Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600-1000 Hz
J Abadie,B Abbott,Richard J Abbott, T D Abbott,M Abernathy,T Accadia,F Acernese,C Adams,R Adhikari,C Affeldt, M Agathos,Koh Agatsuma,P Ajith,Barry J Allen,E Amador Ceron, D Amariutei,S Anderson,W G Anderson,Kazuaki Arai,M A Arain,M Araya,S M Aston,P Astone,D Atkinson,P Aufmuth, C Aulbert, B E Aylott, S Babak,P Baker,G Ballardin,S Ballmer, J C B Barayoga,David J P Barker,F Barone,B Barr,L Barsotti,M Barsuglia,M A Barton,I Bartos,R Bassiri,M Bastarrika,A Basti, J Batch,J Bauchrowitz,Th Bauer, M Bebronne, Douglas L Beck,B Behnke,M Bejger,M G Beker,A S Bell,A Belletoile,I Belopolski,M Benacquista, J M Berliner,A Bertolini, J Betzwieser,N Beveridge,P T Beyersdorf,I A Bilenko,G Billingsley,J M Birch,R Biswas,M Bitossi,M A Bizouard,E Black,J K Blackburn,L Blackburn,D G Blair,B Bland,M Blom,O Bock,T P Bodiya, C Bogan,R Bondarescu,F Bondu,L Bonelli,R Bonnand,R Bork,Maaike Van Den Born,V Boschi, S Bose, L Bosi,B Bouhou,S Braccini,C Bradaschia,P R Brady,V B Braginsky,M Branchesi, J Brau,J Breyer,T Briant,D O Bridges,A Brillet, M Brinkmann,V Brisson,M Britzger,A F Brooks, D A Brown,T Bulik,H Bulten,A Buonanno,J Burguetcastell,D Buskulic,C Buy,Robert L Byer,L Cadonati,G Cagnoli,E Calloni,J B Camp,P Campsie,John K Cannizzo,K Cannon,B Canuel, Jun Cao,C D Capano,F Carbognani, Laura D Carbone,S Caride,Samuel P Caudill,Marco Cavaglia,F Cavalier,R P Cavalieri,G Cella, C Cepeda,E Cesarini,O Chaibi,T Chalermsongsak,P Charlton,E Chassandemottin,S Chelkowski,Wenbin Chen,Xu Chen,Y Chen,A Chincarini,A Chiummo,H S Cho,J Chow, N B Christensen,S S Y Chua,C T Y Chung,S Chung,G Ciani,F Clara,D Clark, Jane E Clark,J H Clayton,F Cleva,E Coccia,P F Cohadon,C N Colacino,J Colas,A Colla,M Colombini,A Conte,R Conte, David M Cook,T R Corbitt,M Cordier,Neil J Cornish,A Corsi,C A Costa,M W Coughlin,J P Coulon,P Couvares,D Coward,Marlon D Cowart,D Coyne,J D E Creighton,T D Creighton,A M Cruise, A Cumming, L Cunningham,E Cuoco,R M Cutler,K Dahl,S L Danilishin,Roger B Dannenberg,S Dantonio,Karsten Danzmann,V Dattilo,B Daudert,H Daveloza, M Davier,E J Daw, Robert M Day,T Dayanga,R De Rosa,D Debra,G Debreczeni,W Del Pozzo,M Del Prete,Thomas Dent,V Dergachev,R Derosa,R Desalvo,S Dhurandhar,L Di Fiore,A Di Lieto,I Di Palma,M Di Paolo Emilio,A Di Virgilio, M A Diaz,A Dietz,Frederick J Donovan,K L Dooley,M Drago, R W P Drever,J C Driggers,Zhihui Du,Jeancharles Dumas,Sandra Dwyer,T Eberle,M Edgar, M J Edwards,A Effler,P Ehrens, G Endroczi,R Engel,T Etzel, K R Evans,M Evans,T E Evans, M Factourovich,V Fafone,Stephen Fairhurst,Yaohui Fan,B F Farr,D Fazi,H Fehrmann,D Feldbaum,F Feroz,I Ferrante,F Fidecaro,L S Finn,I Fiori,R P Fisher,R Flaminio,M Flanigan,S Foley,E Forsi,L A Forte,N Fotopoulos,J D Fournier,J Franc,S Frasca,F Frasconi,M Frede,M Frei,Z Frei,A Freise,R Frey,T Fricke,D Friedrich,P Fritschel,V V Frolov,M Fujimoto,P Fulda,M Fyffe,Jonathan R Gair,M Galimberti,L Gammaitoni,Jose A Garcia,F Garufi,M Gaspar,G Gemme,R Geng,E Genin,A Gennai,Laszlo A Gergely,S Ghosh,J A Giaime, S Giampanis,K D Giardina,A Giazotto, S Gilcasanova,C Gill,J Gleason,E Goetz,L M Goggin,Gabriela Gonzalez,M L Gorodetsky,S Gosler,R Gouaty,C Graef,P B Graff,M Granata,A Grant,Slawomir Gras,C Gray,Nathanael S Gray, R J S Greenhalgh,A M Gretarsson,C Greverie, R Grosso,H Grote,S Grunewald,G Guidi, C Guido, Ravi Gupta,E K Gustafson,R Gustafson,Taekjip Ha,J M Hallam,D Hammer,G Hammond,John B Hanks,C Hanna, J V Hanson,J Harms,G M Harry,I W Harry,E D Harstad,M T Hartman,K Haughian,K Hayama, J F Hayau,J Heefner,A Heidmann,M Heintze,H Heitmann,P Hello,M Hendry,I S Heng,A Heptonstall,V Herrera,M Hewitson, S Hild, D Hoak,K A Hodge,K Holt, M Holtrop,T Hong,Shaun Hooper,D J Hosken, J Hough,Eric Howell,B Hughey,Sascha Husa,S H Huttner,T Huynhdinh,D R Ingram,R Inta,T Isogai,A Ivanov,Kouji Izumi,Mark Z Jacobson, E James,Yong Ju Jang,P Jaranowski,E Jesse,W Johnson,D I Jones, Geraint Jones, R Jones,L Ju,P I P Kalmus,V Kalogera, S Kandhasamy,Gungwon Kang,J B Kanner,Rangachar Kasturi,E Katsavounidis, W Katzman,H Kaufer,K Kawabe,S Kawamura, F Kawazoe,D Kelley,W Kells,D G Keppel,Zoltan Keresztes,A Khalaidovski,F Y Khalili,E A Khazanov,B K Kim,C Kim, Hansoo Kim,Kihong Kim,N Kim, Y M Kim,P J King,D L Kinzel,J S Kissel,S Klimenko, K Kokeyama, V N Kondrashov,S Koranda, W Z Korth,I Kowalska,D Kozak, O Kranz,V Kringel,S S Krishnamurthy,B Krishnan,Andrzej Krolak,Glenn D Kuehn,Rakesh Kumar,P Kwee,Ping Koy Lam,M Landry,B Lantz,N Lastzka, C Lawrie,A Lazzarini,P Leaci, C H Lee, H K Lee, J R Leong,I Leonor,N Leroy,N Letendre,J Li,T G F Li,N Liguori,P Lindquist,Y Liu, Zaochang Liu, N A Lockerbie,D Lodhia,M Lorenzini,V Loriette,M Lormand,G Losurdo, J Lough,Jianan Luan,M Lubinski,H Luck,A Lundgren,E Macdonald, B Machenschalk,M Macinnis, D M Macleod,M Mageswaran, K Mailand,E Majorana,I Maksimovic,N Man,I Mandel,V Mandic,M Mantovani,Alireza Marandi,Fabio Marchesoni,F Marion,S Marka,Z Marka,A S Markosyan,E Maros,J Marque, F Martelli,I Martin,Richard M Martin,J N Marx, K O Mason,A Masserot,F Matichard,L Matone,Richard A Matzner, N Mavalvala, G Mazzolo,Richard Mccarthy,D E Mcclelland,S C Mcguire,G J Mcintyre,J Mciver,D J A Mckechan,Sean T Mcwilliams,G D Meadors, M Mehmet,T Meier,A Melatos,A C Melissinos,G Mendell,R A Mercer,S Meshkov,C Messenger,M Meyer,H Miao,C Michel, L Milano,J Miller,Y Minenkov,V P Mitrofanov, G Mitselmakher,R Mittleman,O Miyakawa,B Moe,M Mohan,S Mohanty, S R P Mohapatra,D Moraru, Gabriel A Moreno,N Morgado,A Morgia, Tatsuya Mori,S R Morriss,S Mosca,K Mossavi,B Mours,C Mowlowry,C Mueller,Geoffrey A Mueller,S C Mukherjee,A Mullavey,H Mullerebhardt,Jean Charles Munch,Daniel S Murphy,P Murray, A Mytidis,T Nash, L Naticchioni, V Necula,J M Nelson,I Neri,G Newton,T Nguyen,A Nishizawa,A Nitz,F Nocera,D Nolting, M E Normandin, L K Nuttall,E Ochsner, J Odell,E Oelker,G H Ogin,J J Oh, S H Oh,B Oreilly,R Oshaughnessy,C Osthelder, C D Ott,D J Ottaway,R S Ottens,H Overmier, B J Owen, A L Page,G Pagliaroli,L Palladino,C Palomba,Y Pan,C Pankow,F Paoletti,M Papa,M Parisi,A 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Schilling,Robert D Schnabel, R Schofield,E Schreiber,B Schulz,Bernard F Schutz,P Schwinberg, Jerry B Scott,S M Scott,Frank Seifert,D Sellers,D Sentenac, Alexander M Sergeev,Daniel A Shaddock, M Shaltev,Bruce A Shapiro,P Shawhan,D H Shoemaker,A Sibley,X Siemens,D Sigg,Adam J Singer,Lianne Singer,A M Sintes,G Skelton,B J J Slagmolen,J Slutsky,J R Smith, Michael R Smith,R Smith, N D Smithlefebvre, K Somiya,B Sorazu,J Soto,F C Speirits,L Sperandio,Michael Stefszky,A Stein,L C Stein, E Steinert,J Steinlechner,S Steinlechner,S Steplewski,A Stochino,R Stone,K A Strain,S Strigin,A Stroeer,R Sturani,A L Stuver,T Z Summerscales,Mingyu Sung,S Susmithan,P J Sutton,B Swinkels,Mario Del Tacca,L Taffarello,D Talukder,D B Tanner,S P Tarabrin,J R Taylor,R Taylor,Paul S Thomas,Kip S Thorne,E Thrane,A Thuring,K V Tokmakov,C Tomlinson,A Toncelli,M Tonelli,O Torre,Clivia M Sotomayor Torres,C I Torrie,E Tournefier,F Travasso,G Traylor,Kingjet Tseng, D Ugolini, H Vahlbruch,G Vajente,J F J Van Den Brand,C Van Den Broeck,S Van Der Putten,A A Van Veggel,S Vass,M Vasuth,R Vaulin,M Vavoulidis, A Vecchio,G Vedovato,J Veitch,P J Veitch,C Veltkamp,D Verkindt,F Vetrano,A Vicere,A Villar,J Y Vinet,Salvatore Vitale,H Vocca,C Vorvick,S P Vyatchanin, A J Wade, L A Wade,Michael S Wade,S J Waldman,L Wallace,Y Wan,M Wang, Xiaoling Wang,Zhuo Wang,A Wanner,R L Ward,M Was,M Weinert,A J Weinstein,Robert H Weiss,L Wen,P Wessels,M West,T Westphal,K Wette,J T Whelan,S E Whitcomb,D J White,B F Whiting, C D W Wilkinson,P A Willems,L Williams,R Williams, B Willke,L Winkelmann, Wendi J Winkler, C C Wipf,A G Wiseman,H Wittel,G Woan,R Wooley, John K Worden,I Yakushin,H Yamamoto,Kazuhiko Yamamoto,C C Yancey, Huijuan Yang,D Yeatonmassey, S Yoshida,P Yu,M Yvert, A Zadrony,M Zanolin,J P Zendri,Fan Zhang,Liping Zhang,Weihua Zhang,C Zhao, N Zotov,M E Zucker,J Zweizig
PHYSICAL REVIEW D（2012）
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摘要
A stochastic background of gravitational waves is expected to arise from a superposition of many incoherent sources of gravitational waves, of either cosmological or astrophysical origin. This background is a target for the current generation of ground-based detectors. In this article we present the first joint search for a stochastic background using data from the LIGO and Virgo interferometers. In a frequency band of 600-1000 Hz, we obtained a 95% upper limit on the amplitude of Omega(GW)(f) = Omega(3)(f/900 Hz)(3), of Omega(3) < 0.32, assuming a value of the Hubble parameter of h(100) = 0.71. These new limits are a factor of seven better than the previous best in this frequency band.
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关键词
cosmology,astrophysics,frequencies,stochastic processes,gravitational waves
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