Frame dragging in black hole-pulsar binaries
| dc.creator | Wex, N. | |
| dc.date | 1999-03-25 | |
| dc.date.accessioned | 2026-07-07T02:30:58Z | |
| dc.date.available | 2026-07-07T02:30:58Z | |
| dc.description | The discovery of frame-dragging effects in binary pulsar timing experiments requires a compact companion with sufficiently large spin. A pulsar orbiting a fast rotating black hole could provide an appropriate test system. In this paper we address questions concerning the identification of a black hole companion in such a system, the measurability of the frame dragging caused by the rotation of the black hole, and the measurability of the quadrupole moment, which would prove the presence of a Kerr black hole. | |
| dc.description | 6 pages, latex, 4 postscript figures. Talk given at "Gravitational Waves and Experimental Gravity," XXXIV Rencontres de Moriond, January 23-30, 1999 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9903389 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9903389 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14007 | |
| dc.subject | Astrophysics | |
| dc.title | Frame dragging in black hole-pulsar binaries | |
| dc.type | text |