No-Hair Theorems and Black Holes with Hair
| dc.creator | Heusler, Markus | |
| dc.date | 1996-10-11 | |
| dc.date.accessioned | 2026-07-07T03:31:19Z | |
| dc.date.available | 2026-07-07T03:31:19Z | |
| dc.description | The critical steps leading to the uniqueness theorem for the Kerr-Newman metric are reexamined in the light of the new black hole solutions with Yang-Mills and scalar hair. Various methods -- including scaling techniques, arguments based on energy conditions, conformal transformations and divergence identities -- are reviewed, and their range of application to selfgravitating scalar and non-Abelian gauge fields is discussed. In particular, the no-hair theorem is extended to harmonic mappings with arbitrary Riemannian target manifolds. (This paper is an extended version of an invited lecture held at the Journées Relativistes 96.) | |
| dc.description | 28 pages, latex | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9610019 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9610019 | |
| dc.identifier | Helv.Phys.Acta 69 (1996) 501-528 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/35819 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | No-Hair Theorems and Black Holes with Hair | |
| dc.type | text |