Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-08-14
Phys.Rev.Lett.101:211102,2008
Astronomy and Astrophysics
Astrophysics
6 pages, 1 Postscript figure
Scientific paper
10.1103/PhysRevLett.101.211102
We present the results of a LIGO search for short-duration gravitational waves (GWs) associated with Soft Gamma Repeater (SGR) bursts. This is the first search sensitive to neutron star f-modes, usually considered the most efficient GW emitting modes. We find no evidence of GWs associated with any SGR burst in a sample consisting of the 27 Dec. 2004 giant flare from SGR 1806-20 and 190 lesser events from SGR 1806-20 and SGR 1900+14 which occurred during the first year of LIGO's fifth science run. GW strain upper limits and model-dependent GW emission energy upper limits are estimated for individual bursts using a variety of simulated waveforms. The unprecedented sensitivity of the detectors allows us to set the most stringent limits on transient GW amplitudes published to date. We find upper limit estimates on the model-dependent isotropic GW emission energies (at a nominal distance of 10 kpc) between 3x10^45 and 9x10^52 erg depending on waveform type, detector antenna factors and noise characteristics at the time of the burst. These upper limits are within the theoretically predicted range of some SGR models.
Barthelmy Scott
Gehrels Neil
Hurley Kevin Christopher
LIGO Scientific Collaboration
Palmer Dave
No associations
LandOfFree
Search for Gravitational Wave Bursts from Soft Gamma Repeaters does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Search for Gravitational Wave Bursts from Soft Gamma Repeaters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Search for Gravitational Wave Bursts from Soft Gamma Repeaters will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-650056