Gravitational radiation from long gamma-ray bursts
| dc.creator | van Putten, Maurice H. P. M. | |
| dc.date | 2001-02-11 | |
| dc.date.accessioned | 2026-07-07T03:25:41Z | |
| dc.date.available | 2026-07-07T03:25:41Z | |
| dc.description | Long gamma-ray bursts (GRBs) are probably powered by high-angular momentum black hole-torus systems in suspended accretion. The torus will radiate gravitational waves as non-axisymmetric instabilities develop. The luminosity in gravitational-wave emissions is expected to compare favorably with the observed isotropic equivalent luminosity in GRB-afterglow emissions. This predicts that long GRBs are potentially the most powerful LIGO/VIRGO burst-sources in the Universe. Their frequency-dynamics is characterized by a horizontal branch in the $\dot{f}(f)-$diagram. | |
| dc.description | submitted; Presented at the 2001 Aspen Winter Conference on Gravitational Waves, Feb. 4-10, 2001, Aspen | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0102043 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0102043 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/33802 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | Astrophysics | |
| dc.title | Gravitational radiation from long gamma-ray bursts | |
| dc.type | text |