Search for Gravitational-Wave Bursts from Soft Gamma Repeaters

B P Abbott ,I Duke,F Grimaldi,H Overmier,S Klimenko,R Gouaty,C Echols,F Kawazoe,C Zhao,L Matone,D S Rabeling,T Etzel,P Ajith,M Samidi,S H Huttner,A Thüring,C Vorvick,P Shawhan,C Van Den Broeck,S C Mcguire,D Sellers,B Lantz,M Bastarrika,J Hanson,P T Beyersdorf,L Bogue,D Sigg,C C Wipf,I A Bilenko,B Sorazu,J Betzwieser,P Kwee,C Gray,M Fyffe,J Heefner,A M Sintes,A Sibley,K Kokeyama,B Bland,N Zotov,M Lormand,S Roddy,K Riles,S Mitra,K A Thorne,B C Barish,A C Searle,S Vass,A Grant,M Mageswaran,H Ward,M Landry,E Hirose,D Lodhia,D Fazi,D Hoak,B J J Slagmolen,N A Lockerbie,S Yoshida,M V Plissi,G Mcivor,V Sandberg,H Bantilan,N A Robertson,K Mailand,G Traylor,R W P Drever,D Barker,L Cardenas,R S Ottens,R M Martin,E Goetz,T Z Summerscales,G Mendell,M Pedraza,H Mukhopadhyay,P Savov,S E Whitcomb,B Sears,P Lu,A Effler,T P Bodiya,J Ulmen,P J Sutton,L Sancho De La Jordana,P Schwinberg,M Sung,G Billingsley,J Garofoli,P Ehrens,M Rakhmanov,K Kawabe,S B Anderson,M Degree,S P Vyachanin,E Myers,K Wette,E K Gustafson,A M Gretarsson,P Charlton,V Boschi,B Rivera,A S Sengupta,B Moe,R Frey,W G Anderson,S Penn,H Rehbein,M Macinnis,I Gholami,I Leonor,A Bullington,H Fehrmann,C Aulbert,H Vahlbruch,E Chalkley,J S Kissel,A Stochino,P Sarin,R Mittleman,S Sakata,A Cumming,K Bayer,F Donovan,K D Giardina,J M Hallam,S Meshkov,B Barr,G Moreno,D Ugolini,M Brinkmann,H Radkins,E Maros,L Wallace,G Mcintyre,N Rainer,V P Mitrofanov,V Leonhardt,M Ramsunder,R Wooley,M Hennessy,J Zweizig,S Márka,J Minelli,A Perreca,J A Giaime,E E Doomes,K V Tokmakov,A G Wiseman,W Kells,A M Rogan,B Machenschalk,V Quetschke,B F Whiting,C Pankow,R Bork,G Brunet,V Kondrashov,T Casebolt,R Desalvo,M Weinert,I Yakushin,S Giampanis,N Gehrels,R M Cutler,P Armor,V V Frolov,Z Márka,J N Marx,R Gustafson,V Parameshwaraiah,M A Barton,R A Mercer,N Fotopoulos,M Guenther,K Mason,T Hayler,E Black,K L Dooley,W Tyler,Ju Li ,Adrian C Melissinos ,I S Heng,Y Aso,R O’Shaughnessy,M Trias,S Desai,M M Fejer,A Buonanno,K Somiya,A J Weinstein ,N Mavalvala,J R Smith,C Wilkinson,John M Miller ,J Markowitz,D B Kozak ,James Dalrymple ,S W Ballmer ,J B Kanner ,C Messenger ,P Lindquist,H Yamamoto,L Blackburn,Masahiro Ito ,E D Harstad ,F J Raab ,A F Brooks ,A W Heptonstall ,K Ryan,R Weiss,P A Willems,S Hild,P J King ,A Lazzarini,R Grosso,J D E Creighton,D H Reitze,W Winkler,G H Ogin ,Malcolm B Gray ,A Vecchio,Ana Cecilia Rodríguez ,R Vaulin,R Mccarthy,David J Hosken ,S Sato,R Schilling,V Sannibale,M R Smith,O Miyakawa,V Mandic,B Hage,R L Byer,Robert W Taylor ,Jianshu Cao ,D B Tanner,D J Ottaway,P Patel,G Mitselmakher,T Nash,J Münch ,H J Pletsch,G Allen,J Worden,Kirk Mckenzie ,R Jones,L Zhang,T T Fricke ,H Grote,G M Harry ,P Russell,B S Sathyaprakash,A Nishizawa,M C Díaz ,J Hough,B J Owen,L Williams,S Goßler ,N Christensen,T Meier,R L Ward ,S M Aston ,M E Zucker ,W Wu,Z Yan,Seiji Kawamura ,G S Davies ,R Khan,S Babak,S M Scott,Laurent Ruet ,F Y Khalili ,J Slutsky,M Pitkin,D C Coyne ,R Kopparapu ,R Conte,P Kalmus,D I Jones,R J S Greenhalgh,J G Rollins ,D J A Mckechan ,D R Ingram ,N D Smith,J Dickson,A S Markosyan ,G Newton,M Hewitson,C Kim,N Leindecker,L Cunningham,C Torres,T R Corbitt ,B F Schutz,R J Dupuis,H R Williams,I M Pinto,H Lück,O Burmeister,D Meyers,P Aufmuth,V Dergachev,R M S Schofield ,David Blair ,S Grünewald ,A L Stuver ,R S Amin ,C Barker,B Johnson,Gabriela González ,T M Evans ,J G Dwyer,J T Whelan,Antonio Lucianetti ,J Harms,R Route,Sajal Mukherjee ,K X Sun ,B Allen,I Bartos,R Stone,K Mossavi,S D Barthelmy ,S Sinha,S Rowan,M C Araya ,F Matichard,Kenji Numata ,R Schnabel,J Nelson,A Dietz,J B Camp,I E Kozhevatov ,Eduardo Espinoza ,A Freise,K Danzmann,D Cook,P R Saulson,M Łubiński ,G Castaldi,V B Braginsky,L M Goggin ,C Robinson,K Hayama,G Woan,G Mueller,R Prix,D Clark,M A Arain,S Chelkowski,P Barriga,D A Hammer ,H Müller‐Ebhardt ,J H Romie ,T.w Pétrie ,K Hurley ,K Blackburn,J D Romano,K G Libbrecht ,Richard A Matzner ,E L Robinson,P R Brady,A Villar,Dimitri Kasprzyk ,P G Murray ,M Lei,Y Chen,J O’Dell,S Dhurandhar,J Veitch,J Degallaix,D E Mcclelland,D Debra,Ian Wilmut ,C Hanna,F Postiglione,S Wen,Rolf Riesen ,B Krishnan,S J Waldman,L Cadonati,B Willke,J A Clark ,M Principe,J Myers,W W Johnson,B O’Reilly,I W Martin ,J K Cannizzo ,J Brau ,Ping Koy Lam ,R X Adhikari ,Keisuke Goda ,Sascha Schediwy ,G Cagnoli,Karel Urbánek ,J Zhang,V Kalogera,K C Cannon ,Thomas Cokelaer ,H Lin,C I Torrie ,X Siemens,P Fritschel,A Rüdiger,R L Savage ,K A Strain,C Cepeda,D G Keppel,S Chatterji,Y Fan,R Biswas,D H Shoemaker,L C Stein,M Zanolin,J C Dumas ,Y Pan,M Van Der Sluys,C M Mow–Lowry ,S Reid,D Strom ,P J Veitch ,E Katsavounidis,M A Papa,S Gras,S Bose,F Seifert,Е А Хазанов ,H Armandula,M Mchugh,L S Finn,S Kamat,S Fairhurst,R Abbott,Hiroyuki R Takahashi ,D A Brown,A Ivanov,Gareth Jones ,John G Thacker ,S Saraf,S D Mohanty ,Kurt Flasch ,Kip S Thorne ,M Lang ,D M Palmer

doi:10.1103/physrevlett.101.211102

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 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.

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