Search for gravitational waves from primordial black hole binary coalescences in the galactic halo

B Abbott,R P Abbott,R Adhikari,A Ageev,B J Allen,R Amin,S Anderson,W Anderson,M Araya,H Armandula, M Ashley,F Asiri,P Aufmuth, C Aulbert, S Babak,R Balasubramanian, S Ballmer,B C Barish,Clyde F Barker,David J P Barker,M Barnes,B Barr, M A Barton,K Bayer,Raymond G Beausoleil,K Belczynski, Richard L Bennett,S Berukoff, J Betzwieser,B M Bhawal,I A Bilenko,G Billingsley,E Black,K Blackburn,L Blackburn,B Bland,Bruce S Bochner, L Bogue,R Bork,S K Bose,P R Brady,V B Braginsky,J Brau,D N Brown,A Bullington,A Bunkowski,A Buonanno,Richard C Burgess,D Busby, W R Butler,Robert L Byer,L Cadonati,G Cagnoli,J B Camp,C A Cantley,L Cardenas,K Carter,M M Casey,J Castiglione,A Chandler,J Chapsky,P Charlton,S Chatterji,S Chelkowski,Y Chen,V Chickarmane,D Chin,Neil D Christensen,D Churches,T Cokelaer,C N Colacino,R L Coldwell, Michael G H Coles, Dane B Cook,T Corbitt,D Coyne,J D E Creighton,T D Creighton,D R M Crooks,P Csatorday,B J Cusack,Curt Cutler, E Dambrosio,Karsten Danzmann,E J Daw,D Debra,T Delker,V Dergachev, R Desalvo,S Dhurandhar,Alessandra Di Credico, M A Diaz,Hongmei Ding,R W P Drever,R J Dupuis,J Edlund,P Ehrens,E Elliffe,T Etzel,M Evans,T E Evans,Stephen Fairhurst,Carsten Fallnich,D Farnham, M M Fejer,T Findley,Michael J Fine,L S Finn,K Y Franzen,A Freise,R Frey,P Fritschel, V V Frolov,M Fyffe,K Ganezer,J Garofoli,J A Giaime,Alan R Gillespie,K Goda,Gabriela Gonzalez,S Gosler,P Grandclement,A Grant,C Gray,A M Gretarsson,D Grimmett,H Grote,S Grunewald,M Guenther,E K Gustafson,R Gustafson,W Hamilton,Milton L Hammond,J Hanson,C Hardham,J Harms,G M Harry,A Hartunian,J Heefner,Y Hefetz,Gerhard Heinzel,I Heng,M Hennessy,N Hepler,A Heptonstall,M Heurs,M Hewitson, S Hild, N Hindman,P Hoang, J Hough,M Hrynevych,Wei Hua,M M Ito, Y Itoh,Andrew Ivanov,O Jennrich, B G H Johnson, W C Johnson,W R Johnston, David R Jones, L W Jones,D Jungwirth,V Kalogera,E Katsavounidis, K Kawabe,Shinichi Kawamura,W Kells,J Kern,A Khan,S Killbourn,C Killow,C Kim,Christopher King,P King,S Klimenko,S Koranda,K Kotter,J Kovalik,D Kozak,B Krishnan,Michael R Landry,J Langdale,B Lantz,R Lawrence,A Lazzarini,Ming Lei,I Leonor,Kenneth G Libbrecht,A Libson,P Lindquist,S Liu,Jennifer A Logan,M Lormand,M Lubinski,H Luck,Thomas Scott Lyons, B Machenschalk,Martin B Macinnis,M Mageswaran, K Mailand,W Majid,M Malec, F A Mann, Antonio F Garcia Marin,S Marka,E Maros,John Alden Mason,K Mason,O Matherny,L Matone, N Mavalvala,Richard E Mccarthy,D E Mcclelland,M I Mchugh,J W C Mcnabb,G Mendell,R A Mercer,S Meshkov,E Messaritaki,C Messenger, V P Mitrofanov, G Mitselmakher,R Mittleman,O Miyakawa,Shinji Miyoki,S Mohanty,Gustavo Adolfo Ligarreto Moreno,K Mossavi,G Mueller,S Mukherjee,P Murray,J Myers,Shigeo Nagano,T Nash,R Nayak, G L Newton,F Nocera,J S Noel,Philip Nutzman,Thomas P Olson,B Oreilly,D J Ottaway,Adrian C Ottewill,D Ouimette,H Overmier,B J Owen,Y Pan,M Papa,V Parameshwaraiah,A Parameswaran,C Parameswariah,M Pedraza,S Penn,M Pitkin, M V Plissi, R Prix,V Quetschke,F J Raab,H Radkins,R Rahkola,M Rakhmanov,S Rao,K Rawlins,S Raymajumder,V Re,David C Redding,Martin W Regehr, T Regimbau,S R Reid,K T Reilly,K Reithmaier,D H Reitze,S Richman,Rolf Riesen,K Riles,B Rivera,Andrea Rizzi, D S Robertson,N A Robertson,Leslie L Robison,S Roddy,J Rollins,J D Romano, J H Romie,H Rong,Douglas F Rose,E Rotthoff,Sheila Rowan,A Rudiger,Pamela J Russell,Kevin C Ryan, I Salzman,V Sandberg,Gary H Sanders,V Sannibale,B S Sathyaprakash, P R Saulson, R Savage,A Sazonov,R Schilling,Kevin C Schlaufman,V Schmidt,R F Schnabel, R Schofield,Bernard F Schutz,P Schwinberg,S M Scott,S E Seader,A C Searle,B Sears,S Seel,Frank Seifert,A S Sengupta,Charles L Shapiro,P Shawhan,D H Shoemaker,Qiang Shu,A Sibley,X Siemens,L Sievers,D Sigg,A M Sintes,John R Smith,Mark Raquet Jim Smith,P Sneddon,R Spero,G Stapfer,D Steussy,K A Strain,D Strom,A L Stuver,T Z Summerscales,M C Sumner,P J Sutton,J Sylvestre,Akiteru Takamori, Donald C Tanner,H Tariq,Imogen Taylor,R J Taylor,Kip S Thorne,M Tibbits,S Tilav,Massimo Tinto,K V Tokmakov,C Torres,C I Torrie,G Traylor,W Tyler, D Ugolini,C Ungarelli,M Vallisneri,M Van Putten,S Vass, A Vecchio,J Veitch,C Vorvick,S P Vyachanin,L Wallace,H Walther,H Ward,B Ware,K Watts,D Webber, A Weidner,U Weiland,A J R Weinstein,Robert E Weiss, H Welling,L Wen,Shuangchun Wen,J T Whelan,S E Whitcomb,B F Whiting,S Wiley,C D W Wilkinson,P A Willems, Patricia A M Williams,R Williams, B Willke, Andrew Wilson,B J Winjum,W Winkler, Steven M Wise,A G Wiseman,G Woan, David Woods,R Wooley,J Worden,Wuchen Wu,I Yakushin,H Yamamoto, S Yoshida,K Zaleski,M Zanolin,I Zawischa,Lun Zhang,Renyuan Zhu, N Zotov,M E Zucker,J Zweizig

PHYSICAL REVIEW D（2005）

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摘要

We use data from the second science run of the LIGO gravitational-wave detectors to search for the gravitational waves from primordial black hole binary coalescence with component masses in the range 0.2-1.0M. The analysis requires a signal to be found in the data from both LIGO observatories, according to a set of coincidence criteria. No inspiral signals were found. Assuming a spherical halo with core radius 5 kpc extending to 50 kpc containing nonspinning black holes with masses in the range 0.2-1.0M, we place an observational upper limit on the rate of primordial black hole coalescence of 63 per year per Milky Way halo (MWH) with 90% confidence.

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