Quantum Cosmology of Kantowski-Sachs like Models
arXiv:gr-qc/9412049 · doi:10.1088/0264-9381/12/10/005
Abstract
The Wheeler-DeWitt equation for a class of Kantowski-Sachs like models is completely solved. The generalized models include the Kantowski-Sachs model with cosmological constant and pressureless dust. Likewise contained is a joined model which consists of a Kantowski-Sachs cylinder inserted between two FRW half--spheres. The (second order) WKB approximation is exact for the wave functions of the complete set and this facilitates the product structure of the wave function for the joined model. In spite of the product structure the wave function can not be interpreted as admitting no correlations between the different regions. This problem is due to the joining procedure and may therefore be present for all joined models. Finally, the {s}ymmetric {i}nitial {c}ondition (SIC) for the wave function is analyzed and compared with the ``no bouindary'' condition. The consequences of the different boundary conditions for the arrow of time are briefly mentioned.
21 pages, uses LaTeX2e, epsf.sty and float.sty, three figures (50 kb); changes: one figure added, new interpretation of quantizing procedure for the joined model and many minor changes
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- Exact solution of the Einstein-Skyrme model in a Kantowski-Sachs spacetime
- Tunneling of Macroscopic Universes
- Two-oscillator Kantowski-Sachs model of the Schwarzschild black hole interior
- Jackiw-Teitelboim Gravity and Lorentzian Quantum Cosmology
- Quantum Schwarzschild-(A)dS Black Holes: Unitarity and Singularity Resolution
- Kantowski-Sachs cosmology in scalar-torsion theory
- Quantum creation of an Inhomogeneous universe
- Cosmological Constant Seesaw in String/M-Theory
- Time-covariant Schrödinger equation and invariant decay probability: The -Kantowski-Sachs universe