Loop Quantum Gravity and the Cyclic Universe
| dc.creator | Bojowald, Martin | |
| dc.creator | Maartens, Roy | |
| dc.creator | Singh, Parampreet | |
| dc.date | 2004-07-14 | |
| dc.date | 2004-09-23 | |
| dc.date.accessioned | 2026-07-07T04:17:11Z | |
| dc.date.available | 2026-07-07T04:17:11Z | |
| dc.description | Loop quantum gravity introduces strong non-perturbative modifications to the dynamical equations in the semi-classical regime, which are responsible for various novel effects, including resolution of the classical singularity in a Friedman universe. Here we investigate the modifications for the case of a cyclic universe potential, assuming that we can apply the four-dimensional loop quantum formalism within the effective four-dimensional theory of the cyclic scenario. We find that loop quantum effects can dramatically alter the near-collision dynamics of the cyclic scenario. In the kinetic-dominated collapse era, the scalar field is effectively frozen by loop quantum friction, so that the branes approach collision and bounce back without actual collision. | |
| dc.description | 6 pages, 4 figures; v2: minor changes to match PRD version | |
| dc.identifier | https://arxiv.org/abs/hep-th/0407115 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0407115 | |
| dc.identifier | Phys.Rev. D70 (2004) 083517 | |
| dc.identifier | doi:10.1103/PhysRevD.70.083517 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/52649 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Loop Quantum Gravity and the Cyclic Universe | |
| dc.type | text |