Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/100065
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dc.contributor.author | Aasi, J. | - |
dc.contributor.author | Abadie, J. | - |
dc.contributor.author | Abbott, B. | - |
dc.contributor.author | Abbott, R. | - |
dc.contributor.author | Abbott, T. | - |
dc.contributor.author | Abernathy, M. | - |
dc.contributor.author | Accadia, T. | - |
dc.contributor.author | Acernese, F. | - |
dc.contributor.author | Adams, C. | - |
dc.contributor.author | Adams, T. | - |
dc.contributor.author | Adhikari, R. | - |
dc.contributor.author | Affeldt, C. | - |
dc.contributor.author | Agathos, M. | - |
dc.contributor.author | Aggarwal, N. | - |
dc.contributor.author | Aguiar, O. | - |
dc.contributor.author | Ajith, P. | - |
dc.contributor.author | Allen, B. | - |
dc.contributor.author | Allocca, A. | - |
dc.contributor.author | Amador Ceron, E. | - |
dc.contributor.author | Amariutei, D. | - |
dc.contributor.author | et al. | - |
dc.date.issued | 2013 | - |
dc.identifier.citation | Physical Review D: Particles, Fields, Gravitation and Cosmology, 2013; 88(12):122004-1-122004-13 | - |
dc.identifier.issn | 1550-7998 | - |
dc.identifier.issn | 1550-2368 | - |
dc.identifier.uri | http://hdl.handle.net/2440/100065 | - |
dc.description.abstract | Long gamma-ray bursts (GRBs) have been linked to extreme core-collapse supernovae from massive stars. Gravitational waves (GW) offer a probe of the physics behind long GRBs. We investigate models of long-lived (~10–1000 s) GW emission associated with the accretion disk of a collapsed star or with its protoneutron star remnant. Using data from LIGO’s fifth science run, and GRB triggers from the Swift experiment, we perform a search for unmodeled long-lived GW transients. Finding no evidence of GW emission, we place 90% confidence-level upper limits on the GW fluence at Earth from long GRBs for three waveforms inspired by a model of GWs from accretion disk instabilities. These limits range from F<3:5 ergs cm⁻2 to F<1200 ergs cm⁻2, depending on the GRB and on the model, allowing us to probe optimistic scenarios of GW production out to distances as far as ≈ 33 Mpc. Advanced detectors are expected to achieve strain sensitivities 10× better than initial LIGO, potentially allowing us to probe the engines of the nearest long GRBs. | - |
dc.description.statementofresponsibility | J. Aasi ... D.J. Hosken ... W. Kim ... E.J. King ... J. Munch ... D. J. Ottaway ... P. J. Veitch | - |
dc.language.iso | en | - |
dc.publisher | American Physical Soc | - |
dc.rights | © 2013 American Physical Society | - |
dc.source.uri | http://dx.doi.org/10.1103/physrevd.88.122004 | - |
dc.title | Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1103/PhysRevD.88.122004 | - |
dc.relation.grant | ARC | - |
pubs.publication-status | Published | - |
Appears in Collections: | Aurora harvest 3 IPAS publications |
Files in This Item:
File | Description | Size | Format | |
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hdl_100065.pdf | Published version | 752.62 kB | Adobe PDF | View/Open |
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