Abstract
We present the construction of a Hamiltonian description for a (non-Lagrangian) Bianchi type-V cosmological model using the solutions of the equations of motion as a starting point. We study the quantization of the model and compare our results to those found using a more standard approach.
- Received 1 October 1991
DOI:https://doi.org/10.1103/PhysRevD.45.3523
©1992 American Physical Society
