학술논문

Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run
Document Type
Working Paper
Author
The LIGO Scientific Collaborationthe Virgo CollaborationAbbott, B. P.Abbott, R.Abbott, T. D.Abernathy, M. R.Acernese, F.Ackley, K.Adams, C.Adams, T.Addesso, P.Adhikari, R. X.Adya, V. B.Affeldt, C.Agathos, M.Agatsuma, K.Aggarwal, N.Aguiar, O. D.Aiello, L.Ain, A.Ajith, P.Allen, B.Allocca, A.Altin, P. A.Ananyeva, A.Anderson, S. B.Anderson, W. G.Appert, S.Arai, K.Araya, M. C.Areeda, J. S.Arnaud, N.Arun, K. G.Ascenzi, S.Ashton, G.Ast, M.Aston, S. M.Astone, P.Aufmuth, P.Aulbert, C.Avila-Alvarez, A.Babak, S.Bacon, P.Bader, M. K. M.Baker, P. T.Baldaccini, F.Ballardin, G.Ballmer, S. W.Barayoga, J. C.Barclay, S. E.Barish, B. C.Barker, D.Barone, F.Barr, B.Barsotti, L.Barsuglia, M.Barta, D.Bartlett, J.Bartos, I.Bassiri, R.Basti, A.Batch, J. C.Baune, C.Bavigadda, V.Bazzan, M.Beer, C.Bejger, M.Belahcene, I.Belgin, M.Bell, A. S.Berger, B. K.Bergmann, G.Berry, C. P. L.Bersanetti, D.Bertolini, A.Betzwieser, J.Bhagwat, S.Bhandare, R.Bilenko, I. A.Billingsley, G.Billman, C. R.Birch, J.Birney, R.Birnholtz, O.Biscans, S.Biscoveanu, A. S.Bisht, A.Bitossi, M.Biwer, C.Bizouard, M. A.Blackburn, J. K.Blackman, J.Blair, C. D.Blair, D. G.Blair, R. M.Bloemen, S.Bock, O.Boer, M.Bogaert, G.Bohe, A.Bondu, F.Bonnand, R.Boom, B. A.Bork, R.Boschi, V.Bose, S.Bouffanais, Y.Bozzi, A.Bradaschia, C.Brady, P. R.Braginsky, V. B.Branchesi, M.Brau, J. E.Briant, T.Brillet, A.Brinkmann, M.Brisson, V.Brockill, P.Broida, J. E.Brooks, A. F.Brown, D. A.Brown, D. D.Brown, N. M.Brunett, S.Buchanan, C. C.Buikema, A.Bulik, T.Bulten, H. J.Buonanno, A.Buskulic, D.Buy, C.Byer, R. L.Cabero, M.Cadonati, L.Cagnoli, G.Cahillane, C.Bustillo, J. Calder'onCallister, T. A.Calloni, E.Camp, J. B.Canepa, M.Cannon, K. C.Cao, H.Cao, J.Capano, C. D.Capocasa, E.Carbognani, F.Caride, S.Diaz, J. CasanuevaCasentini, C.Caudill, S.Cavagli`a, M.Cavalier, F.Cavalieri, R.Cella, G.Cepeda, C. B.Baiardi, L. CerboniCerretani, G.Cesarini, E.Chamberlin, S. J.Chan, M.Chao, S.Charlton, P.Chassande-Mottin, E.Cheeseboro, B. D.Chen, H. Y.Chen, Y.Cheng, H. -P.Chincarini, A.Chiummo, A.Chmiel, T.Cho, H. S.Cho, M.Chow, J. H.Christensen, N.Chu, Q.Chua, A. J. K.Chua, S.Chung, S.Ciani, G.Clara, F.Clark, J. A.Cleva, F.Cocchieri, C.Coccia, E.Cohadon, P. -F.Colla, A.Collette, C. G.Cominsky, L.Constancio Jr., M.Conti, L.Cooper, S. J.Corbitt, T. R.Cornish, N.Corsi, A.Cortese, S.Costa, C. A.Coughlin, E.Coughlin, M. W.Coughlin, S. B.Coulon, J. -P.Countryman, S. T.Couvares, P.Covas, P. B.Cowan, E. E.Coward, D. M.Cowart, M. J.Coyne, D. C.Coyne, R.Creighton, J. D. E.Creighton, T. D.Cripe, J.Crowder, S. G.Cullen, T. J.Cumming, A.Cunningham, L.Cuoco, E.Canton, T. DalDanilishin, S. L.D'Antonio, S.Danzmann, K.Dasgupta, A.Costa, C. F. Da SilvaDattilo, V.Dave, I.Davier, M.Davies, G. S.Davis, D.Daw, E. J.Day, B.Day, R.De, S.DeBra, D.Debreczeni, G.Degallaix, J.De Laurentis, M.Del'eglise, S.Del Pozzo, W.Denker, T.Dent, T.Dergachev, V.De Rosa, R.DeRosa, R. T.DeSalvo, R.Devine, R. C.Dhurandhar, S.D'iaz, M. C.Di Fiore, L.Di Giovanni, M.Di Girolamo, T.Di Lieto, A.Di Pace, S.Di Palma, I.Di Virgilio, A.Doctor, Z.Dolique, V.Donovan, F.Dooley, K. L.Doravari, S.Dorrington, I.Douglas, R.'Alvarez, M. DovaleDownes, T. P.Drago, M.Drever, R. W. P.Driggers, J. C.Du, Z.Ducrot, M.Dwyer, S. E.Edo, T. B.Edwards, M. C.Effler, A.Eggenstein, H. -B.Ehrens, P.Eichholz, J.Eikenberry, S. S.Essick, R. C.Etienne, Z.Etzel, T.Evans, M.Evans, T. M.Everett, R.Factourovich, M.Fafone, V.Fair, H.Fairhurst, S.Fan, X.Farinon, S.Farr, B.Farr, W. M.Fauchon-Jones, E. J.Favata, M.Fays, M.Fehrmann, H.Fejer, M. M.Galiana, A. Fern'andezFerrante, I.Ferreira, E. C.Ferrini, F.Fidecaro, F.Fiori, I.Fiorucci, D.Fisher, R. P.Flaminio, R.Fletcher, M.Fong, H.Forsyth, S. S.Fournier, J. -D.Frasca, S.Frasconi, F.Frei, Z.Freise, A.Frey, R.Frey, V.Fries, E. M.Fritschel, P.Frolov, V. V.Fulda, P.Fyffe, M.Gabbard, H.Gadre, B. U.Gaebel, S. M.Gair, J. R.Gammaitoni, L.Gaonkar, S. G.Garufi, F.Gaur, G.Gayathri, V.Gehrels, N.Gemme, G.Genin, E.Gennai, A.George, J.Gergely, L.Germain, V.Ghonge, S.Ghosh, AbhirupGhosh, ArchismanGhosh, S.Giaime, J. A.Giardina, K. D.Giazotto, A.Gill, K.Glaefke, A.Goetz, E.Goetz, R.Gondan, L.Gonz'alez, G.Castro, J. M. GonzalezGopakumar, A.Gorodetsky, M. L.Gossan, S. E.Gosselin, M.Gouaty, R.Grado, A.Graef, C.Granata, M.Grant, A.Gras, S.Gray, C.Greco, G.Green, A. C.Groot, P.Grote, H.Grunewald, S.Guidi, G. M.Guo, X.Gupta, A.Gupta, M. K.Gushwa, K. E.Gustafson, E. K.Gustafson, R.Hacker, J. J.Hall, B. R.Hall, E. D.Hammond, G.Haney, M.Hanke, M. M.Hanks, J.Hanna, C.Hannam, M. D.Hanson, J.Hardwick, T.Harms, J.Harry, G. M.Harry, I. W.Hart, M. J.Hartman, M. T.Haster, C. -J.Haughian, K.Healy, J.Heidmann, A.Heintze, M. C.Heitmann, H.Hello, P.Hemming, G.Hendry, M.Heng, I. S.Hennig, J.Henry, J.Heptonstall, A. W.Heurs, M.Hild, S.Hoak, D.Hofman, D.Holt, K.Holz, D. E.Hopkins, P.Hough, J.Houston, E. A.Howell, E. J.Hu, Y. M.Huerta, E. A.Huet, D.Hughey, B.Husa, S.Huttner, S. H.Huynh-Dinh, T.Indik, N.Ingram, D. R.Inta, R.Isa, H. N.Isac, J. -M.Isi, M.Isogai, T.Iyer, B. R.Izumi, K.Jacqmin, T.Jani, K.Jaranowski, P.Jawahar, S.Jim'enez-Forteza, F.Johnson, W. W.Jones, D. I.Jones, R.Jonker, R. J. G.Ju, L.Junker, J.Kalaghatgi, C. V.Kalogera, V.Kandhasamy, S.Kang, G.Kanner, J. B.Karki, S.Karvinen, K. S.Kasprzack, M.Katsavounidis, E.Katzman, W.Kaufer, S.Kaur, T.Kawabe, K.K'ef'elian, F.Keitel, D.Kelley, D. B.Kennedy, R.Key, J. S.Khalili, F. Y.Khan, I.Khan, S.Khan, Z.Khazanov, E. A.Kijbunchoo, N.Kim, ChungleeKim, J. C.Kim, WhansunKim, W.Kim, Y. -M.Kimbrell, S. J.King, E. J.King, P. J.Kirchhoff, R.Kissel, J. S.Klein, B.Kleybolte, L.Klimenko, S.Koch, P.Koehlenbeck, S. M.Koley, S.Kondrashov, V.Kontos, A.Korobko, M.Korth, W. Z.Kowalska, I.Kozak, D. B.Kr"amer, C.; Kringel, V.Kr'olak, A.Kuehn, G.Kumar, P.Kumar, R.Kuo, L.Kutynia, A.Lackey, B. D.Landry, M.Lang, R. N.Lange, J.Lantz, B.Lanza, R. K.Lartaux-Vollard, A.Lasky, P. D.Laxen, M.Lazzarini, A.Lazzaro, C.Leaci, P.Leavey, S.Lebigot, E. O.Lee, C. H.Lee, H. K.Lee, H. M.Lee, K.Lehmann, J.Lenon, A.Leonardi, M.Leong, J. R.Leroy, N.Letendre, N.Levin, Y.Li, T. G. F.Libson, A.Littenberg, T. B.Liu, J.Lockerbie, N. A.Lombardi, A. L.London, L. T.Lord, J. E.Lorenzini, M.Loriette, V.Lormand, M.Losurdo, G.Lough, J. D.Lovelace, G.L"uck, H.; Lundgren, A. P.Lynch, R.Ma, Y.Macfoy, S.Machenschalk, B.MacInnis, M.Macleod, D. M.Magaña-Sandoval, F.Majorana, E.Maksimovic, I.Malvezzi, V.Man, N.Mandic, V.Mangano, V.Mansell, G. L.Manske, M.Mantovani, M.Marchesoni, F.Marion, F.M'arka, S.M'arka, Z.Markosyan, A. S.Maros, E.Martelli, F.Martellini, L.Martin, I. W.Martynov, D. V.Mason, K.Masserot, A.Massinger, T. J.Masso-Reid, M.Mastrogiovanni, S.Matas, A.Matichard, F.Matone, L.Mavalvala, N.Mazumder, N.McCarthy, R.McClelland, D. E.McCormick, S.McGrath, C.McGuire, S. C.McIntyre, G.McIver, J.McManus, D. J.McRae, T.McWilliams, S. T.Meacher, D.Meadors, G. D.Meidam, J.Melatos, A.Mendell, G.Mendoza-Gandara, D.Mercer, R. A.Merilh, E. L.Merzougui, M.Meshkov, S.Messenger, C.Messick, C.Metzdorff, R.Meyers, P. M.Mezzani, F.Miao, H.Michel, C.Middleton, H.Mikhailov, E. E.Milano, L.Miller, A. L.Miller, A.Miller, B. B.Miller, J.Millhouse, M.Minenkov, Y.Ming, J.Mirshekari, S.Mishra, C.Mitra, S.Mitrofanov, V. P.Mitselmakher, G.Mittleman, R.Moggi, A.Mohan, M.Mohapatra, S. R. P.Montani, M.Moore, B. C.Moore, C. J.Moraru, D.Moreno, G.Morriss, S. R.Mours, B.Mow-Lowry, C. M.Mueller, G.Muir, A. W.Mukherjee, ArunavaMukherjee, D.Mukherjee, S.Mukund, N.Mullavey, A.Munch, J.Muniz, E. A. M.Murray, P. G.Mytidis, A.Napier, K.Nardecchia, I.Naticchioni, L.Nelemans, G.Nelson, T. J. N.Neri, M.Nery, M.Neunzert, A.Newport, J. M.Newton, G.Nguyen, T. T.Nielsen, A. B.Nissanke, S.Nitz, A.Noack, A.Nocera, F.Nolting, D.Normandin, M. E. N.Nuttall, L. K.Oberling, J.Ochsner, E.Oelker, E.Ogin, G. H.Oh, J. J.Oh, S. H.Ohme, F.Oliver, M.Oppermann, P.Oram, Richard J.O'Reilly, B.O'Shaughnessy, R.Ottaway, D. J.Overmier, H.Owen, B. J.Pace, A. E.Page, J.Pai, A.Pai, S. A.Palamos, J. R.Palashov, O.Palomba, C.Pal-Singh, A.Pan, H.Pankow, C.Pannarale, F.Pant, B. C.Paoletti, F.Paoli, A.Papa, M. A.Paris, H. R.Parker, W.Pascucci, D.Pasqualetti, A.Passaquieti, R.Passuello, D.Patricelli, B.Pearlstone, B. L.Pedraza, M.Pedurand, R.Pekowsky, L.Pele, A.Penn, S.Perez, C. J.Perreca, A.Perri, L. M.Pfeiffer, H. P.Phelps, M.Piccinni, O. J.Pichot, M.Piergiovanni, F.Pierro, V.Pillant, G.Pinard, L.Pinto, I. M.Pitkin, M.Poe, M.Poggiani, R.Popolizio, P.Post, A.Powell, J.Prasad, J.Pratt, J. W. W.Predoi, V.Prestegard, T.Prijatelj, M.Principe, M.Privitera, S.Prodi, G. A.Prokhorov, L. G.Puncken, O.Punturo, M.Puppo, P.P"urrer, M.; Qi, H.Qin, J.Qiu, S.Quetschke, V.Quintero, E. A.Quitzow-James, R.Raab, F. J.Rabeling, D. S.Radkins, H.Raffai, P.Raja, S.Rajan, C.Rakhmanov, M.Rapagnani, P.Raymond, V.Razzano, M.Re, V.Read, J.Regimbau, T.Rei, L.Reid, S.Reitze, D. H.Rew, H.Reyes, S. D.Rhoades, E.Ricci, F.Riles, K.Rizzo, M.Robertson, N. A.Robie, R.Robinet, F.Rocchi, A.Rolland, L.Rollins, J. G.Roma, V. J.Romano, J. D.Romano, R.Romie, J. H.Rosi'nska, D.Rowan, S.R"udiger, A.; Ruggi, P.Ryan, K.Sachdev, S.Sadecki, T.Sadeghian, L.Sakellariadou, M.Salconi, L.Saleem, M.Salemi, F.Samajdar, A.Sammut, L.Sampson, L. M.Sanchez, E. J.Sandberg, V.Sanders, J. R.Sassolas, B.Sathyaprakash, B. S.Saulson, P. R.Sauter, O.Savage, R. L.Sawadsky, A.Schale, P.Scheuer, J.Schlassa, S.Schmidt, E.Schmidt, J.Schmidt, P.Schnabel, R.Schofield, R. M. S.Sch"onbeck, A.; Schreiber, E.Schuette, D.Schutz, B. F.Schwalbe, S. G.Scott, J.Scott, S. M.Sellers, D.Sengupta, A. S.Sentenac, D.Sequino, V.Sergeev, A.Setyawati, Y.Shaddock, D. A.Shaffer, T. J.Shahriar, M. S.Shapiro, B.Shawhan, P.Sheperd, A.Shoemaker, D. H.Shoemaker, D. M.Siellez, K.Siemens, X.Sieniawska, M.Sigg, D.Silva, A. D.Singer, A.Singer, L. P.Singh, A.Singh, R.Singhal, A.Sintes, A. M.Slagmolen, B. J. J.Smith, B.Smith, J. R.Smith, R. J. E.Son, E. J.Sorazu, B.Sorrentino, F.Souradeep, T.Spencer, A. P.Srivastava, A. K.Staley, A.Steinke, M.Steinlechner, J.Steinlechner, S.Steinmeyer, D.Stephens, B. C.Stevenson, S. P.Stone, R.Strain, K. A.Straniero, N.Stratta, G.Strigin, S. E.Sturani, R.Stuver, A. L.Summerscales, T. Z.Sun, L.Sunil, S.Sutton, P. J.Swinkels, B. L.Szczepa'nczyk, M. J.Tacca, M.Talukder, D.Tanner, D. B.Tao, D.T'apai, M.Taracchini, A.Taylor, R.Theeg, T.Thomas, E. G.Thomas, M.Thomas, P.Thorne, K. A.Thrane, E.Tippens, T.Tiwari, S.Tiwari, V.Tokmakov, K. V.Toland, K.Tomlinson, C.Tonelli, M.Tornasi, Z.Torrie, C. I.T"oyr"a, D.; Travasso, F.Traylor, G.Trifir`o, D.Trinastic, J.Tringali, M. C.Trozzo, L.Tse, M.Tso, R.Turconi, M.Tuyenbayev, D.Ugolini, D.Unnikrishnan, C. S.Urban, A. L.Usman, S. A.Vahlbruch, H.Vajente, G.Valdes, G.van Bakel, N.van Beuzekom, M.Brand, J. F. J. van denBroeck, C. Van DenVander-Hyde, D. C.van der Schaaf, L.van Heijningen, J. V.van Veggel, A. A.Vardaro, M.Varma, V.Vass, S.Vas'uth, M.Vecchio, A.Vedovato, G.Veitch, J.Veitch, P. J.Venkateswara, K.Venugopalan, G.Verkindt, D.Vetrano, F.Vicer'e, A.Viets, A. D.Vinciguerra, S.Vine, D. J.Vinet, J. -Y.Vitale, S.Vo, T.Vocca, H.Vorvick, C.Voss, D. V.Vousden, W. D.Vyatchanin, S. P.Wade, A. R.Wade, L. E.Wade, M.Walker, M.Wallace, L.Walsh, S.Wang, G.Wang, H.Wang, M.Wang, Y.Ward, R. L.Warner, J.Was, M.Watchi, J.Weaver, B.Wei, L. -W.Weinert, M.Weinstein, A. J.Weiss, R.Wen, L.Wessels, P.Westphal, T.Wette, K.Whelan, J. T.Whiting, B. F.Whittle, C.Williams, D.Williams, R. D.Williamson, A. R.Willis, J. L.Willke, B.Wimmer, M. H.Winkler, W.Wipf, C. C.Wittel, H.Woan, G.Woehler, J.Worden, J.Wright, J. L.Wu, D. S.Wu, G.Yam, W.Yamamoto, H.Yancey, C. C.Yap, M. J.Yu, HangYu, HaocunYvert, M.zny, A. Zadro.Zangrando, L.Zanolin, M.Zendri, J. -P.Zevin, M.Zhang, L.Zhang, M.Zhang, T.Zhang, Y.Zhao, C.Zhou, M.Zhou, Z.Zhu, S. J.Zhu, X. J.Zucker, M. E.Zweizig, J.
Source
Phys. Rev. Lett. 118, 121101 (2017)
Subject
General Relativity and Quantum Cosmology
Astrophysics - Cosmology and Nongalactic Astrophysics
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
A wide variety of astrophysical and cosmological sources are expected to contribute to a stochastic gravitational-wave background. Following the observations of GW150914 and GW151226, the rate and mass of coalescing binary black holes appear to be greater than many previous expectations. As a result, the stochastic background from unresolved compact binary coalescences is expected to be particularly loud. We perform a search for the isotropic stochastic gravitational-wave background using data from Advanced LIGO's first observing run. The data display no evidence of a stochastic gravitational-wave signal. We constrain the dimensionless energy density of gravitational waves to be $\Omega_0<1.7\times 10^{-7}$ with 95% confidence, assuming a flat energy density spectrum in the most sensitive part of the LIGO band (20-86 Hz). This is a factor of ~33 times more sensitive than previous measurements. We also constrain arbitrary power-law spectra. Finally, we investigate the implications of this search for the background of binary black holes using an astrophysical model for the background.
Comment: 13 pages, 6 figures