Constructing "hair" for the three charge hole
| dc.creator | Mathur, Samir D. | |
| dc.creator | Saxena, Ashish | |
| dc.creator | Srivastava, Yogesh K. | |
| dc.date | 2003-11-11 | |
| dc.date | 2003-11-13 | |
| dc.date.accessioned | 2026-07-07T11:32:14Z | |
| dc.date.available | 2026-07-07T11:32:14Z | |
| dc.description | It has been found that the states of the 2-charge extremal D1-D5 system are given by smooth geometries that have no singularity and no horizon individually, but a `horizon' does arise after `coarse-graining'. To see how this concept extends to the 3-charge extremal system, we construct a perturbation on the D1-D5 geometry that carries one unit of momentum charge $P$. The perturbation is found to be regular everywhere and normalizable, so we conclude that at least this state of the 3-charge system behaves like the 2-charge states. The solution is constructed by matching (to several orders) solutions in the inner and outer regions of the geometry. We conjecture the general form of `hair' expected for the 3-charge system, and the nature of the interior of black holes in general. | |
| dc.description | 37 pages, 7 figures LaTex, Minor revision in the discussion | |
| dc.identifier | https://arxiv.org/abs/hep-th/0311092 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0311092 | |
| dc.identifier | Nucl.Phys.B680:415-449,2004 | |
| dc.identifier | doi:10.1016/j.nuclphysb.2003.12.022 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/197525 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Constructing "hair" for the three charge hole | |
| dc.type | text |