Quantum Cosmology for a Quadratic Theory of Gravity
arXiv:gr-qc/9411072 · doi:10.1088/0264-9381/11/9/007
Abstract
For pure fourth order () quantum cosmology the Wheeler-DeWitt equation is solved exactly for the closed homogeneous and isotropic model. It is shown that by imposing as boundary condition that at the origin of the universe the wave functions behave as suggested by Vilenkin.
13 pages, latex,no figures
References in corpus (2)
Cited by in corpus (7)
- Quadratic quantum cosmology with Schutz' perfect fluid
- Quantum Cosmology With R+R^2 Gravity
- Hamiltonian formulation of curvature squared action
- Classical and Quantum Solutions and the Problem of Time in Cosmology
- Hamiltonian Formulation of Bianchi Cosmological Models in Quadratic Theories of Gravity
- Period-doubling bifurcation in strongly anisotropic Bianchi I quantum cosmology
- Supersymmetric higher-derivative models in quantum cosmology