Evolution of Randall-Sundrum Black Holes in Dense Media
| dc.creator | Van Elewyck, Veronique | |
| dc.date | 2003-05-14 | |
| dc.date.accessioned | 2026-07-07T03:49:39Z | |
| dc.date.available | 2026-07-07T03:49:39Z | |
| dc.description | In the framework of Randall-Sundrum model, we discuss the evolution of microscopic black holes created by cosmic particles hitting a neutron or a strange star. We set up the general equations of evolution for the black hole mass and momentum in a dense medium, and discuss the possibility of collapse due to the black hole's growth inside the star. | |
| dc.description | 2 pages, Latex. Talk presented at the XXXVIIIth Rencontres de Moriond (Electroweak Interactions and Unified Theories), Les Arcs, France, March 15-22, 2003. To appear in the Proceedings | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0305147 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0305147 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/42487 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Evolution of Randall-Sundrum Black Holes in Dense Media | |
| dc.type | text |