Hamiltonian formulation and canonical quantization of perfect-fluid-filled Kantowski-Sachs cosmological models
A Hamiltonian formulation of anisotropic perfect-fluid-filled Kantowski-Sachs universes based on Demaret and Moncrief 's unconstrained Arnowitt-Deser-Misner Hamiltonian is given; the canonical equations are derived and shown to be equivalent to the field equations, which proves the coherence of the reduction process. A canonical quantization method equivalent to the one previously used to quantize the perfect-fluid-filled diagonal Bianchi types I, V, and IX cosmological models is applied to the Kantowski-Sachs universes, leading to a Schroedinger equation for the wave function of these models and thus to a probability interpretation of the formalism. The density of probability of finding these universes in the classical singular state is shown to be zero for each barotropic equation of state of the type p = (..gamma..-1)rho (1< or =..gamma..< or =2) apart from a set of measure zero of models corresponding to the stiff equation of state p = rho.
- Research Organization:
- Institut d'Astrophysique, Universite de Liege, B-4200, Cointe-Ougree, Belgium
- OSTI ID:
- 6370441
- Journal Information:
- Phys. Rev. D; (United States), Vol. 26:12
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
GENERAL PHYSICS
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
COSMOLOGICAL MODELS
LAGRANGIAN FIELD THEORY
EQUATIONS OF STATE
FIELD EQUATIONS
HAMILTONIANS
PROBABILITY
QUANTUM FIELD THEORY
SPACE-TIME
UNIVERSE
WAVE FUNCTIONS
EQUATIONS
FIELD THEORIES
FUNCTIONS
MATHEMATICAL MODELS
MATHEMATICAL OPERATORS
QUANTUM OPERATORS
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