Theory of thin shells in general relativity: Equivalence of direct and Wheeler-DeWitt quantizations
| dc.creator | Zloshchastiev, Konstantin G. | |
| dc.date | 1997-09-12 | |
| dc.date | 1998-09-22 | |
| dc.date.accessioned | 2026-07-07T09:03:05Z | |
| dc.date.available | 2026-07-07T09:03:05Z | |
| dc.description | We justify the way of the direct quantization which means immediate quantization of a conservation law. It is shown that this approach is equivalent to introducing the super Hamiltonian on a minisuperspace in spirit of the Wheeler-DeWitt's approach. Then we will have: (i) all values are observable and have an obvious physical meaning and well-defined application domain; (ii) wave function is well-defined without time slicing and often can be exactly obtained; (iii) we can take off major mathematical troubles, and therefore, more complicate models can be considered exactly without the perturbation theory. | |
| dc.description | 5 pages, LaTeX | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9709030 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9709030 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/148874 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Theory of thin shells in general relativity: Equivalence of direct and Wheeler-DeWitt quantizations | |
| dc.type | text |