Artigo
Search for gravitational radiation from intermediate mass black hole binaries in data from the second LIGO-Virgo joint science run
Registro en:
Physical Review D. College Pk: Amer Physical Soc, v. 89, n. 12, 15 p., 2012.
1550-7998
10.1103/PhysRevD.89.122003
WOS:000338661100001
WOS000338661100001.pdf
Autor
Aasi, J.
Abbott, B. P.
Abbott, R.
Abbott, T.
Abernathy, M. R.
Accadia, T.
Acernese, F.
Ackley, K.
Adams, C.
Adams, T.
Addesso, P.
Adhikari, R. X.
Affeldt, C.
Agathos, M.
Aggarwal, N.
Aguiar, O. D.
Ain, A.
Ajith, P.
Alemic, A.
Allen, B.
Allocca, A.
Amariutei, D.
Andersen, M.
Anderson, R.
Anderson, S. B.
Anderson, W. G.
Arai, K.
Araya, M. C.
Arceneaux, C.
Areeda, J.
Aston, S. M.
Astone, P.
Aufmuth, P.
Aulbert, C.
Austin, L.
Aylott, B. E.
Babak, S.
Baker, P. T.
Ballardin, G.
Ballmer, S. W.
Barayoga, J. C.
Barbet, M.
Barish, B. C.
Barker, D.
Barone, F.
Barr, B.
Barsotti, L.
Barsuglia, M.
Barton, M. A.
Bartos, I.
Bassiri, R.
Basti, A.
Batch, J. C.
Bauchrowitz, J.
Bauer, Th. S.
Bavigadda, V.
Behnke, B.
Bejger, M.
Beker, M. G.
Belczynski, C.
Bell, A. S.
Bell, C.
Bergmann, G.
Bersanetti, D.
Bertolini, A.
Betzwieser, J.
Beyersdorf, P. T.
Bilenko, I. A.
Billingsley, G.
Birch, J.
Biscans, S.
Bitossi, M.
Bizouard, M. A.
Black, E.
Blackburn, J. K.
Blackburn, L.
Blair, D.
Bloemen, S.
Blom, M.
Bock, O.
Bodiya, T. P.
Boer, M.
Bogaert, G.
Bogan, C.
Bond, C.
Bondu, F.
Bonelli, L.
Bonnand, R.
Bork, R.
Born, M.
Boschi, V.
Bose, Sukanta
Bosi, L.
Bradaschia, C.
Brady, P. R.
Braginsky, V. B.
Branchesi, M.
Brau, J. E.
Briant, T.
Bridges, D. O.
Brillet, A.
Brinkmann, M.
Brisson, V.
Brooks, A. F.
Brown, D. A.
Brown, D. D.
Brueckner, F.
Buchman, S.
Bulik, T.
Bulten, H. J.
Buonanno, A.
Burman, R.
Buskulic, D.
Buy, C.
Cadonati, L.
Cagnoli, G.
Calderon Bustillo, J.
Calloni, E.
Camp, J. B.
Campsie, P.
Cannon, K. C.
Canuel, B.
Cao, J.
Capano, C. D.
Carbognani, F.
Carbone, L.
Caride, S.
Castiglia, A.
Caudill, S.
Cavaglia, M.
Cavalier, F.
Cavalieri, R.
Celerier, C.
Cella, G.
Cepeda, C.
Cesarini, E.
Chakraborty, R.
Chalermsongsak, T.
Chamberlin, S. J.
Chao, S.
Charlton, P.
Chassande-Mottin, E.
Chen, X.
Chen, Y.
Chincarini, A.
Chiummo, A.
Cho, H. S.
Chow, J.
Christensen, N.
Chu, Q.
Chua, S. S. Y.
Chung, S.
Ciani, G.
Clara, F.
Clark, J. A.
Cleva, F.
Coccia, E.
Cohadon, P. -F.
Colla, A.
Collette, C.
Colombini, M.
Cominsky, L.
Constancio, M.
Conte, A.
Cook, D.
Corbitt, T. R.
Cordier, M.
Cornish, N.
Corpuz, A.
Corsi, A.
Costa, C. A.
Coughlin, M. W.
Coughlin, S.
Coulon, J. -P.
Countryman, S.
Couvares, P.
Coward, D. M.
Cowart, M.
Coyne, D. C.
Coyne, R.
Craig, K.
Creighton, J. D. E.
Crowder, S. G.
Cumming, A.
Cunningham, L.
Cuoco, E.
Dahl, K.
Dal Canton, T.
Damjanic, M.
Danilishin, S. L.
D'Antonio, S.
Danzmann, K.
Dattilo, V.
Daveloza, H.
Davier, M.
Davies, G. S.
Daw, E. J.
Day, R.
Dayanga, T.
Debreczeni, G.
Degallaix, J.
Deleglise, S.
Del Pozzo, W.
Denker, T.
Dent, T.
Dereli, H.
Dergachev, V.
De Rosa, R.
DeRosa, R. T.
DeSalvo, R.
Dhurandhar, S.
Diaz, M.
Di Fiore, L.
Di Lieto, A.
Di Palma, I.
Di Virgilio, A.
Donath, A.
Donovan, F.
Dooley, K. L.
Doravari, S.
Dossa, S.
Douglas, R.
Downes, T. P.
Drago, M.
Drever, R. W. P.
Driggers, J. C.
Du, Z.
Ducrot, M.
Dwyer, S.
Eberle, T.
Edo, T.
Edwards, M.
Effler, A.
Eggenstein, H.
Ehrens, P.
Eichholz, J.
Eikenberry, S. S.
Endroczi, G.
Essick, R.
Etzel, T.
Evans, M.
Evans, T.
Factourovich, M.
Fafone, V.
Fairhurst, S.
Fang, Q.
Farinon, S.
Farr, B.
Farr, W. M.
Favata, M.
Fehrmann, H.
Fejer, M. M.
Feldbaum, D.
Feroz, F.
Ferrante, I.
Ferrini, F.
Fidecaro, F.
Finn, L. S.
Fiori, I.
Fisher, R. P.
Flaminio, R.
Fournier, J. -D.
Franco, S.
Frasca, S.
Frasconi, F.
Frede, M.
Frei, Z.
Freise, A.
Frey, R.
Fricke, T. T.
Fritschel, P.
Frolov, V. V.
Fulda, P.
Fyffe, M.
Gair, J.
Gammaitoni, L.
Gaonkar, S.
Garufi, F.
Gehrels, N.
Gemme, G.
Genin, E.
Gennai, A.
Ghosh, S.
Giaime, J. A.
Giardina, K. D.
Giazotto, A.
Gill, C.
Gleason, J.
Goetz, E.
Goetz, R.
Gondan, L.
Gonzalez, G.
Gordon, N.
Gorodetsky, M. L.
Gossan, S.
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Gouaty, R.
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Gretarsson, A. M.
Groot, P.
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Grover, K.
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Gushwa, K.
Gustafson, E. K.
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Hammer, D.
Hammond, G.
Hanke, M.
Hanks, J.
Hanna, C.
Hanson, J.
Harms, J.
Harry, G. M.
Harry, I. W.
Harstad, E. D.
Hart, M.
Hartman, M. T.
Haster, C. -J.
Haughian, K.
Heidmann, A.
Heintze, M.
Heitmann, H.
Hello, P.
Hemming, G.
Hendry, M.
Heng, I. S.
Heptonstall, A. W.
Heurs, M.
Hewitson, M.
Hild, S.
Hoak, D.
Hodge, K. A.
Holt, K.
Hooper, S.
Hopkins, P.
Hosken, D. J.
Hough, J.
Howell, E. J.
Hu, Y.
Huerta, E.
Hughey, B.
Husa, S.
Huttner, S. H.
Huynh, M.
Huynh-Dinh, T.
Ingram, D. R.
Inta, R.
Isogai, T.
Ivanov, A.
Iyer, B. R.
Izumi, K.
Jacobson, M.
James, E.
Jang, H.
Jaranowski, P.
Ji, Y.
Jimenez-Forteza, F.
Johnson, W. W.
Jones, D. I.
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Ju, L.
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Kalmus, P.
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LIGO Sci Collaboration
Virgo Collaboration
Resumen
This paper reports on an unmodeled, all-sky search for gravitational waves from merging intermediate mass black hole binaries (IMBHB). The search was performed on data from the second joint science run of the LIGO and Virgo detectors (July 2009-October 2010) and was sensitive to IMBHBs with a range up to similar to 200 Mpc, averaged over the possible sky positions and inclinations of the binaries with respect to the line of sight. No significant candidate was found. Upper limits on the coalescence-rate density of nonspinning IMBHBs with total masses between 100 and 450 M-circle dot and mass ratios between 0.25 and 1 were placed by combining this analysis with an analogous search performed on data from the first LIGO-Virgo joint science run (November 2005-October 2007). The most stringent limit was set for systems consisting of two 88 M-circle dot black holes and is equal to 0.12 Mpc(-3) Myr(-1) at the 90% confidence level. This paper also presents the first estimate, for the case of an unmodeled analysis, of the impact on the search range of IMBHB spin configurations: the visible volume for IMBHBs with nonspinning components is roughly doubled for a population of IMBHBs with spins aligned with the binary's orbital angular momentum and uniformly distributed in the dimensionless spin parameter up to 0.8, whereas an analogous population with antialigned spins decreases the visible volume by similar to 20%. United States National Science Foundation for the construction and operation of the LIGO Laboratory Science and Technology Facilities Council of the United Kingdom Max-Planck-Society State of Niedersachsen/Germany Australian Research Council International Science Linkages program of the Commonwealth of Australia Council of Scientific and Industrial Research of India Istituto Nazionale di Fisica Nucleare of Italy Spanish Ministerio de Economia y Competitividad Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears Foundation for Fundamental Research on Matter Netherlands Organisation for Scientific Research Polish Ministry of Science and Higher Education FOCUS Programme of Foundation for Polish Science Royal Society Scottish Funding Council Scottish Universities Physics Alliance National Aeronautics and Space Administration OTKA of Hungary Lyon Institute of Origins (LIO) National Research Foundation of Korea Industry Canada Province of Ontario through the Ministry of Economic Development and Innovation National Science and Engineering Research Council Canada Carnegie Trust Leverhulme Trust David and Lucile Packard Foundation Research Corporation Alfred P. Sloan Foundation LIGO Calif Inst Technol, Pasadena, CA 91125 USA Louisiana State Univ, Baton Rouge, LA 70803 USA Univ Savoie, CNRS, IN2P3, Lab Annecy le Vieux Phys Particules LAPP, F-74941 Annecy Le Vieux, France Complesso Univ Monte S Angelo, Sez Napoli, Ist Nazl Fis Nucl, I-80126 Naples, Italy Univ Salerno, I-84084 Salerno, Italy Univ Florida, Gainesville, FL 32611 USA LIGO Livingston Observ, Livingston, LA 70754 USA Cardiff Univ, Cardiff CF24 3AA, S Glam, Wales Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany Nikhef, NL-1098 XG Amsterdam, Netherlands LIGO Massachusetts Inst Technol, Cambridge, MA 02139 USA Inst Nacl Pesquisas Espaciais, BR-12227010 Sao Jose Dos Campos, SP, Brazil Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India Tata Inst Fundamental Res, Bombay 400005, Maharashtra, India Syracuse Univ, Syracuse, NY 13244 USA Univ Wisconsin, Milwaukee, WI 53201 USA Leibniz Univ Hannover, D-30167 Hannover, Germany Ist Nazl Fis Nucl, Sez 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Hanyang Univ, Seoul 133791, South Korea IM PAN, PL-00956 Warsaw, Poland NCBJ, PL-05400 Otwock, Poland Inst Plasma Res, Bhat 382428, Gandhinagar, India Univ Melbourne, Melbourne, Vic 3010, Australia Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy Monash Univ, Clayton, Vic 3800, Australia Univ Strathclyde, SUPA, Glasgow G1 1XQ, Lanark, Scotland ESPCI, CNRS, F-75005 Paris, France Argentinian Gravitat Wave Grp, RA-5000 Cordoba, Argentina Univ Camerino, Dipartmento Fis, I-62032 Camerino, Italy Univ Texas Austin, Austin, TX 78712 USA Southern Univ, Baton Rouge, LA 70813 USA A&M Coll, Baton Rouge, LA 70813 USA Coll William & Mary, Williamsburg, VA 23187 USA IISER Kolkata, Mohanpur 741252, W Bengal, India Natl Inst Math Sci, Taejon 305390, South Korea Hobart & William Smith Coll, Geneva, NY 14456 USA RRCAT, Indore 452013, Madhya Pradesh, India Univ West Scotland, SUPA, Paisley PA1 2BE, Renfrew, Scotland Inst Astron, PL-65265 Zielona Gora, Poland Indian Inst Technol, Ahmadabad 382424, Gujarat, India Univ Estadual Paulista, Inst Fis Teor, Int Ctr Theoret Phys, South Amer Inst Res, BR-01140070 Sao Paulo, Brazil Andrews Univ, Berrien Springs, MI 49104 USA Trinity Univ, San Antonio, TX 78212 USA Univ Washington, Seattle, WA 98195 USA SE Louisiana Univ, Hammond, LA 70402 USA Abilene Christian Univ, Abilene, TX 79699 USA Univ Estadual Paulista, Inst Fis Teor, Int Ctr Theoret Phys, South Amer Inst Res, BR-01140070 Sao Paulo, Brazil