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