Multidimensional Sigma-Model with Black Holes and p-Branes
| dc.creator | Rainer, Martin | |
| dc.date | 1999-12-02 | |
| dc.date.accessioned | 2026-07-07T03:33:45Z | |
| dc.date.available | 2026-07-07T03:33:45Z | |
| dc.description | The bosonic content of string theory in curved background of multidimensional structure with p-branes has a systematic geometrical description as an effective sigma-model of gravity in lower dimension (say 3+1) with additional interacting dilatonic and p-brane fields. If the target-space is locally symmetric, solutions with intersecting p-branes can be found. Some static solutions are p-brane generalizations of black holes (including the standard Reissner-Nordstr"om class), which allow the prediction of detectable features of the higher-dimensional p-brane geometry via scaling properties of black hole thermal properties. E.g. the Hawking temperature T_H depends critically on the p-brane intersection topology. | |
| dc.description | 10 pages, latex & AMS symb., presented at ERE 99 (Bilbao) | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9912012 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9912012 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/36699 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Multidimensional Sigma-Model with Black Holes and p-Branes | |
| dc.type | text |