Canonical wave packets in quantum cosmology
| dc.creator | Gousheh, S. S. | |
| dc.creator | Sepangi, H. R. | |
| dc.creator | Pedram, P. | |
| dc.creator | Mirzaei, M. | |
| dc.date | 2007-01-05 | |
| dc.date | 2007-08-20 | |
| dc.date.accessioned | 2026-07-07T11:01:34Z | |
| dc.date.available | 2026-07-07T11:01:34Z | |
| dc.description | We discuss the construction of wave packets resulting from the solutions of a class of Wheeler-DeWitt equations in Robertson-Walker type cosmologies, for arbitrary curvature. We show that there always exists a ``canonical initial slope" for a given initial wave function, which optimizes some desirable properties of the resulting wave packet, most importantly good classical-quantum correspondence. This can be properly denoted as a canonical wave packet. We introduce a general method for finding these canonical initial slopes which is generalization of our earlier work. | |
| dc.description | 19 pages, 8 figures | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0701035 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0701035 | |
| dc.identifier | Class.Quant.Grav.24:4377-4390,2007 | |
| dc.identifier | doi:10.1088/0264-9381/24/17/007 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/187986 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Canonical wave packets in quantum cosmology | |
| dc.type | text |