The Bianchi IX model in Loop Quantum Cosmology
arXiv:gr-qc/0404039 · doi:10.1088/0264-9381/21/14/015
Abstract
The Bianchi IX model has been used often to investigate the structure close to singularities of general relativity. Its classical chaos is expected to have, via the BKL scenario, implications even for the approach to general inhomogeneous singularities. Thus, it is a popular model to test consequences of modifications to general relativity suggested by quantum theories of gravity. This paper presents a detailed proof that modifications coming from loop quantum gravity lead to a non-chaotic effective behavior. The way this is realized, independently of quantization ambiguities, suggests a new look at initial and final singularities.
41 pages, 3 figures, revtex4
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- Loop Quantum Cosmology
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- Spherically Symmetric Quantum Geometry: Hamiltonian Constraint
- Homogeneous Loop Quantum Cosmology: The Role of the Spin Connection
- Genericness of Big Bounce in isotropic loop quantum cosmology
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- Quantum gravitational Kasner transitions in Bianchi-I spacetime
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- Genericness of inflation in isotropic loop quantum cosmology
- Primordial Density Perturbation in Effective Loop Quantum Cosmology
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- Singularity avoidance in a quantum model of the Mixmaster universe
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- Inflationary scalar spectrum in loop quantum cosmology
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- Quantum gravity might restrict a cyclic evolution
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