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.
| Original language | English |
|---|---|
| Pages (from-to) | 3523-3527 |
| Number of pages | 5 |
| Journal | Physical Review D |
| Volume | 45 |
| Issue number | 10 |
| DOIs | |
| State | Published - 1992 |