Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/51761
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DC Field | Value | Language |
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dc.contributor.author | Abbott, B. | - |
dc.contributor.author | Abbott, R. | - |
dc.contributor.author | Adhikari, R. | - |
dc.contributor.author | Ajith, P. | - |
dc.contributor.author | Allen, B. | - |
dc.contributor.author | Allen, G. | - |
dc.contributor.author | Amin, R. | - |
dc.contributor.author | Anderson, S. | - |
dc.contributor.author | Anderson, W. | - |
dc.contributor.author | Arain, M. | - |
dc.contributor.author | Araya, M. | - |
dc.contributor.author | Armandula, H. | - |
dc.contributor.author | Armor, P. | - |
dc.contributor.author | Aso, Y. | - |
dc.contributor.author | Aston, S. | - |
dc.contributor.author | Aufmuth, P. | - |
dc.contributor.author | Aulbert, C. | - |
dc.contributor.author | Babak, S. | - |
dc.contributor.author | Ballmer, S. | - |
dc.contributor.author | Bantilan, H. | - |
dc.contributor.author | et al. | - |
dc.date.issued | 2008 | - |
dc.identifier.citation | Physical Review Letters, 2008; 101(21):211102-1-211102-6 | - |
dc.identifier.issn | 0031-9007 | - |
dc.identifier.issn | 1079-7114 | - |
dc.identifier.uri | http://hdl.handle.net/2440/51761 | - |
dc.description.abstract | We present a LIGO search for short-duration gravitational waves (GWs) associated with soft gamma ray 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. 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 3×10⁴⁵ and 9×10⁵² 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. | - |
dc.description.statementofresponsibility | B. Abbott... D. J. Hosken... J. Munch... P. J. Veitch...et al. (LIGO Scientific Collaboration) | - |
dc.language.iso | en | - |
dc.publisher | American Physical Soc | - |
dc.rights | ©2008 American Physical Society | - |
dc.source.uri | http://dx.doi.org/10.1103/physrevlett.101.211102 | - |
dc.subject | LIGO Scientific Collaboration | - |
dc.title | Search for gravitational-wave bursts from soft gamma repeaters | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1103/PhysRevLett.101.211102 | - |
dc.relation.grant | ARC | - |
pubs.publication-status | Published | - |
dc.identifier.orcid | Ottaway, D. [0000-0001-6794-1591] | - |
dc.identifier.orcid | Veitch, P. [0000-0002-2597-435X] | - |
Appears in Collections: | Aurora harvest Environment Institute publications Physics publications |
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hdl_51761.pdf | Published version | 184.59 kB | Adobe PDF | View/Open |
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