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

B. Abbott, R. Abbott, R. Adhikari, A. Ageev, B. Allen, R. Amin, S.B. Anderson, W.G. Anderson, M. Araya, H. Armandula, M. Ashley, F. Asiri, P. Aufmuth, C. Aulbert, S. Babak, R. Balasubramanian, S. Ballmer, B.C. Barish, C. Barker, D. BarkerM. Barnes, B. Barr, M.A. Barton, K. Bayer, R. Beausoleil, K. Belczynski, R. Bennett, S.J. Berukoff, J. Betzwieser, B. Bhawal, I.A. Bilenko, G. Billingsley, E. Black, K. Blackburn, L. Blackburn, B. Bland, B. Bochner, L. Bogue, R. Bork, S. Bose, P.R. Brady, V.B. Braginsky, J.E. Brau, D.A. Brown, A. Bullington, A. Bunkowski, A. Buonanno, R. Burgess, D. Busby, W.E. Butler, R.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, N. Christensen, D. Churches, T. Cokelaer, C. Colacino, R. Coldwell, M. Coles, D. Cook, T. Corbitt, D. Coyne, J.D.E. Creighton, T.D. Creighton, D.R.M. Crooks, P. Csatorday, B.J. Cusack, C. Cutler, E. D'Ambrosio, K. Danzmann, E. Daw, D. Debra, T. Delker, V. Dergachev, R. Desalvo, S. Dhurandhar, A.D. Credico, M. Díaz, H. Ding, R.W.P. Drever, R.J. Dupuis, J.A. Edlund, P. Ehrens, E.J. Elliffe, T. Etzel, M. Evans, T. Evans, S. Fairhurst, C. Fallnich, D. Farnham, M.M. Fejer, T. Findley, M. Fine, L.S. Finn, K.Y. Franzen, A. Freise, R. Frey, P. Fritschel, V.V. Frolov, M. Fyffe, K.S. Ganezer, J. Garofoli, J.A. Giaime, A. Gillespie, K. Goda, G. González, S. Goßler, P. Grandclément, A. Grant, C. Gray, A.M. Gretarsson, D. Grimmett, H. Grote, S. Grunewald, M. Guenther, E. Gustafson, R. Gustafson, W.O. Hamilton, M. Hammond, J. Hanson, C. Hardham, J. Harms, G. Harry, A. Hartunian, J. Heefner, Y. Hefetz, G. Heinzel, I.S. Heng, M. Hennessy, N. Hepler, A. Heptonstall, M. Heurs, M. Hewitson, S. Hild, N. Hindman, P. Hoang, J. Hough, M. Hrynevych, W. Hua, M. Ito, Y. Itoh, A. Ivanov, O. Jennrich, B. Johnson, W.W. Johnson, W.R. Johnston, D.I. Jones, L. Jones, D. Jungwirth, V. Kalogera, E. Katsavounidis, K. Kawabe, S. Kawamura, W. Kells, J. Kern, A. Khan, S. Killbourn, C.J. Killow, C. Kim, C. King, P. King, S. Klimenko, S. Koranda, K. Kötter, J. Kovalik, D. Kozak, B. Krishnan, M. Landry, J. Langdale, B. Lantz, R. Lawrence, A. Lazzarini, M. Lei, I. Leonor, K. Libbrecht, A. Libson, P. Lindquist, S. Liu, J. Logan, M. Lormand, M. Lubinski, H. Lück, T.T. Lyons, B. MacHenschalk, M. MacInnis, M. Mageswaran, K. Mailand, W. Majid, M. Malec, F. Mann, A. Marin, S. Márka, E. Maros, J. Mason, K. Mason, O. Matherny, L. Matone, N. Mavalvala, R. McCarthy, D.E. McClelland, M. 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, S. Miyoki, S. Mohanty, G. Moreno, K. Mossavi, G. Mueller, S. Mukherjee, P. Murray, J. Myers, S. Nagano, T. Nash, R. Nayak, G. Newton, F. Nocera, J.S. Noel, P. Nutzman, T. Olson, B. O'Reilly, D.J. Ottaway, A. Ottewill, D. Ouimette, H. Overmier, B.J. Owen, Y. Pan, M.A. Papa, V. Parameshwaraiah, A. Parameswaran, C. Parameswariah, M. Pedraza, S. Penn, M. Pitkin, M. Plissi, R. Prix, V. Quetschke, F. Raab, H. Radkins, R. Rahkola, M. Rakhmanov, S.R. Rao, K. Rawlins, S. Ray-Majumder, V. Re, D. Redding, M.W. Regehr, T. Regimbau, S. Reid, K.T. Reilly, K. Reithmaier, D.H. Reitze, S. Richman, R. Riesen, K. Riles, B. Rivera, A. Rizzi, D.I. Robertson, N.A. Robertson, L. Robison, S. Roddy, J. Rollins, J.D. Romano, J. Romie, H. Rong, D. Rose, E. Rotthoff, S. Rowan, A. Rüdiger, P. Russell, K. Ryan, I. Salzman, V. Sandberg, G.H. Sanders, V. Sannibale, B. Sathyaprakash, P.R. Saulson, R. Savage, A. Sazonov, R. Schilling, K. Schlaufman, V. Schmidt, R. Schnabel, R. Schofield, B.F. Schutz, P. Schwinberg, S.M. Scott, S.E. Seader, A.C. Searle, B. Sears, S. Seel, F. Seifert, A.S. Sengupta, C.A. Shapiro, P. Shawhan, D.H. Shoemaker, Q.Z. Shu, A. Sibley, X. Siemens, L. Sievers, D. Sigg, A.M. Sintes, J.R. Smith, M. Smith, M.R. Smith, P.H. Sneddon, R. Spero, G. Stapfer, D. Steussy, K.A. Strain, D. Strom, A. Stuver, T. Summerscales, M.C. Sumner, P.J. Sutton, J. Sylvestre, A. Takamori, D.B. Tanner, H. Tariq, I. Taylor, R. Taylor, R. Taylor, K.A. Thorne, K.S. Thorne, M. Tibbits, S. Tilav, M. Tinto, K.V. Tokmakov, C. Torres, C. 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. Weinstein, R. Weiss, H. Welling, L. Wen, S. Wen, J.T. Whelan, S.E. Whitcomb, B.F. Whiting, S. Wiley, C. Wilkinson, P.A. Willems, P.R. Williams, R. Williams, B. Willke, A. Wilson, B.J. Winjum, W. Winkler, S. Wise, A.G. Wiseman, G. Woan, D. Woods, R. Wooley, J. Worden, W. Wu, I. Yakushin, H. Yamamoto, S. Yoshida, K.D. Zaleski, M. Zanolin, I. Zawischa, L. Zhang, R. Zhu, N. Zotov, M. Zucker, J. Zweizig

Research output: Contribution to JournalArticleAcademicpeer-review

Abstract

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.
Original languageEnglish
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume72
Issue number8
DOIs
Publication statusPublished - 15 Oct 2005
Externally publishedYes

Fingerprint Dive into the research topics of 'Search for gravitational waves from primordial black hole binary coalescences in the galactic halo'. Together they form a unique fingerprint.

Cite this