Some consequences of the effective low-energy lagrangian for gravity
| dc.creator | Dobado, A. | |
| dc.creator | Lopez, A. | |
| dc.date | 1993-09-03 | |
| dc.date.accessioned | 2026-07-07T12:03:08Z | |
| dc.date.available | 2026-07-07T12:03:08Z | |
| dc.description | We consider the minimal low-energy action for gravity up to six derivatives which is renormalizable at the two-loop level modulo higher derivative corrections. Then we study the classical solutions corresponding to the Schwarzschild and the Robertson-Walker metrics. In the first case we find a singularity close to the gravitational radius and in the second case we find inflationary de Sitter solutions in absence of any matter or cosmological constant. | |
| dc.description | 13 pages | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9309221 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9309221 | |
| dc.identifier | Phys.Lett.B316:250-256,1993; ERRATUM-ibid.B321:435,1994 | |
| dc.identifier | doi:10.1016/0370-2693(93)90322-9 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/207678 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Some consequences of the effective low-energy lagrangian for gravity | |
| dc.type | text |