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dc.contributor.authorBarsotti, Lisa
dc.contributor.authorBlackburn, Lindy L.
dc.contributor.authorBodiya, Timothy Paul
dc.contributor.authorCao, Jianshu
dc.contributor.authorCorbitt, Thomas R.
dc.contributor.authorDonovan, Frederick J.
dc.contributor.authorDuke, I.
dc.contributor.authorEvans, Matthew J.
dc.contributor.authorFoley, Stephany
dc.contributor.authorFritschel, Peter K.
dc.contributor.authorHarry, Gregory
dc.contributor.authorHughey, Barbara
dc.contributor.authorKatsavounidis, Erotokritos
dc.contributor.authorMacInnis, Myron E.
dc.contributor.authorMarkowitz, Jared John
dc.contributor.authorMason, Kenneth R.
dc.contributor.authorMatichard, Fabrice
dc.contributor.authorMavalvala, Nergis
dc.contributor.authorMittleman, Richard K.
dc.contributor.authorSarin, P.
dc.contributor.authorShapiro, B.
dc.contributor.authorShoemaker, David H.
dc.contributor.authorSmith, N. D.
dc.contributor.authorStein, Andrew J.
dc.contributor.authorStein, Leo Chaim
dc.contributor.authorWaldman, Samuel J.
dc.contributor.authorWeiss, Rainer
dc.contributor.authorWipf, Christopher C.
dc.contributor.authorZucker, Michael E.
dc.date.accessioned2011-05-31T15:00:27Z
dc.date.available2011-05-31T15:00:27Z
dc.date.issued2011-03
dc.date.submitted2010-11
dc.identifier.issn1550-7998
dc.identifier.issn1550-2368
dc.identifier.urihttp://hdl.handle.net/1721.1/63136
dc.description.abstractThe physical mechanisms responsible for pulsar timing glitches are thought to excite quasinormal mode oscillations in their parent neutron star that couple to gravitational-wave emission. In August 2006, a timing glitch was observed in the radio emission of PSR B0833-45, the Vela pulsar. At the time of the glitch, the two colocated Hanford gravitational-wave detectors of the Laser Interferometer Gravitational-wave observatory (LIGO) were operational and taking data as part of the fifth LIGO science run (S5). We present the first direct search for the gravitational-wave emission associated with oscillations of the fundamental quadrupole mode excited by a pulsar timing glitch. No gravitational-wave detection candidate was found. We place Bayesian 90% confidence upper limits of 6.3×10-21 to 1.4×10-20 on the peak intrinsic strain amplitude of gravitational-wave ring-down signals, depending on which spherical harmonic mode is excited. The corresponding range of energy upper limits is 5.0×1044 to 1.3×1045  erg.en_US
dc.description.sponsorshipDavid & Lucile Packard Foundationen_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administrationen_US
dc.description.sponsorshipAlfred P. Sloan Foundationen_US
dc.description.sponsorshipCarnegie Trusten_US
dc.description.sponsorshipNational Science Foundation (U.S.)en_US
dc.description.sponsorshipResearch Corporationen_US
dc.description.sponsorshipLeverhulme Trusten_US
dc.language.isoen_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevD.83.042001en_US
dc.rightsArticle 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.en_US
dc.sourceAPSen_US
dc.titleSearch for gravitational waves associated with the August 2006 timing glitch of the Vela pulsaren_US
dc.typeArticleen_US
dc.identifier.citationAbadie, J. et al. (The LIGO Scientific Collaboration) "Search for gravitational waves associated with the August 2006 timing glitch of the Vela pulsar." Phys. Rev. D 83, 042001 (2011) [13 pages] © 2011 American Physical Society.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Chemistryen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.approverCao, Jianshu
dc.contributor.mitauthorCao, Jianshu
dc.contributor.mitauthorBarsotti, Lisa
dc.contributor.mitauthorBlackburn, Lindy L.
dc.contributor.mitauthorBodiya, Timothy Paul
dc.contributor.mitauthorCorbitt, Thomas R.
dc.contributor.mitauthorDonovan, Frederick J.
dc.contributor.mitauthorDuke, I.
dc.contributor.mitauthorEvans, Matthew J.
dc.contributor.mitauthorFoley, Stephany
dc.contributor.mitauthorFritschel, Peter K.
dc.contributor.mitauthorHarry, Gregory
dc.contributor.mitauthorHughey, Barbara
dc.contributor.mitauthorKatsavounidis, Erotokritos
dc.contributor.mitauthorMacInnis, Myron E.
dc.contributor.mitauthorMarkowitz, Jared John
dc.contributor.mitauthorMason, Kenneth R.
dc.contributor.mitauthorMatichard, Fabrice
dc.contributor.mitauthorMavalvala, Nergis
dc.contributor.mitauthorMittleman, Richard K.
dc.contributor.mitauthorSarin, P.
dc.contributor.mitauthorShapiro, B.
dc.contributor.mitauthorShoemaker, David H.
dc.contributor.mitauthorSmith, N. D.
dc.contributor.mitauthorStein, Andrew J.
dc.contributor.mitauthorStein, Leo Chaim
dc.contributor.mitauthorWaldman, Samuel J.
dc.contributor.mitauthorWeiss, Rainer
dc.contributor.mitauthorWipf, Christopher C.
dc.contributor.mitauthorZucker, Michael E.
dc.relation.journalPhysical Review Den_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsAbadie, J.; Abbott, B.; Abbott, R.; Adhikari, R.; Ajith, P.; Allen, B.; Allen, G.; Amador Ceron, E.; Amin, R.; Anderson, S.; Anderson, W.; Arain, M.; Araya, M.; Aso, Y.; Aston, S.; Aufmuth, P.; Aulbert, C.; Babak, S.; Baker, P.; Ballmer, S.; Barker, D.; Barr, B.; Barriga, P.; Barsotti, L.; Barton, M.; Bartos, I.; Bassiri, R.; Bastarrika, M.; Behnke, B.; Benacquista, M.; Bennett, M.; Betzwieser, J.; Beyersdorf, P.; Bilenko, I.; Billingsley, G.; Biswas, R.; Black, E.; Blackburn, J.; Blackburn, L.; Blair, D.; Bland, B.; Bock, O.; Bodiya, T.; Bondarescu, R.; Bork, R.; Born, M.; Bose, S.; Brady, P.; Braginsky, V.; Brau, J.; Breyer, J.; Bridges, D.; Brinkmann, M.; Britzger, M.; Brooks, A.; Brown, D.; Bullington, A.; Buonanno, A.; Burmeister, O.; Byer, R.; Cadonati, L.; Cain, J.; Camp, J.; Cannizzo, J.; Cannon, K.; Cao, J.; Capano, C.; Cardenas, L.; Caudill, S.; Cavaglià, M.; Cepeda, C.; Chalermsongsak, T.; Chalkley, E.; Charlton, P.; Chatterji, S.; Chelkowski, S.; Chen, Y.; Christensen, N.; Chua, S.; Chung, C.; Clark, D.; Clark, J.; Clayton, J.; Conte, R.; Cook, D.; Corbitt, T.; Cornish, N.; Coward, D.; Coyne, D.; Creighton, J.; Creighton, T.; Cruise, A.; Culter, R.; Cumming, A.; Cunningham, L.; Dahl, K.; Danilishin, S.; Danzmann, K.; Daudert, B.; Davies, G.; Daw, E.; Dayanga, T.; DeBra, D.; Degallaix, J.; Dergachev, V.; DeSalvo, R.; Dhurandhar, S.; Díaz, M.; Donovan, F.; Dooley, K.; Doomes, E.; Drever, R.; Driggers, J.; Dueck, J.; Duke, I.; Dumas, J.-C.; Edgar, M.; Edwards, M.; Effler, A.; Ehrens, P.; Etzel, T.; Evans, M.; Evans, T.; Fairhurst, S.; Faltas, Y.; Fan, Y.; Fazi, D.; Fehrmann, H.; Finn, L.; Flasch, K.; Foley, S.; Forrest, C.; Fotopoulos, N.; Frede, M.; Frei, M.; Frei, Z.; Freise, A.; Frey, R.; Fricke, T.; Friedrich, D.; Fritschel, P.; Frolov, V.; Fulda, P.; Fyffe, M.; Garofoli, J.; Ghosh, S.; Giaime, J.; Giampanis, S.; Giardina, K.; Goetz, E.; Goggin, L.; González, G.; Goßler, S.; Grant, A.; Gras, S.; Gray, C.; Greenhalgh, R.; Gretarsson, A.; Grosso, R.; Grote, H.; Grunewald, S.; Gustafson, E.; Gustafson, R.; Hage, B.; Hallam, J.; Hammer, D.; Hammond, G.; Hanna, C.; Hanson, J.; Harms, J.; Harry, G.; Harry, I.; Harstad, E.; Haughian, K.; Hayama, K.; Hayler, T.; Heefner, J.; Heng, I.; Heptonstall, A.; Hewitson, M.; Hild, S.; Hirose, E.; Hoak, D.; Hodge, K.; Holt, K.; Hosken, D.; Hough, J.; Howell, E.; Hoyland, D.; Hughey, B.; Husa, S.; Huttner, S.; Ingram, D.; Isogai, T.; Ivanov, A.; Johnson, W.; Jones, D.; Jones, G.; Jones, R.; Ju, L.; Kalmus, P.; Kalogera, V.; Kandhasamy, S.; Kanner, J.; Katsavounidis, E.; Kawabe, K.; Kawamura, S.; Kawazoe, F.; Kells, W.; Keppel, D.; Khalaidovski, A.; Khalili, F.; Khan, R.; Khazanov, E.; Kim, H.; King, P.; Kissel, J.; Klimenko, S.; Kokeyama, K.; Kondrashov, V.; Kopparapu, R.; Koranda, S.; Kozak, D.; Kringel, V.; Krishnan, B.; Kuehn, G.; Kullman, J.; Kumar, R.; Kwee, P.; Lam, P.; Landry, M.; Lang, M.; Lantz, B.; Lastzka, N.; Lazzarini, A.; Leaci, P.; Lei, M.; Leindecker, N.; Leonor, I.; Lin, H.; Lindquist, P.; Littenberg, T.; Lockerbie, N.; Lodhia, D.; Lormand, M.; Lu, P.; Lubinski, M.; Lucianetti, A.; Lück, H.; Lundgren, A.; Machenschalk, B.; MacInnis, M.; Mageswaran, M.; Mailand, K.; Mak, C.; Mandel, I.; Mandic, V.; Márka, S.; Márka, Z.; Markosyan, A.; Markowitz, J.; Maros, E.; Martin, I.; Martin, R.; Marx, J.; Mason, K.; Matichard, F.; Matone, L.; Matzner, R.; Mavalvala, N.; McCarthy, R.; McClelland, D.; McGuire, S.; McIntyre, G.; McKechan, D.; Mehmet, M.; Melatos, A.; Melissinos, A.; Mendell, G.; Menéndez, D.; Mercer, R.; Merrill, L.; Meshkov, S.; Messenger, C.; Meyer, M.; Miao, H.; Miller, J.; Mino, Y.; Mitra, S.; Mitrofanov, V.; Mitselmakher, G.; Mittleman, R.; Miyakawa, O.; Moe, B.; Mohanty, S.; Mohapatra, S.; Moreno, G.; Mors, K.; Mossavi, K.; MowLowry, C.; Mueller, G.; Müller-Ebhardt, H.; Mukherjee, S.; Mullavey, A.; Munch, J.; Murray, P.; Nash, T.; Nawrodt, R.; Nelson, J.; Newton, G.; Nishida, E.; Nishizawa, A.; O’Dell, J.; O’Reilly, B.; O’Shaughnessy, R.; Ochsner, E.; Ogin, G.; Oldenburg, R.; Ottaway, D.; Ottens, R.; Overmier, H.; Owen, B.; Page, A.; Pan, Y.; Pankow, C.; Papa, M.; Patel, P.; Pathak, D.; Pedraza, M.; Pekowsky, L.; Penn, S.; Peralta, C.; Perreca, A.; Pickenpack, M.; Pinto, I.; Pitkin, M.; Pletsch, H.; Plissi, M.; Postiglione, F.; Principe, M.; Prix, R.; Prokhorov, L.; Puncken, O.; Quetschke, V.; Raab, F.; Rabeling, D.; Radkins, H.; Raffai, P.; Raics, Z.; Rakhmanov, M.; Raymond, V.; Reed, C.; Reed, T.; Rehbein, H.; Reid, S.; Reitze, D.; Riesen, R.; Riles, K.; Roberts, P.; Robertson, N.; Robinson, C.; Robinson, E.; Roddy, S.; Röver, C.; Rollins, J.; Romano, J.; Romie, J.; Rowan, S.; Rüdiger, A.; Ryan, K.; Sakata, S.; Sammut, L.; Sancho de la Jordana, L.; Sandberg, V.; Sannibale, V.; Santamaría, L.; Santostasi, G.; Saraf, S.; Sarin, P.; Sathyaprakash, B.; Sato, S.; Satterthwaite, M.; Saulson, P.; Savage, R.; Schilling, R.; Schnabel, R.; Schofield, R.; Schulz, B.; Schutz, B.; Schwinberg, P.; Scott, J.; Scott, S.; Searle, A.; Seifert, F.; Sellers, D.; Sengupta, A.; Sergeev, A.; Shapiro, B.; Shawhan, P.; Shoemaker, D.; Sibley, A.; Siemens, X.; Sigg, D.; Sintes, A.; Skelton, G.; Slagmolen, B.; Slutsky, J.; Smith, J.; Smith, M.; Smith, N.; Somiya, K.; Sorazu, B.; Speirits, F.; Stein, A.; Stein, L.; Steplewski, S.; Stochino, A.; Stone, R.; Strain, K.; Strigin, S.; Stroeer, A.; Stuver, A.; Summerscales, T.; Sung, M.; Susmithan, S.; Sutton, P.; Szokoly, G.; Talukder, D.; Tanner, D.; Tarabrin, S.; Taylor, J.; Taylor, R.; Thorne, K.; Thorne, K.; Thüring, A.; Titsler, C.; Tokmakov, K.; Torres, C.; Torrie, C.; Traylor, G.; Trias, M.; Turner, L.; Ugolini, D.; Urbanek, K.; Vahlbruch, H.; Vallisneri, M.; Van Den Broeck, C.; van der Sluys, M.; van Veggel, A.; Vass, S.; Vaulin, R.; Vecchio, A.; Veitch, J.; Veitch, P.; Veltkamp, C.; Villar, A.; Vorvick, C.; Vyachanin, S.; Waldman, S.; Wallace, L.; Wanner, A.; Ward, R.; Wei, P.; Weinert, M.; Weinstein, A.; Weiss, R.; Wen, L.; Wen, S.; Wessels, P.; West, M.; Westphal, T.; Wette, K.; Whelan, J.; Whitcomb, S.; Whiting, B.; Wilkinson, C.; Willems, P.; Williams, H.; Williams, L.; Willke, B.; Wilmut, I.; Winkelmann, L.; Winkler, W.; Wipf, C.; Wiseman, A.; Woan, G.; Wooley, R.; Worden, J.; Yakushin, I.; Yamamoto, H.; Yamamoto, K.; Yeaton-Massey, D.; Yoshida, S.; Zanolin, M.; Zhang, L.; Zhang, Z.; Zhao, C.; Zotov, N.; Zucker, M.; Zweizig, J.; Buchner, S.en
dc.identifier.orcidhttps://orcid.org/0000-0003-0219-9706
dc.identifier.orcidhttps://orcid.org/0000-0001-6550-3045
dc.identifier.orcidhttps://orcid.org/0000-0002-4147-2560
dc.identifier.orcidhttps://orcid.org/0000-0001-7616-7809
dc.identifier.orcidhttps://orcid.org/0000-0001-8166-6805
dc.identifier.orcidhttps://orcid.org/0000-0001-8459-4499
dc.identifier.orcidhttps://orcid.org/0000-0002-2544-1596
dc.identifier.orcidhttps://orcid.org/0000-0003-1983-3187
dspace.mitauthor.errortrue
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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