Dynamics of spin-2 fields in Kerr background geometries
| dc.creator | Krivan, W. | |
| dc.creator | Laguna, P. | |
| dc.creator | Papadopoulos, P. | |
| dc.date | 1997-01-15 | |
| dc.date.accessioned | 2026-07-07T03:31:26Z | |
| dc.date.available | 2026-07-07T03:31:26Z | |
| dc.description | We have developed a numerical method for evolving perturbations of rotating black holes. Solutions are obtained by integrating the Teukolsky equation written as a first-order in time, coupled system of equations, in a form that explicitly exhibits the radial characteristic directions. We follow the propagation of generic initial data through the burst, quasi-normal ringing and power-law tail phases. Future results may help to clarify the role of black hole angular momentum on signals produced during the final stages of black hole coalescence. | |
| dc.description | 3 pages LaTeX using sprocl.sty, 1 figure, to appear in: Proceedings of the 18th Texas Symposium on Relativistic Astrophysics (eds Olinto, Frieman and Schramm, World Scientific) | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9701036 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9701036 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/35862 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Dynamics of spin-2 fields in Kerr background geometries | |
| dc.type | text |