Phys. Rev. D
72,
082002
(2005)
[8 pages]
Search for gravitational waves from primordial black hole binary coalescences in the galactic halo
B. Abbott et al. LIGO Scientific Collaboration
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B. Abbott12, R. Abbott15, R. Adhikari13, A. Ageev20,27, B. Allen39, R. Amin34, S. B. Anderson12, W. G. Anderson29, M. Araya12, H. Armandula12, M. Ashley28, F. Asiri12,*, P. Aufmuth31, C. Aulbert1, S. Babak7, R. Balasubramanian7, S. Ballmer13, B. C. Barish12, C. Barker14, D. Barker14, M. Barnes12,†, B. Barr35, M. A. Barton12, K. Bayer13, R. Beausoleil26,‡, K. Belczynski23, R. Bennett35,§, S. J. Berukoff1,**, J. Betzwieser13, B. Bhawal12, I. A. Bilenko20, G. Billingsley12, E. Black12, K. Blackburn12, L. Blackburn13, B. Bland14, B. Bochner13,††, L. Bogue12, R. Bork12, S. Bose40, P. R. Brady39, V. B. Braginsky20, J. E. Brau37, D. A. Brown12, A. Bullington26, A. Bunkowski2,31, A. Buonanno6,‡‡, R. Burgess13, D. Busby12, W. E. Butler38, R. L. Byer26, L. Cadonati13, G. Cagnoli35, J. B. Camp21, C. A. Cantley35, L. Cardenas12, K. Carter15, M. M. Casey35, J. Castiglione34, A. Chandler12, J. Chapsky12,†, P. Charlton12,a, S. Chatterji13, S. Chelkowski2,31, Y. Chen6, V. Chickarmane16,b, D. Chin36, N. Christensen8, D. Churches7, T. Cokelaer7, C. Colacino33, R. Coldwell34, M. Coles15,c, D. Cook14, T. Corbitt13, D. Coyne12, J. D. E. Creighton39, T. D. Creighton12, D. R. M. Crooks35, P. Csatorday13, B. J. Cusack3, C. Cutler1, E. D’Ambrosio12, K. Danzmann2,31, E. Daw16,d, D. DeBra26, T. Delker1,34, V. Dergachev36, R. DeSalvo12, S. Dhurandhar11, A. Di Credico27, M. Díaz29, H. Ding12, R. W. P. Drever4, R. J. Dupuis35, J. A. Edlund12,†, P. Ehrens12, E. J. Elliffe35, T. Etzel12, M. Evans12, T. Evans15, S. Fairhurst39, C. Fallnich31, D. Farnham12, M. M. Fejer26, T. Findley25, M. Fine12, L. S. Finn28, K. Y. Franzen34, A. Freise2,f, R. Frey37, P. Fritschel13, V. V. Frolov15, M. Fyffe15, K. S. Ganezer5, J. Garofoli14, J. A. Giaime16, A. Gillespie12,g, K. Goda13, G. González16, S. Goßler31, P. Grandclément23,h, A. Grant35, C. Gray14, A. M. Gretarsson15, D. Grimmett12, H. Grote2, S. Grunewald1, M. Guenther14, E. Gustafson26,i, R. Gustafson36, W. O. Hamilton16, M. Hammond15, J. Hanson15, C. Hardham26, J. Harms19, G. Harry13, A. Hartunian12, J. Heefner12, Y. Hefetz13, G. Heinzel2, I. S. Heng31, M. Hennessy26, N. Hepler28, A. Heptonstall35, M. Heurs31, M. Hewitson2, S. Hild2, N. Hindman14, P. Hoang12, J. Hough35, M. Hrynevych12,j, W. Hua26, M. Ito37, Y. Itoh1, A. Ivanov12, O. Jennrich35,k, B. Johnson14, W. W. Johnson16, W. R. Johnston29, D. I. Jones28, L. Jones28, D. Jungwirth12,l, V. Kalogera23, E. Katsavounidis13, K. Kawabe14, S. Kawamura22, W. Kells12, J. Kern15,m, A. Khan15, S. Killbourn35, C. J. Killow35, C. Kim23, C. King12, P. King12, S. Klimenko34, S. Koranda39, K. Kötter31, J. Kovalik15,†, D. Kozak12, B. Krishnan1, M. Landry14, J. Langdale15, B. Lantz26, R. Lawrence13, A. Lazzarini12, M. Lei12, I. Leonor37, K. Libbrecht12, A. Libson8, P. Lindquist12, S. Liu12, J. Logan12,n, M. Lormand15, M. Lubinski14, H. Lück2,31, T. T. Lyons12,n, B. Machenschalk1, M. MacInnis13, M. Mageswaran12, K. Mailand12, W. Majid12,†, M. Malec2,31, F. Mann12, A. Marin13,o, S. Márka12,p, E. Maros12, J. Mason12,q, K. Mason13, O. Matherny14, L. Matone14, N. Mavalvala13, R. McCarthy14, D. E. McClelland3, M. McHugh18, J. W. C. McNabb28, G. Mendell14, R. A. Mercer33, S. Meshkov12, E. Messaritaki39, C. Messenger33, V. P. Mitrofanov20, G. Mitselmakher34, R. Mittleman13, O. Miyakawa12, S. Miyoki12,r, S. Mohanty29, G. Moreno14, K. Mossavi2, G. Mueller34, S. Mukherjee29, P. Murray35, J. Myers14, S. Nagano2, T. Nash12, R. Nayak11, G. Newton35, F. Nocera12, J. S. Noel40, P. Nutzman23, T. Olson24, B. O’Reilly15, D. J. Ottaway13, A. Ottewill39,s, D. Ouimette12,l, H. Overmier15, B. J. Owen28, Y. Pan6, M. A. Papa1, V. Parameshwaraiah14, A. Parameswaran1, C. Parameswariah15, M. Pedraza12, S. Penn10, M. Pitkin35, M. Plissi35, R. Prix1, V. Quetschke34, F. Raab14, H. Radkins14, R. Rahkola37, M. Rakhmanov34, S. R. Rao12, K. Rawlins13, S. Ray-Majumder39, V. Re33, D. Redding12,†, M. W. Regehr12,†, T. Regimbau7, S. Reid35, K. T. Reilly12, K. Reithmaier12, D. H. Reitze34, S. Richman13,t, R. Riesen15, K. Riles36, B. Rivera14, A. Rizzi15,u, D. I. Robertson35, N. A. Robertson26,35, L. Robison12, S. Roddy15, J. Rollins13, J. D. Romano7, J. Romie12, H. Rong34,g, D. Rose12, E. Rotthoff28, S. Rowan35, A. Rüdiger2, P. Russell12, K. Ryan14, I. Salzman12, V. Sandberg14, G. H. Sanders12,v, V. Sannibale12, B. Sathyaprakash7, P. R. Saulson27, R. Savage14, A. Sazonov34, R. Schilling2, K. Schlaufman28, V. Schmidt12,w, R. Schnabel19, R. Schofield37, B. F. Schutz1,7, P. Schwinberg14, S. M. Scott3, S. E. Seader40, A. C. Searle3, B. Sears12, S. Seel12, F. Seifert19, A. S. Sengupta11, C. A. Shapiro28,x, P. Shawhan12, D. H. Shoemaker13, Q. Z. Shu34,y, A. Sibley15, X. Siemens39, L. Sievers12,†, D. Sigg14, A. M. Sintes1,32, J. R. Smith2, M. Smith13, M. R. Smith12, P. H. Sneddon35, R. Spero12,†, G. Stapfer15, D. Steussy8, K. A. Strain35, D. Strom37, A. Stuver38, T. Summerscales28, M. C. Sumner12, P. J. Sutton12, J. Sylvestre12,z, A. Takamori12, D. B. Tanner34, H. Tariq12, I. Taylor7, R. Taylor35, R. Taylor12, K. A. Thorne28, K. S. Thorne6, M. Tibbits28, S. Tilav12,, M. Tinto4,†, K. V. Tokmakov20, C. Torres29, C. Torrie12, G. Traylor15, W. Tyler12, D. Ugolini30, C. Ungarelli33, M. Vallisneri6,, M. van Putten13, S. Vass12, A. Vecchio33, J. Veitch35, C. Vorvick14, S. P. Vyachanin20, L. Wallace12, H. Walther19, H. Ward35, B. Ware12,†, K. Watts15, D. Webber12, A. Weidner19, U. Weiland31, A. Weinstein12, R. Weiss13, H. Welling31, L. Wen12, S. Wen16, J. T. Whelan18, S. E. Whitcomb12, B. F. Whiting34, S. Wiley5, C. Wilkinson14, P. A. Willems12, P. R. Williams1,, R. Williams4, B. Willke31, A. Wilson12, B. J. Winjum28,**, W. Winkler2, S. Wise34, A. G. Wiseman39, G. Woan35, D. Woods1, R. Wooley15, J. Worden14, W. Wu34, I. Yakushin15, H. Yamamoto12, S. Yoshida25, K. D. Zaleski28, M. Zanolin13, I. Zawischa31,, L. Zhang11, R. Zhu1, N. Zotov17, M. Zucker15, and J. Zweizig12 (LIGO Scientific Collaboration)
1Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany 2Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany 3Australian National University, Canberra, 0200, Australia 4California Institute of Technology, Pasadena, California 91125, USA 5California State University Dominguez Hills, Carson, California 90747, USA 6Caltech-CaRT, Pasadena, California 91125, USA 7Cardiff University, Cardiff, CF2 3YB, United Kingdom 8Carleton College, Northfield, Minnesota 55057, USA 9Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA 10Hobart and William Smith Colleges, Geneva, New York 14456, USA 11Inter-University Centre for Astronomy and Astrophysics, Pune-411007, India 12LIGO—California Institute of Technology, Pasadena, California 91125, USA 13LIGO—Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA 14LIGO Hanford Observatory, Richland, Washington 99352, USA 15LIGO Livingston Observatory, Livingston, Louisiana 70754, USA 16Louisiana State University, Baton Rouge, Louisiana 70803, USA 17Louisiana Tech University, Ruston, Louisiana 71272, USA 18Loyola University, New Orleans, Louisiana 70118, USA 19Max Planck Institut für Quantenoptik, D-85748, Garching, Germany 20Moscow State University, Moscow, 119992, Russia 21NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA 22National Astronomical Observatory of Japan, Tokyo 181-8588, Japan 23Northwestern University, Evanston, Illinois 60208, USA 24Salish Kootenai College, Pablo, Montana 59855, USA 25Southeastern Louisiana University, Hammond, Louisiana 70402, USA 26Stanford University, Stanford, California 94305, USA 27Syracuse University, Syracuse, New York 13244, USA 28The Pennsylvania State University, University Park, Pennsylvania 16802, USA 29The University of Texas at Brownsville and Texas Southmost College, Brownsville, Texas 78520, USA 30Trinity University, San Antonio, Texas 78212, USA 31Universität Hannover, D-30167 Hannover, Germany 32Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain 33University of Birmingham, Birmingham, B15 2TT, United Kingdom 34University of Florida, Gainesville, Florida 32611, USA 35University of Glasgow, Glasgow, G12 8QQ, United Kingdom 36University of Michigan, Ann Arbor, Michigan 48109, USA 37University of Oregon, Eugene, Oregon 97403, USA 38University of Rochester, Rochester, New York 14627, USA 39University of Wisconsin–Milwaukee, Milwaukee, Wisconsin 53201, USA 40Washington State University, Pullman, Washington 99164, USA
Received 30 May 2005; published 25 October 2005
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.
© 2005 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevD.72.082002
DOI:
10.1103/PhysRevD.72.082002
PACS:
95.85.Sz, 04.80.Nn, 07.05.Kf, 95.35.+d
*Currently at Stanford Linear Accelerator Center. †Currently at Jet Propulsion Laboratory. ‡Permanent Address: HP Laboratories. §Currently at Rutherford Appleton Laboratory. **Currently at University of California, Los Angeles. ††Currently at Hofstra University. ‡‡Permanent Address: GReCO, Institut d’Astrophysique de Paris (CNRS). aCurrently at La Trobe University, Bundoora VIC, Australia. bCurrently at Keck Graduate Institute. cCurrently at National Science Foundation. dCurrently at University of Sheffield. eCurrently at Ball Aerospace Corporation. fCurrently at European Gravitational Observatory. gCurrently at Intel Corp. hCurrently at University of Tours, France. iCurrently at Lightconnect Inc. jCurrently at W. M. Keck Observatory. kCurrently at ESA Science and Technology Center. lCurrently at Raytheon Corporation. mCurrently at NM Institute of Mining and Technology/Magdalena Ridge Observatory Interferometer. nCurrently at Mission Research Corporation. oCurrently at Harvard University. pPermanent Address: Columbia University. qCurrently at Lockheed-Martin Corporation. rPermanent Address: University of Tokyo, Institute for Cosmic Ray Research. sPermanent Address: University College Dublin. tCurrently at Research Electro-Optics Inc. uCurrently at Institute of Advanced Physics, Baton Rouge, LA. vCurrently at Thirty Meter Telescope Project at Caltech. wCurrently at European Commission, DG Research, Brussels, Belgium. xCurrently at University of Chicago. yCurrently at LightBit Corporation. zPermanent Address: IBM Canada Ltd. Currently at University of Delaware. Permanent Address: Jet Propulsion Laboratory. Currently at Shanghai Astronomical Observatory. Currently at Laser Zentrum Hannover.
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