High-Frequency Gravitational Waves from Hairy Black Holes
| dc.creator | Slagter, Reinoud J. | |
| dc.date | 1999-02-27 | |
| dc.date | 1999-03-05 | |
| dc.date.accessioned | 2026-07-07T03:33:00Z | |
| dc.date.available | 2026-07-07T03:33:00Z | |
| dc.description | We investigated the stability of the spherically symmetric non-abelian (Bartnik-McKinnon) black hole solution of the SU(2) Einstein-Yang-Mills system using the multiple-scale analysis. It is found, in contrast with the vacuum situation, that a spherically symmetric oscillatory perturbation to second order cannot be constructed. The singular behavior of gravitational waves is induced by the coupling of the gravitational waves to the Yang-Mills waves. | |
| dc.description | 5 pages in REVTEX. To appear in the proceedings of the XXXIV-th Rencontres de Moriond on "Gravitational Waves and Experimental Gravity", Les Arcs, France [January 23-30, 1999] | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9903001 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9903001 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/36450 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | High-Frequency Gravitational Waves from Hairy Black Holes | |
| dc.type | text |