From massive gravity to dark matter density
| dc.creator | Scharf, G. | |
| dc.date | 2007-11-23 | |
| dc.date | 2008-04-28 | |
| dc.date.accessioned | 2026-07-07T09:35:12Z | |
| dc.date.available | 2026-07-07T09:35:12Z | |
| dc.description | Massive gravity previously constructed as the spin-2 quantum gauge theory is studied in the classical limit. The vector-graviton field v which does not decouple in the limit of vanishing graviton mass gives rise to a modification of general relativity. The modified Schwarzschild solution contains a contribution which can be interpreted as the dark mass density. We calculate the density profile in the simplest spherically symmetric geometry. | |
| dc.description | 10 pages, further clarification, better numerical results | |
| dc.identifier | https://arxiv.org/abs/0711.3749 | |
| dc.identifier | http://arxiv.org/abs/0711.3749 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/159755 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | From massive gravity to dark matter density | |
| dc.type | text |