Quantum Geometrodynamics in the Bohm-de Broglie Interpretation
| dc.creator | Santini, E. Sergio | |
| dc.date | 2000-05-22 | |
| dc.date.accessioned | 2026-07-07T03:24:58Z | |
| dc.date.available | 2026-07-07T03:24:58Z | |
| dc.description | In this thesis the Bohm-de Broglie interpretation of quantum mechanics is applied to canonical quantum gravity. It is shown that, irrespective of any regularization or choice of factor ordering of the Wheeler-DeWitt equation, the unique relevant quantum effect which does not break spacetime is the change of its signature from lorentzian to euclidean. The other quantum effects are either trivial or break the four-geometry of spacetime. A Bohm-de Broglie picture of quantum geometrodynamics is constructed, which allows the investigation of these latter structures. For instance, it is shown that any real solution of the Wheeler-De Witt equation yields a generate four-geometry compatible with the strong gravity limit of General Relativity and the Carroll group. We prove that quantum geometrodynamics in the Bohm-de Broglie interpretation is consistent for any quantum potential. As a previous step to introduce our metodology, we study the quantum theory of fields in Minkowski spacetime in the Bohm-de Broglie interpretation and exhibit a concrete example where Lorentz invariance of individual events is broken. | |
| dc.description | PhD Thesis at CBPF-Rio de Janeiro-May 2000 (Advisor: N. Pinto-Neto, 95 pages, in Portuguese) | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0005092 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0005092 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/33546 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Quantum Physics | |
| dc.title | Quantum Geometrodynamics in the Bohm-de Broglie Interpretation | |
| dc.type | text |