Resumen
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.
Idioma original | Inglés |
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Páginas (desde-hasta) | 3523-3527 |
Número de páginas | 5 |
Publicación | Physical Review D |
Volumen | 45 |
N.º | 10 |
DOI | |
Estado | Publicada - 1992 |