Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts

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 i...

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Main Authors: Barnum, Sam, Barsotti, Lisa, Bodiya, Timothy Paul, Donovan, Frederick J., Essick, Reed Clasey, Evans, Matthew J., Foley, S., Fritschel, Peter K., Gras, Slawek, Isogai, Tomoki, Katsavounidis, Erotokritos, Kissel, Jeffrey S., Kwee, Patrick, Lee, J., MacInnis, Myron E., Mason, Kenneth R., Matichard, Fabrice, Mavalvala, Nergis, Mittleman, Richard K., Oelker, Eric Glenn, Shoemaker, David H., Vaulin, Ruslan, Vitale, Salvatore, Waldman, S. J., Weiss, Rainer, Wipf, Christopher, Zhang, Fan, Zucker, Michael E., Aggarwal, Nancy,Ph. D.Massachusetts Institute of Technology.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: American Physical Society 2014
Online Access:http://hdl.handle.net/1721.1/87745
https://orcid.org/0000-0002-0026-3877
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0003-2815-7387
https://orcid.org/0000-0001-6550-3045
https://orcid.org/0000-0002-4147-2560
https://orcid.org/0000-0001-8459-4499
https://orcid.org/0000-0001-8150-7062
https://orcid.org/0000-0002-2544-1596
https://orcid.org/0000-0003-2700-0767
https://orcid.org/0000-0003-1983-3187
https://orcid.org/0000-0001-8196-9267
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author Barnum, Sam
Barsotti, Lisa
Bodiya, Timothy Paul
Donovan, Frederick J.
Essick, Reed Clasey
Evans, Matthew J.
Foley, S.
Fritschel, Peter K.
Gras, Slawek
Isogai, Tomoki
Katsavounidis, Erotokritos
Kissel, Jeffrey S.
Kwee, Patrick
Lee, J.
MacInnis, Myron E.
Mason, Kenneth R.
Matichard, Fabrice
Mavalvala, Nergis
Mittleman, Richard K.
Oelker, Eric Glenn
Shoemaker, David H.
Vaulin, Ruslan
Vitale, Salvatore
Waldman, S. J.
Weiss, Rainer
Wipf, Christopher
Zhang, Fan
Zucker, Michael E.
Aggarwal, Nancy,Ph. D.Massachusetts Institute of Technology.
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Barnum, Sam
Barsotti, Lisa
Bodiya, Timothy Paul
Donovan, Frederick J.
Essick, Reed Clasey
Evans, Matthew J.
Foley, S.
Fritschel, Peter K.
Gras, Slawek
Isogai, Tomoki
Katsavounidis, Erotokritos
Kissel, Jeffrey S.
Kwee, Patrick
Lee, J.
MacInnis, Myron E.
Mason, Kenneth R.
Matichard, Fabrice
Mavalvala, Nergis
Mittleman, Richard K.
Oelker, Eric Glenn
Shoemaker, David H.
Vaulin, Ruslan
Vitale, Salvatore
Waldman, S. J.
Weiss, Rainer
Wipf, Christopher
Zhang, Fan
Zucker, Michael E.
Aggarwal, Nancy,Ph. D.Massachusetts Institute of Technology.
author_sort Barnum, Sam
collection MIT
description 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[superscript −2] to F < 1200  ergs cm[superscript −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.
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spelling mit-1721.1/877452022-09-29T21:47:15Z Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts Barnum, Sam Barsotti, Lisa Bodiya, Timothy Paul Donovan, Frederick J. Essick, Reed Clasey Evans, Matthew J. Foley, S. Fritschel, Peter K. Gras, Slawek Isogai, Tomoki Katsavounidis, Erotokritos Kissel, Jeffrey S. Kwee, Patrick Lee, J. MacInnis, Myron E. Mason, Kenneth R. Matichard, Fabrice Mavalvala, Nergis Mittleman, Richard K. Oelker, Eric Glenn Shoemaker, David H. Vaulin, Ruslan Vitale, Salvatore Waldman, S. J. Weiss, Rainer Wipf, Christopher Zhang, Fan Zucker, Michael E. Aggarwal, Nancy,Ph. D.Massachusetts Institute of Technology. Massachusetts Institute of Technology. Department of Physics MIT Kavli Institute for Astrophysics and Space Research LIGO (Observatory : Massachusetts Institute of Technology) Aggarwal, Nancy Barnum, Sam Barsotti, Lisa Bodiya, Timothy Paul Donovan, Frederick J. Essick, Reed Clasey Evans, Matthew J. Foley, S. Fritschel, Peter K. Gras, Slawek Isogai, Tomoki Katsavounidis, Erotokritos Kissel, Jeffrey S. Kwee, Patrick Lee, J. MacInnis, Myron E. Mason, Kenneth R. Matichard, Fabrice Mavalvala, Nergis Mittleman, Richard K. Oelker, Eric Glenn Shoemaker, David H. Vaulin, Ruslan Vitale, Salvatore Waldman, S. J. Weiss, Rainer Wipf, Christopher Zhang, Fan Zucker, Michael E. 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[superscript −2] to F < 1200  ergs cm[superscript −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. National Science Foundation (U.S.) United States. National Aeronautics and Space Administration Carnegie Trust David & Lucile Packard Foundation Research Corporation Alfred P. Sloan Foundation 2014-06-12T15:56:17Z 2014-06-12T15:56:17Z 2013-12 2013-10 Article http://purl.org/eprint/type/JournalArticle 1550-7998 1550-2368 http://hdl.handle.net/1721.1/87745 Aasi, J., J. Abadie, B. Abbott, R. Abbott, T. Abbott, M. Abernathy, T. Accadia, et al. “Search for Long-Lived Gravitational-Wave Transients Coincident with Long Gamma-Ray Bursts.” Phys. Rev. D 88, no. 12 (December 2013). © 2013 American Physical Society https://orcid.org/0000-0002-0026-3877 https://orcid.org/0000-0003-0219-9706 https://orcid.org/0000-0003-2815-7387 https://orcid.org/0000-0001-6550-3045 https://orcid.org/0000-0002-4147-2560 https://orcid.org/0000-0001-8459-4499 https://orcid.org/0000-0001-8150-7062 https://orcid.org/0000-0002-2544-1596 https://orcid.org/0000-0003-2700-0767 https://orcid.org/0000-0003-1983-3187 https://orcid.org/0000-0001-8196-9267 en_US http://dx.doi.org/10.1103/PhysRevD.88.122004 Physical Review D Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf American Physical Society American Physical Society
spellingShingle Barnum, Sam
Barsotti, Lisa
Bodiya, Timothy Paul
Donovan, Frederick J.
Essick, Reed Clasey
Evans, Matthew J.
Foley, S.
Fritschel, Peter K.
Gras, Slawek
Isogai, Tomoki
Katsavounidis, Erotokritos
Kissel, Jeffrey S.
Kwee, Patrick
Lee, J.
MacInnis, Myron E.
Mason, Kenneth R.
Matichard, Fabrice
Mavalvala, Nergis
Mittleman, Richard K.
Oelker, Eric Glenn
Shoemaker, David H.
Vaulin, Ruslan
Vitale, Salvatore
Waldman, S. J.
Weiss, Rainer
Wipf, Christopher
Zhang, Fan
Zucker, Michael E.
Aggarwal, Nancy,Ph. D.Massachusetts Institute of Technology.
Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts
title Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts
title_full Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts
title_fullStr Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts
title_full_unstemmed Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts
title_short Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts
title_sort search for long lived gravitational wave transients coincident with long gamma ray bursts
url http://hdl.handle.net/1721.1/87745
https://orcid.org/0000-0002-0026-3877
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0003-2815-7387
https://orcid.org/0000-0001-6550-3045
https://orcid.org/0000-0002-4147-2560
https://orcid.org/0000-0001-8459-4499
https://orcid.org/0000-0001-8150-7062
https://orcid.org/0000-0002-2544-1596
https://orcid.org/0000-0003-2700-0767
https://orcid.org/0000-0003-1983-3187
https://orcid.org/0000-0001-8196-9267
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