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E-raamat: Deparametrization And Path Integral Quantization Of Cosmological Models

(Univ De Buenos Aires, Argentina)
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The problem of time is a central feature of quantum cosmology: differing from ordinary quantum mechanics, in cosmology there is nothing outside the system which plays the role of clock, and this makes difficult the obtention of a consistent quantization. A possible solution is to assume that a subset of the variables describing the state of the universe can be a clock for the remaining of the system. Following this line, in this book a new proposal consisting in the previous identification of time by means of gauge fixation is applied to the quantization of homogeneous cosmological models. Both path integral and canonical formulations are studied for relativistic and string cosmologies; in particular, a complete chapter about low energy string cosmology is included. The required basic concepts (as for example the Hamiltonian formulation of General Relativity) are reviewed, so that the book can be of interest not only for a researcher but also for a student.
Preface vii
Introduction
1(6)
The gravitational field as a constrained Hamiltonian system
7(10)
Momentum and Hamiltonian constraints
7(3)
Minisuperspaces as constrained systems
10(3)
Quantization
13(4)
Canonical quantization
13(1)
Path integral quantization
14(3)
Deparametrization and path integral quantization
17(28)
The identification of time
17(4)
Gauge fixation and deparametrization
17(3)
Topology of the constraint surface: intrinsic and extrinsic time
20(1)
Gauge-invariant action for a parametrized system
21(7)
End point terms
22(2)
Observables and time
24(3)
Non separable constraints
27(1)
Path integral
28(5)
General formalism
28(3)
The function f and the reduced Hamiltonian. Unitarity
31(2)
Examples
33(12)
Feynman propagator for the Klein-Gordon equation
33(3)
The ideal clock
36(4)
Transition probability for empty Friedmann-Robertson-Walker universes
40(5)
Homogeneous relativistic cosmologies
45(32)
Isotropic universes
45(16)
A toy model
46(2)
True degrees of freedom
48(4)
A more general constraint
52(6)
Extrinsic time. The closed ``de Sitter'' universe
58(3)
Comment
61(1)
Anisotropic universes
61(16)
The Kantowski-Sachs universe
63(5)
The Taub universe
68(6)
Other anisotropic models
74(3)
String cosmologies
77(14)
String theory on background fields
77(3)
String cosmological models
80(2)
Path integral quantization
82(9)
Gauge-invariant action
82(2)
Extrinsic time
84(2)
Intrinsic time and path integral
86(2)
Summary
88(3)
Canonical quantization
91(14)
Approximate solutions of the Wheeler-DeWitt equation
92(1)
Gauge fixation and Schrodinger equation for isotropic models
93(1)
The Taub universe
94(6)
Standard procedure
94(1)
Boundary conditions and Schrodinger equation
95(2)
Wheeler-DeWitt equation with extrinsic time
97(3)
String cosmologies
100(5)
Wheeler-DeWitt equation
100(2)
Schrodinger equation
102(3)
Discussion
105(6)
Appendix A Constrained Hamiltonian systems 111(6)
A.1 Hamiltonian formalism for constrained systems
111(3)
A.2 Gauge transformations and gauge fixation
114(3)
Appendix B Path integral and inner product 117(6)
B.1 Ordinary mechanical systems
117(1)
B.2 Constrained systems
118(1)
B.3 Inner product for constrained systems
119(2)
B.4 Propagator and projected kernel
121(2)
Appendix C End point terms 123(6)
Appendix D An extrinsic time for the Taub universe 129(2)
Appendix E Free-particle constraint for minisuperspaces 131(2)
Bibliography 133(4)
Index 137