Search for high frequency gravitational-wave bursts in the first calendar year of LIGO's fifth science run
B. P. Abbott,R. Adhikari,P. Ajith,B. Allen,G. Allen,R. S. Amin,S. B. Anderson,W. G. Anderson,M. A. Arain,M. Araya,H. Armandula,P. Armor,Y. Aso,S. Aston,P. Aufmuth,C. Aulbert,S. Babak,P. Baker,S. Ballmer,C. Barker,D. Barker,B. Barr,P. Barriga,L. Barsotti,M. Benacquista,I. Bartos,R. Bassiri,M. Bastarrika,B. Behnke, M. Benacquista, J. Betzwieser,P. T. Beyersdorf,I. A. Bilenko,G. Billingsley,R. Biswas,E. Black,J. K. Blackburn,L. Blackburn, D. Blair,B. Bland,T. P. Bodiya,L. Bogue, R. Bork,V. Boschi, S. Bose,P. R. Brady,V. B. Braginsky,J. E. Brau,D. O. Bridges, M. Brinkmann,A. F. Brooks,D. A. Brown,A. Brummit,G. Brunet,A. Bullington,A. Buonanno,O. Burmeister,R. L. Byer,L. Cadonati, J. B. Camp,J. Cannizzo,K. C. Cannon,J. Cao,L. Cardenas,S. Caride,G. Castaldi,S. Caudill,M. Cavaglia, C. Cepeda,T. Chalermsongsak,E. Chalkley,P. Charlton,S. Chatterji,S. Chelkowski,Y. Chen,N. Christensen,C. T. Y. Chung,D. Clark,J. Clark,J. H. Clayton,T. Cokelaer,C. N. Colacino,R. Conte,D. Cook,T. R. C. Corbitt,N. Cornish,D. Coward,D. C. Coyne,A. Di Credico,J. D. E. Creighton,T. D. Creighton,A. M. Cruise,R. M. Culter, A. Cumming, L. Cunningham,S. L. Danilishin, K. Danzmann,B. Daudert,G. Davies,E. J. Daw,D. DeBra,J. Degallaix,V. Dergachev,S. Desai,R. DeSalvo,S. Dhurandhar,M. Diaz,A. Dietz,F. Donovan,K. L. Dooley,E. E. Doomes, R. W. P. Drever,J. Dueck,I. Duke,J.-C. Dumas,J. G. Dwyer,C. Echols,M. Edgar,A. Effler,P. Ehrens,E. Espinoza,T. Etzel,M. Evans,T. Evans,S. Fairhurst,Y. Faltas,Y. Fan,D. Fazi,H. Fehrmann,Lee Samuel Finn,K. Flasch,S. Foley,C. Forrest,N. Fotopoulos,A. Franzen,M. Frede,M. Frei,Z. Frei,A. Freise,R. Frey,T. Fricke,P. Fritschel, V. V. Frolov,M. Fyffe,V. Galdi,J. A. Garofoli,I. Gholami,J. A. Giaime, S. Giampanis,K. D. Giardina,K. Goda,E. Goetz,L. M. Goggin,G. Gonzalez,M. L. Gorodetsky, S. Gossler,R. Gouaty,A. Grant,S. Gras,C. Gray,M. Gray,R. J. S. Greenhalgh,A. M. Gretarsson,F. Grimaldi, R. Grosso,H. Grote,S. Grunewald,M. Guenther,E. K. Gustafson,R. Gustafson, B. Hughey,J. M. Hallam,D. Hammer,G. D. Hammond,C. Hanna,J. Hanson,J. Harms,G. M. Harry, I. W. Harry,E. D. Harstad,K. Haughian, K. Hayama,J. Heefner,I. S. Heng,A. Heptonstall,M. Hewitson, S. Hild,E. Hirose, D. Hoak,K. A. Hodge,K. Holt,D. J. Hosken, J. Hough,D. Hoyland,B. Hughey,S. H. Huttner,D. R. Ingram,T. Isogai,M. Ito,A. Ivanov,B. Johnson, W. W. Johnson,D. I. Jones, G. Jones,R. Jones,L. Ju,P. Kalmus,V. Kalogera, S. Kandhasamy,J. Kanner,D. Kasprzyk, E. Katsavounidis, K. Kawabe,S. Kawamura, F. Kawazoe,W. Kells,D. G. Keppel,A. Khalaidovski,F. Y. Khalili,R. Khan,E. Khazanov,P. King,J. S. Kissel,S. Klimenko, K. Kokeyama,V. Kondrashov,R. Kopparapu,S. Koranda,D. Kozak,B. Krishnan,R. Kumar,P. Kwee, P. K. Lam,M. Landry,B. Lantz,A. Lazzarini,H. Lei,M. Lei,N. Leindecker,I. Leonor,C. Li,H. Lin,P. E. Lindquist,T. B. Littenberg,N. A. Lockerbie,D. Lodhia,M. Longo,M. Lormand,P. Lu,M. Lubinski,A. Lucianetti,H. Lueck, B. Machenschalk,M. MacInnis,M. Mageswaran, K. Mailand,I. Mandel,V. Mandic,S. Marka,Z. Marka,A. Markosyan,J. Markowitz,E. Maros,I. W. Martin,R. M. Martin,J. N. Marx,K. Mason,F. Matichard,L. Matone, R. A. Matzner, N. Mavalvala, R. McCarthy,D. E. McClelland,S. C. McGuire,M. McHugh,G. McIntyre,D. J. A. McKechan,K. McKenzie, M. Mehmet,A. Melatos,A. C. Melissinos,D. F. Menendez,G. Mendell,R. A. Mercer,S. Meshkov,C. Messenger,M. S. Meyer,J. Miller,J. Minelli,Y. Mino,V. P. Mitrofanov, G. Mitselmakher,R. Mittleman,O. Miyakawa,B. Moe,S. D. Mohanty, S. R. P. Mohapatra,G. Moreno,T. Morioka,K. Mors,K. Mossavi,C. MowLowry,G. Mueller,H. Muller-Ebhardt,D. Muhammad,S. Mukherjee,H. Mukhopadhyay,A. Mullavey,J. Munch, P. G. Murray,E. Myers,J. Myers,T. Nash,J. Nelson,G. Newton,A. Nishizawa,K. Numata,J. O’Dell,B. O’Reilly,R. O’Shaughnessy,E. Ochsner,G. H. Ogin,D. J. Ottaway,R. S. Ottens,H. Overmier,B. J. Owen,Y. Pan,C. Pankow,M. A. Papa,V. Parameshwaraiah,P. Patel,M. Pedraza,S. Penn,A. Perraca,V. Pierro,I. M. Pinto,M. Pitkin,H. J. Pletsch,M. V. Plissi,F. Postiglione,M. Principe,R. Prix,L. Prokhorov,O. Puncken,V. Quetschke,F. J. Raab,D. S. Rabeling,H. Radkins,P. Raffai,Z. Raics,N. Rainer,M. Rakhmanov,V. Raymond,C. M. Reed,T. Reed,H. Rehbein,S. Reid,D. H. Reitze,R. Riesen,K. Riles, B. Rivera,P. Roberts,N. A. Robertson,C. Robinson, E. L. Robinson,S. Roddy,C. Roever,J. Rollins, J. D. Romano,J. H. Romie,S. Rowan,A. Rudiger,P. Russell,K. Ryan,S. Sakata,L. Sancho de la Jordana,V. Sandberg,V. Sannibale,L. Santamaria,S. Saraf,P. Sarin,B. S. Sathyaprakash,S. Sato,M. Satterthwaite,P. R. Saulson,R. Savage,P. Savov,M. Scanlan,R. Schilling,R. Schnabel, R. Schofield,B. Schulz,B. F. Schutz,P. Schwinberg,J. Scott,S. M. Scott,A. C. Searle,B. Sears, F. Seifert,D. Sellers,A. S. Sengupta,A. Sergeev,B. Shapiro,P. Shawhan,D. H. Shoemaker,A. Sibley,X. Siemens,D. Sigg,S. Sinha,A. M. Sintes,B. J. J. Slagmolen,J. Slutsky,J. R. Smith, M. R. Smith, N. D. Smith,K. Somiya,B. Sorazu,A. Stein,L. C. Stein,S. Steplewski,A. Stochino,R. Stone,K. A. Strain,S. Strigin,A. Stroeer,A. L. Stuver,T. Z. Summerscales,K.-X. Sun,M. Sung,P. J. Sutton,G. P. Szokoly,D. Talukder,L. Tang,D. B. Tanner,S. P. Tarabrin,J. R. Taylor, R. Taylor,J. Thacker,K. A. Thorne,K. S. Thorne,A. Thuring,K. V. Tokmakov,C. Torres,C. Torrie,G. Traylor,M. Trias, D. Ugolini,J. Ulmen,K. Urbanek, H. Vahlbruch,M. Vallisneri,C. Van Den Broeck,M. V. van der Sluys,A. A. van Veggel,S. Vass,R. Vaulin,A. Vecchio,J. Veitch, P. Veitch,C. Veltkamp,J. Villadsen,A. Villar, C. Vorvick,S. P. Vyachanin,S. J. Waldman,L. Wallace,R. L. Ward,A. Weidner,M. Weinert, A. J. Weinstein,R. Weiss,L. Wen,S. Wen,K. Wette,J. T. Whelan,S. E. Whitcomb,B. F. Whiting,C. Wilkinson,P. A. Willems,H. R. Williams,L. Williams,B. Willke,I. Wilmut,L. Winkelmann, W. Winkler, C. C. Wipf,A. G. Wiseman,G. Woan,R. Wooley, J. Worden,W. Wu,I. Yakushin,H. Yamamoto,Z. Yan,S. Yoshida, M. Zanolin,J. Zhang,L. Zhang,C. Zhao, N. Zotov,M. E. Zucker,H. zur Muehlen,J. Zweizig
PHYSICAL REVIEW D（2009）
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摘要
We present an all-sky search for gravitational waves in the frequency range 1 to 6 kHz during the first calendar year of LIGO's fifth science run. This is the first untriggered LIGO burst analysis to be conducted above 3 kHz. We discuss the unique properties of interferometric data in this regime. 161.3 days of triple-coincident data were analyzed. No gravitational events above threshold were observed and a frequentist upper limit of 5.4 year(-1) on the rate of strong gravitational-wave bursts was placed at a 90% confidence level. Implications for specific theoretical models of gravitational-wave emission are also discussed.
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关键词
confidence level,quantum mechanics,high frequency,gravitational wave
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