restoration at high temperature
39(3)
Second-order phase transitions
42(3)
First-order phase transitions
45(3)
Inflationary scenarios
48(6)
The inflationary paradigm
48(2)
Slow-rollover models
50(3)
Other inflationary models
53(1)
Topological defects
54(32)
Introducing defects
54(6)
Topological conservation laws
54(2)
Evading Derrick's theorem
56(1)
Higher dimensions
57(2)
The Kibble mechanism
59(1)
Basic properties
60(11)
Domain walls
60(1)
Strings
61(3)
Monopoles
64(1)
Textures
65(1)
Transient defects
66(3)
Time-dependent solitons
69(1)
Quantum corrections
70(1)
Classification
71(15)
The fundamental group
72(4)
Lie groups and the fundamental theorem
76(4)
Higher homotopy groups and exact sequences
80(4)
Energetic considerations
84(2)
String field theory
86(36)
The abelian-Higgs model
86(8)
Detailed vortex structure
87(3)
Critical coupling
90(3)
Global U(1)-strings
93(1)
Non-abelian strings
94(9)
Structure and zero modes
94(2)
ZN-strings
96(2)
Phenomenological strings
98(1)
Alice strings
99(2)
Semilocal strings
101(1)
`Electroweak' strings
102(1)
String--strings interactions
103(13)
The inter-vortex potential
103(3)
Vortex scattering in two dimensions
106(3)
The two-vortex moduli space
109(4)
Reconnection in three dimensions
113(3)
Effective string actions
116(6)
The Nambu action
117(2)
The Kalb--Ramond action
119(3)
Superconducting strings
122(32)
Bosonic string superconductivity
122(17)
Scalar condensate models
122(4)
Persistent currents
126(2)
Current quenching
128(4)
Worldsheet charge
132(1)
Microphysical string interactions
133(1)
An effective action
134(2)
Current growth in an electric field
136(1)
Gauge boson superconductivity
137(2)
Fermionic string superconductivity
139(10)
Vortex zero modes
139(2)
Fermionic currents
141(1)
Anomaly cancellation
142(2)
Some Fermi phenomenology
144(1)
Charge carrier scattering
145(2)
Bosonization and the effective action
147(1)
Massive fermionic bound states
148(1)
Vacuum effects
149(5)
Pair production
149(3)
W-condensation
152(2)
String dynamics
154(28)
The Nambu action
154(2)
Strings in flat spacetime
156(7)
Equations of motion and gauge fixing
156(2)
Oscillating loops
158(1)
Cusps and kinks
159(2)
Some loop examples
161(2)
Strings in curved spacetime
163(7)
Gauge fixing
163(2)
Strings in an expanding universe
165(3)
Strings in a stationary field
168(2)
String interactions
170(4)
Reconnection
170(2)
Loop fragmentation
172(2)
Strings with small-scale structure
174(4)
Equation of state
174(3)
Wiggly string dynamics
177(1)
String thermodynamics
178(4)
String gravity
182(38)
Straight string metric
182(10)
Linearized gravity
183(2)
Full Einstein gravity
185(6)
Gravity in (2+1)-dimensions
191(1)
Propagation of particles and light
192(4)
Double images
193(1)
String Doppler shifts
194(1)
Field theory in a conical space
195(1)
Gravitational field of a global string
196(2)
Gravitational field of an oscillating loop
198(5)
The average field
199(1)
Effects of cusps and kinks
200(3)
Gravitational radiation from a loop
203(6)
Radiation power
203(3)
Angular distribution and spectrum
206(2)
Radiation of momentum
208(1)
Wiggly string gravity
209(6)
The average field
209(1)
Propagation of particles and light
210(2)
Gravitational radiation
212(1)
Travelling waves on strings
213(2)
Self-interaction and related issues
215(5)
Gravitational back-reaction
215(2)
Strings as distributional sources
217(3)
String interactions
220(37)
Particle scattering by strings
220(7)
Scattering cross-section
220(4)
Frictional force
224(1)
String dynamics with friction
225(2)
Particle production
227(2)
Global string dynamics and radiation
229(9)
An effective action
229(1)
Global string dynamics
230(5)
Goldstone boson radiation
235(3)
String electrodynamics I: Formalism
238(4)
Basic equations
238(2)
Gauge conditions
240(1)
Charge renormalization
241(1)
String electrodynamics II: Applications
242(9)
Free superconducting strings
242(2)
Strings in an external field
244(2)
Electromagnetic radiation from loops
246(2)
Radiative damping and string dynamos
248(1)
Pair production
249(1)
Loop lifetimes
250(1)
Plasma interactions
251(6)
String evolution
257(35)
String formation
257(6)
The Kibble mechanism
257(2)
Network configuration at formation
259(4)
Damped epoch evolution
263(2)
The `one-scale' model
265(9)
Heuristic picture
265(3)
Strings in an expanding universe
268(1)
The `scaling' solution
269(3)
Further analytic modelling
272(2)
Numerical modelling
274(11)
Simulation techniques
275(2)
The `scaling' regime
277(4)
Long-string substructure
281(2)
Loop production mechanisms
283(2)
String domination
285(4)
Non-intercommuting strings
286(2)
A tangled network
288(1)
String--monopole network evolution
289(3)
Cosmological implications of strings
292(25)
Summary of string properties and evolution
292(6)
Gravitational properties of strings
292(2)
String evolution
294(4)
Microwave background anisotropies
298(4)
Strings as gravitational lenses
302(4)
Gravitational radiation background
306(7)
Radiation by loops: simple derivation
306(1)
Radiation by loops: improved derivation
307(4)
Radiation by infinite strings
311(1)
Observational bounds
311(2)
Black hole formation
313(2)
Baryon asymmetry
315(2)
Structure formation with strings
317(26)
Defects and structure formation
317(3)
Accretion onto loops
320(8)
The Zel'dovich approximation
320(2)
Static loops
322(1)
Moving loops
323(3)
Effects of hot dark matter and baryons
326(2)
Loops as seeds for galaxies and clusters
328(6)
Cold dark matter
329(2)
Hot dark matter
331(2)
Baryon-dominated universe
333(1)
Wakes
334(4)
Wakes due to straight strings
334(3)
Wakes due to wiggly strings
337(1)
Wakes and large-scale structure
338(3)
Wakes and the origin of cosmic magnetic fields
341(1)
Outlook
342(1)
Cosmology of superconducting and global strings
343(25)
Superconducting strings
343(19)
String electrodynamics: a review
343(4)
Strings within the Galaxy
347(3)
Light superconducting strings
350(3)
Strings and primordial magnetic fields
353(6)
Springs and vortons
359(3)
Global string cosmology
362(6)
Global string evolution
362(2)
Goldstone boson background
364(1)
Axion constraints
365(3)
Domain walls
368(29)
Field theory
368(4)
Domain wall models
368(2)
Walls bounded by strings
370(2)
Domain wall dynamics
372(6)
Action for a domain wall
372(1)
Wall motion
373(2)
Walls in an expanding universe
375(1)
Dynamics of thick domain walls
376(1)
Decay of metastable domain walls
377(1)
Gravitational effects of domain walls
378(3)
Gravitational field of planar and spherical walls
378(2)
A wall-dominated universe
380(1)
Interaction with particles
381(3)
Reflection probability
381(2)
Frictional force
383(1)
Cosmological evolution
384(8)
Domain wall formation
384(1)
Evolution
385(5)
Observational bounds
390(1)
Avoiding wall domination
391(1)
Evolution of walls bounded by strings
392(5)
Monopoles
397(32)
Field theory
397(6)
The 't Hooft--Polyakov monopole
397(2)
The charge quantization condition
399(1)
Monopole mass and structure
400(1)
Bogomol'nyi bound and Prasad--Sommerfield limit
401(1)
Monopoles and grand unification
402(1)
Interaction with particles
403(3)
The drag force
403(2)
Baryon decay catalysis
405(1)
Formation and evolution of monopoles
406(7)
Formation
406(1)
Annihilation mechanisms
407(3)
Observational bounds
410(2)
Solutions to the monopole problem
412(1)
Monopoles connected by strings
413(8)
Physical properties
413(2)
Formation and evolution
415(3)
Langacker--Pi model
418(1)
Causality considerations
419(1)
Metastable monopoles?
420(1)
Global monopoles
421(8)
Physical properties
421(2)
Gravitational field
423(2)
Evolution
425(1)
Cosmological implications
426(1)
Global monopoles connected by strings
427(2)
Textures
429(15)
Effective action
429(2)
Field equations with a constraint
431(1)
Texture collapse
432(2)
Gravitational field of a collapsing texture
434(2)
Cosmological evolution
436(2)
Cosmological effects of texture
438(4)
Microwave background anisotropy
438(2)
Structure formation
440(2)
Gauge texture
442(2)
Topological defects and inflation
444(16)
Formation of defects after inflation
444(1)
Phase transitions during inflation
445(2)
Formation of defects by quantum fluctuations
447(4)
Defect solutions in de Sitter space
451(1)
Quantum nucleation of defects
452(5)
Physics of nucleation
452(4)
Cosmological implications of nucleating defects
456(1)
String--driven inflation
457(3)
References 460(35)
Index 495