Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence

Detalhes bibliográficos
Autor(a) principal: Abbott, B. P.
Data de Publicação: 2016
Outros Autores: 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., Anderson, S. B., Anderson, W. G., Arai, K., Araya, M. C., Arceneaux, C. C., Areeda, J. S., Arnaud, N., Arun, K. G., Ascenzi, S., Ashton, G., Ast, M., Aston, S. M., Astone, P., Aufmuth, P., Aulbert, C., 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., Bejger, 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., Birch, J., Birney, R., Biscans, S., Bisht, A., Bitossi, M., Biwer, C., Bizouard, M. A., Blackburn, J. K., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bock, O., Boer, M., Bogaert, G., Bogan, C., Bohe, A., Bond, C., 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., Calderón Bustillo, J., Callister, T., Calloni, E., Camp, J. B., Cannon, K. C., Cao, J., Capano, C. D., Capocasa, E., Carbognani, F., Caride, S., Casanueva Diaz, J., Casentini, C., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. B., Cerboni Baiardi, L., Cerretani, G., Cesarini, E., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chassande-Mottin, E., Cheeseboro, B. D., Chen, H. Y., Chen, Y., Cheng, C., Chincarini, A., Chiummo, A., Cho, H. S., Cho, M., Chow, J. H., Christensen, N., Chu, Q., Chua, S., Chung, S., Ciani, G., Clara, F., Clark, J. A., Cleva, F., Coccia, E., Cohadon, P. F., Colla, A., Collette, C. G., Cominsky, L., Constancio, M., Conte, A., Conti, L., Cook, D., Corbitt, T. R., Cornish, N., Corsi, A., Cortese, S., Costa, C. A., Coughlin, M. W., Coughlin, S. B., Coulon, J. P., Countryman, S. T., Couvares, P., Cowan, E. E., Coward, D. M., Cowart, M. J., Coyne, D. C., Coyne, R., Craig, K., Creighton, J. D.E., Cripe, J., Crowder, S. G., Cumming, A., Cunningham, L., Cuoco, E., Dal Canton, T., Danilishin, S. L., D'Antonio, S., Danzmann, K., Darman, N. S., Dasgupta, A., Da Silva Costa, C. F., Dattilo, V., Dave, I., Davier, M., Davies, G. S., Daw, E. 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D., Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H. A.G., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., Garufi, F., Gaur, G., Gehrels, N., Gemme, G., Geng, P., Genin, E., Gennai, A., George, J., Gergely, L., Germain, V., Ghosh, Abhirup, Ghosh, Archisman, Ghosh, S., Giaime, J. A., Giardina, K. D., Giazotto, A., Gill, K., Glaefke, A., Goetz, E., Goetz, R., Gondan, L., González, G., Gonzalez Castro, J. M., Gopakumar, A., Gordon, N. A., Gorodetsky, M. L., Gossan, S. E., Gosselin, M., Gouaty, R., Grado, A., Graef, C., Graff, P. B., 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., Hanson, J., Hardwick, T., Harms, J., Harry, G. M., Harry, I. W., Hart, M. 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Y., Khan, I., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Kim, Chi-Woong, Kim, Chunglee, Kim, J., Kim, K., Kim, N., Kim, W., Kim, Y. M., Kimbrell, S. J., King, E. J., King, P. J., Kissel, J. S., Klein, B., Kleybolte, L., Klimenko, S., Koehlenbeck, S. M., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Kowalska, I., Kozak, D. B., Kringel, V., Królak, A., Krueger, C., Kuehn, G., Kumar, P., Kumar, R., Kuo, L., Kutynia, A., Lackey, B. D., Landry, M., Lange, J., Lantz, B., 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., Lenon, A., Leonardi, M., Leong, J. R., Leroy, N., Letendre, N., Levin, Y., Lewis, J. B., Li, T. G.F., Libson, A., Littenberg, T. B., Lockerbie, N. A., Lombardi, A. L., Lord, J. E., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lück, H., Lundgren, A. P., Lynch, R., Ma, Y., Machenschalk, B., Macinnis, M., Macleod, D. 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Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.94.064035
http://hdl.handle.net/11449/228230
Resumo: We compare GW150914 directly to simulations of coalescing binary black holes in full general relativity, including several performed specifically to reproduce this event. Our calculations go beyond existing semianalytic models, because for all simulations - including sources with two independent, precessing spins - we perform comparisons which account for all the spin-weighted quadrupolar modes, and separately which account for all the quadrupolar and octopolar modes. Consistent with the posterior distributions reported by Abbott et al. [Phys. Rev. Lett. 116, 241102 (2016)] (at the 90% credible level), we find the data are compatible with a wide range of nonprecessing and precessing simulations. Follow-up simulations performed using previously estimated binary parameters most resemble the data, even when all quadrupolar and octopolar modes are included. Comparisons including only the quadrupolar modes constrain the total redshifted mass Mz [64 M-82 M], mass ratio 1/q=m2/m1 [0.6,1], and effective aligned spin χeff [-0.3,0.2], where χeff=(S1/m1+S2/m2)·L/M. Including both quadrupolar and octopolar modes, we find the mass ratio is even more tightly constrained. Even accounting for precession, simulations with extreme mass ratios and effective spins are highly inconsistent with the data, at any mass. Several nonprecessing and precessing simulations with similar mass ratio and χeff are consistent with the data. Though correlated, the components' spins (both in magnitude and directions) are not significantly constrained by the data: the data is consistent with simulations with component spin magnitudes a1,2 up to at least 0.8, with random orientations. Further detailed follow-up calculations are needed to determine if the data contain a weak imprint from transverse (precessing) spins. For nonprecessing binaries, interpolating between simulations, we reconstruct a posterior distribution consistent with previous results. The final black hole's redshifted mass is consistent with Mf,z in the range 64.0 M-73.5 M and the final black hole's dimensionless spin parameter is consistent with af=0.62-0.73. As our approach invokes no intermediate approximations to general relativity and can strongly reject binaries whose radiation is inconsistent with the data, our analysis provides a valuable complement to Abbott et al. [Phys. Rev. Lett. 116, 241102 (2016)].
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spelling Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescenceWe compare GW150914 directly to simulations of coalescing binary black holes in full general relativity, including several performed specifically to reproduce this event. Our calculations go beyond existing semianalytic models, because for all simulations - including sources with two independent, precessing spins - we perform comparisons which account for all the spin-weighted quadrupolar modes, and separately which account for all the quadrupolar and octopolar modes. Consistent with the posterior distributions reported by Abbott et al. [Phys. Rev. Lett. 116, 241102 (2016)] (at the 90% credible level), we find the data are compatible with a wide range of nonprecessing and precessing simulations. Follow-up simulations performed using previously estimated binary parameters most resemble the data, even when all quadrupolar and octopolar modes are included. Comparisons including only the quadrupolar modes constrain the total redshifted mass Mz [64 M-82 M], mass ratio 1/q=m2/m1 [0.6,1], and effective aligned spin χeff [-0.3,0.2], where χeff=(S1/m1+S2/m2)·L/M. Including both quadrupolar and octopolar modes, we find the mass ratio is even more tightly constrained. Even accounting for precession, simulations with extreme mass ratios and effective spins are highly inconsistent with the data, at any mass. Several nonprecessing and precessing simulations with similar mass ratio and χeff are consistent with the data. Though correlated, the components' spins (both in magnitude and directions) are not significantly constrained by the data: the data is consistent with simulations with component spin magnitudes a1,2 up to at least 0.8, with random orientations. Further detailed follow-up calculations are needed to determine if the data contain a weak imprint from transverse (precessing) spins. For nonprecessing binaries, interpolating between simulations, we reconstruct a posterior distribution consistent with previous results. The final black hole's redshifted mass is consistent with Mf,z in the range 64.0 M-73.5 M and the final black hole's dimensionless spin parameter is consistent with af=0.62-0.73. As our approach invokes no intermediate approximations to general relativity and can strongly reject binaries whose radiation is inconsistent with the data, our analysis provides a valuable complement to Abbott et al. [Phys. Rev. Lett. 116, 241102 (2016)].LIGO California Institute of TechnologyLouisiana State UniversityAmerican UniversityUniversità di SalernoINFN Sezione di Napoli Complesso Universitario di Monte S.AngeloUniversity of FloridaLIGO Livingston ObservatoryLaboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP) Université Savoie Mont Blanc CNRS/IN2P3University of Sannio at BeneventoAlbert-Einstein-Institut Max-Planck-Institut für GravitationsphysikNikhef Science ParkLIGO Massachusetts Institute of TechnologyInstituto Nacional de Pesquisas EspaciaisINFN Gran Sasso Science InstituteINFN Sezione di Roma Tor VergataInter-University Centre for Astronomy and AstrophysicsInternational Centre for Theoretical Sciences Tata Institute of Fundamental ResearchUniversity of Wisconsin-MilwaukeeLeibniz Universität HannoverUniversità di PisaINFN Sezione di PisaAustralian National UniversityUniversity of MississippiCalifornia State University FullertonLAL Univ. 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UniversityPennsylvania State UniversityNational Tsing Hua UniversityCharles Sturt UniversityWest Virginia UniversityUniversity of ChicagoCaltech CaRTKorea Institute of Science and Technology InformationUniversità di Roma la SapienzaUniversity of BrusselsSonoma State UniversityNorthwestern UniversityUniversity of MinnesotaUniversity of MelbourneInstitute for Plasma ResearchUniversity of SheffieldUniversity of Texas Rio Grande ValleyDipartimento di FisicaTrento Institute for Fundamental Physics and ApplicationsMontclair State UniversityCardiff UniversityLendulet Astrophysics Research GroupNational Astronomical Observatory of JapanUniversity of EdinburghIndian Institute of TechnologyUniversity of SzegedEmbry-Riddle Aeronautical UniversityOsservatorio Astronomico di CapodimonteUniversity of MichiganRochester Institute of TechnologyUniversity of Illinois at Urbana-ChampaignUniversity of Biał YstokUniversity of StrathclydeIEECCET CampusUniversity of TorontoInstitute of Applied PhysicsPusan National UniversityHanyang UniversityUniversity of AdelaideNCBJIM-PANMonash UniversitySeoul National UniversityChinese University of Hong KongUniversity of Alabama in HuntsvilleUniversity of Massachusetts-AmherstCNRSA and M CollegeCollege of William and MaryUniversidade Estadual Paulista (UNESP)University of CambridgeIISER-KolkataHSICWhitman CollegeNational Institute for Mathematical SciencesUniversité de LyonHobart and William Smith CollegesUniversity of Zielona GóraUniversity of LondonAndrews UniversityUniversità di SienaTrinity UniversityUniversity of WashingtonKenyon CollegeAbilene Christian UniversityCornell UniversitySezione di NapoliAbbott, 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.Anderson, S. B.Anderson, W. G.Arai, K.Araya, M. C.Arceneaux, C. C.Areeda, J. S.Arnaud, N.Arun, K. G.Ascenzi, S.Ashton, G.Ast, M.Aston, S. M.Astone, P.Aufmuth, P.Aulbert, C.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.Bejger, 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.Birch, J.Birney, R.Biscans, S.Bisht, A.Bitossi, M.Biwer, C.Bizouard, M. A.Blackburn, J. K.Blair, C. D.Blair, D. G.Blair, R. M.Bloemen, S.Bock, O.Boer, M.Bogaert, G.Bogan, C.Bohe, A.Bond, C.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.Calderón Bustillo, J.Callister, T.Calloni, E.Camp, J. B.Cannon, K. C.Cao, J.Capano, C. D.Capocasa, E.Carbognani, F.Caride, S.Casanueva Diaz, J.Casentini, C.Caudill, S.Cavaglià, M.Cavalier, F.Cavalieri, R.Cella, G.Cepeda, C. B.Cerboni Baiardi, L.Cerretani, G.Cesarini, E.Chamberlin, S. J.Chan, M.Chao, S.Charlton, P.Chassande-Mottin, E.Cheeseboro, B. D.Chen, H. Y.Chen, Y.Cheng, C.Chincarini, A.Chiummo, A.Cho, H. S.Cho, M.Chow, J. H.Christensen, N.Chu, Q.Chua, S.Chung, S.Ciani, G.Clara, F.Clark, J. A.Cleva, F.Coccia, E.Cohadon, P. F.Colla, A.Collette, C. G.Cominsky, L.Constancio, M.Conte, A.Conti, L.Cook, D.Corbitt, T. R.Cornish, N.Corsi, A.Cortese, S.Costa, C. A.Coughlin, M. W.Coughlin, S. B.Coulon, J. P.Countryman, S. T.Couvares, P.Cowan, E. E.Coward, D. M.Cowart, M. J.Coyne, D. C.Coyne, R.Craig, K.Creighton, J. D.E.Cripe, J.Crowder, S. G.Cumming, A.Cunningham, L.Cuoco, E.Dal Canton, T.Danilishin, S. L.D'Antonio, S.Danzmann, K.Darman, N. S.Dasgupta, A.Da Silva Costa, C. F.Dattilo, V.Dave, I.Davier, M.Davies, G. S.Daw, E. J.Day, R.De, S.Debra, D.Debreczeni, G.Degallaix, J.De Laurentis, M.Deléglise, S.Del Pozzo, W.Denker, T.Dent, T.Dergachev, V.De Rosa, R.Derosa, R. T.Desalvo, R.Devine, R. C.Dhurandhar, S.Díaz, M. C.Di Fiore, L.Di Giovanni, M.Di Girolamo, T.Di Lieto, A.Di Pace, S.Di Palma, I.Di Virgilio, A.Dolique, V.Donovan, F.Dooley, K. L.Doravari, S.Douglas, R.Downes, T. P.Drago, M.Drever, R. W.P.Driggers, J. C.Ducrot, M.Dwyer, S. E.Edo, T. B.Edwards, M. C.Effler, A.Eggenstein, H. B.Ehrens, P.Eichholz, J.Eikenberry, S. S.Engels, W.Essick, R. C.Etzel, T.Evans, M.Evans, T. M.Everett, R.Factourovich, M.Fafone, V.Fair, H.Fan, X.Fang, Q.Farinon, S.Farr, B.Farr, W. M.Favata, M.Fays, M.Fehrmann, H.Fejer, M. M.Fenyvesi, E.Ferrante, I.Ferreira, E. C.Ferrini, F.Fidecaro, F.Fiori, I.Fiorucci, D.Fisher, R. P.Flaminio, R.Fletcher, M.Fournier, J. D.Frasca, S.Frasconi, F.Frei, Z.Freise, A.Frey, R.Frey, V.Fritschel, P.Frolov, V. V.Fulda, P.Fyffe, M.Gabbard, H. A.G.Gair, J. R.Gammaitoni, L.Gaonkar, S. G.Garufi, F.Gaur, G.Gehrels, N.Gemme, G.Geng, P.Genin, E.Gennai, A.George, J.Gergely, L.Germain, V.Ghosh, AbhirupGhosh, ArchismanGhosh, S.Giaime, J. A.Giardina, K. D.Giazotto, A.Gill, K.Glaefke, A.Goetz, E.Goetz, R.Gondan, L.González, G.Gonzalez Castro, J. M.Gopakumar, A.Gordon, N. A.Gorodetsky, M. L.Gossan, S. E.Gosselin, M.Gouaty, R.Grado, A.Graef, C.Graff, P. B.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.Hanson, J.Hardwick, T.Harms, J.Harry, G. M.Harry, I. W.Hart, M. J.Hartman, M. T.Haster, C. J.Haughian, K.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.Huang, S.Huerta, E. A.Huet, D.Hughey, B.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.Jang, H.Jani, K.Jaranowski, P.Jawahar, S.Jian, L.Jiménez-Forteza, F.Johnson, W. W.Jones, D. I.Jones, R.Jonker, R. J.G.Ju, L.Haris, K.Kalaghatgi, C. V.Kalogera, V.Kandhasamy, S.Kang, G.Kanner, J. B.Kapadia, S. J.Karki, S.Karvinen, K. S.Kasprzack, M.Katsavounidis, E.Katzman, W.Kaufer, S.Kaur, T.Kawabe, K.Kéfélian, F.Kehl, M. S.Keitel, D.Kelley, D. B.Kells, W.Kennedy, R.Key, J. S.Khalili, F. Y.Khan, I.Khan, Z.Khazanov, E. A.Kijbunchoo, N.Kim, Chi-WoongKim, ChungleeKim, J.Kim, K.Kim, N.Kim, W.Kim, Y. M.Kimbrell, S. J.King, E. J.King, P. J.Kissel, J. S.Klein, B.Kleybolte, L.Klimenko, S.Koehlenbeck, S. M.Koley, S.Kondrashov, V.Kontos, A.Korobko, M.Korth, W. Z.Kowalska, I.Kozak, D. B.Kringel, V.Królak, A.Krueger, C.Kuehn, G.Kumar, P.Kumar, R.Kuo, L.Kutynia, A.Lackey, B. D.Landry, M.Lange, J.Lantz, B.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.Lenon, A.Leonardi, M.Leong, J. R.Leroy, N.Letendre, N.Levin, Y.Lewis, J. B.Li, T. G.F.Libson, A.Littenberg, T. B.Lockerbie, N. A.Lombardi, A. L.Lord, J. E.Lorenzini, M.Loriette, V.Lormand, M.Losurdo, G.Lough, J. D.Lück, H.Lundgren, A. P.Lynch, R.Ma, Y.Machenschalk, B.Macinnis, M.Macleod, D. M.Magaña-Sandoval, F.Zertuche, L. MagañaMagee, R. M.Majorana, E.Maksimovic, I.Malvezzi, V.Man, N.Mandic, V.Mangano, V.Mansell, G. L.Manske, M.Mantovani, M.Marchesoni, F.Marion, F.Márka, S.Márka, Z.Markosyan, A. S.Maros, E.Martelli, F.Martellini, L.Martin, I. W.Martynov, D. V.Marx, J. N.Mason, K.Masserot, A.Massinger, T. J.Masso-Reid, M.Mastrogiovanni, S.Matichard, F.Matone, L.Mavalvala, N.Mazumder, N.McCarthy, R.McClelland, D. E.McCormick, S.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.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. [UNESP]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.Mossavi, K.Mours, B.Mow-Lowry, C. M.Mueller, G.Muir, A. W.Mukherjee, ArunavaMukherjee, D.Mukherjee, S.Mukund, N.Mullavey, A.Munch, J.Murphy, D. J.Murray, P. G.Mytidis, A.Nardecchia, I.Naticchioni, L.Nayak, R. K.Nedkova, K.Nelemans, G.Nelson, T. J.N.Neri, M.Neunzert, A.Newton, G.Nguyen, T. T.Nielsen, A. B.Nissanke, S.Nitz, A.Nocera, F.Nolting, D.Normandin, M. E.N.Nuttall, L. K.Oberling, J.Ochsner, E.O'Dell, J.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.Pai, A.Pai, S. A.Palamos, J. R.Palashov, O.Palomba, C.Pal-Singh, A.Pan, H.Pankow, C.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.Patrick, Z.Pearlstone, B. L.Pedraza, M.Pedurand, R.Pekowsky, L.Pele, A.Penn, S.Perreca, A.Perri, L. M.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.Predoi, V.Prestegard, T.Price, L. R.Prijatelj, M.Principe, M.Privitera, S.Prodi, G. A.Prokhorov, L.Puncken, O.Punturo, M.Puppo, P.Pürrer, 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.Reed, C. M.Regimbau, T.Rei, L.Reid, S.Reitze, D. H.Rew, H.Reyes, S. D.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.Romanov, G.Romie, J. H.Rosińska, D.Rowan, S.Rüdiger, A.Ruggi, P.Ryan, K.Sachdev, S.Sadecki, T.Sadeghian, L.Sakellariadou, M.Salconi, L.Saleem, M.Salemi, F.Samajdar, A.Sammut, L.Sanchez, E. J.Sandberg, V.Sandeen, B.Sanders, J. R.Sassolas, B.Saulson, P. R.Sauter, O. E.S.Savage, R. L.Sawadsky, A.Schale, P.Schilling, R.Schmidt, J.Schmidt, P.Schnabel, R.Schofield, R. M.S.Schönbeck, A.Schreiber, E.Schuette, D.Schutz, B. F.Scott, J.Scott, S. M.Sellers, D.Sengupta, A. S.Sentenac, D.Sequino, V.Sergeev, A.Setyawati, Y.Shaddock, D. A.Shaffer, T.Shahriar, M. S.Shaltev, M.Shapiro, B.Shawhan, P.Sheperd, A.Shoemaker, D. H.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, J. R.Smith, N. D.Smith, R. J.E.Son, E. J.Sorazu, B.Sorrentino, F.Souradeep, T.Srivastava, A. K.Staley, A.Steinke, M.Steinlechner, J.Steinlechner, S.Steinmeyer, D.Stephens, B. C.Stone, R.Strain, K. A.Straniero, N.Stratta, G.Strauss, N. A.Strigin, S.Sturani, R. [UNESP]Stuver, A. L.Summerscales, T. Z.Sun, L.Sunil, S.Sutton, P. J.Swinkels, B. L.Szczepańczyk, M. J.Tacca, M.Talukder, D.Tanner, D. B.Tápai, M.Tarabrin, S. P.Taracchini, A.Taylor, R.Theeg, T.Thirugnanasambandam, M. P.Thomas, E. G.Thomas, M.Thomas, P.Thorne, K. A.Thorne, K. S.Thrane, E.Tiwari, S.Tiwari, V.Tokmakov, K. V.Toland, K.Tomlinson, C.Tonelli, M.Tornasi, Z.Torres, C. V.Torrie, C. I.Töyrä, D.Travasso, F.Traylor, G.Trifirò, D.Tringali, M. C.Trozzo, L.Tse, M.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.Van Den Brand, J. F.J.Van Den Broeck, C.Vander-Hyde, D. C.Van Der Schaaf, L.Van Heijningen, J. V.Van Veggel, A. A.Vardaro, M.Vass, S.Vasúth, M.Vaulin, R.Vecchio, A.Vedovato, G.Veitch, J.Veitch, P. J.Venkateswara, K.Verkindt, D.Vetrano, F.Viceré, A.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, X.Wang, Y.Ward, R. L.Warner, J.Was, M.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.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.Yablon, J.Yam, W.Yamamoto, H.Yancey, C. C.Yu, H.Yvert, M.Zadrożny, A.Zangrando, L.Zanolin, M.Zendri, J. P.Zevin, M.Zhang, L.Zhang, M.Zhang, Y.Zhao, C.Zhou, M.Zhou, Z.Zhu, X. J.Zucker, M. E.Zuraw, S. E.Zweizig, J.Boyle, M.Campanelli, M.Chu, T.Clark, M.Fauchon-Jones, E.Fong, H.Healy, J.Hemberger, D.Hinder, I.Husa, S.Kalaghati, C.Khan, S.Kidder, L. E.Kinsey, M.Laguna, P.London, L. T.Lousto, C. O.Lovelace, G.Ossokine, S.Pannarale, F.Pfeiffer, H. P.Scheel, M.Shoemaker, D. M.Szilagyi, B.Teukolsky, S.Vinuales, A. VanoZlochower, Y.2022-04-29T07:52:03Z2022-04-29T07:52:03Z2016-09-14info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.94.064035Physical Review D, v. 94, n. 6, 2016.2470-00292470-0010http://hdl.handle.net/11449/22823010.1103/PhysRevD.94.0640352-s2.0-84990985966Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2022-04-29T07:53:43Zoai:repositorio.unesp.br:11449/228230Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T18:19:31.837610Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
title Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
spellingShingle Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
Abbott, B. P.
title_short Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
title_full Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
title_fullStr Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
title_full_unstemmed Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
title_sort Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
author Abbott, B. P.
author_facet Abbott, B. P.
Abbott, R.
Abbott, T. D.
Abernathy, M. R.
Acernese, F.
Ackley, K.
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Kim, Chunglee
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Mishra, C.
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Neri, M.
Neunzert, A.
Newton, G.
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Smith, R. J.E.
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Steinlechner, S.
Steinmeyer, D.
Stephens, B. C.
Stone, R.
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Stratta, G.
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Stuver, A. L.
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Williamson, A. R.
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Willke, B.
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Wu, G.
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Yam, W.
Yamamoto, H.
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Yu, H.
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Zanolin, M.
Zendri, J. P.
Zevin, M.
Zhang, L.
Zhang, M.
Zhang, Y.
Zhao, C.
Zhou, M.
Zhou, Z.
Zhu, X. J.
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Zuraw, S. E.
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Boyle, M.
Campanelli, M.
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Clark, M.
Fauchon-Jones, E.
Fong, H.
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Hinder, I.
Husa, S.
Kalaghati, C.
Khan, S.
Kidder, L. E.
Kinsey, M.
Laguna, P.
London, L. T.
Lousto, C. O.
Lovelace, G.
Ossokine, S.
Pannarale, F.
Pfeiffer, H. P.
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Shoemaker, D. M.
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Teukolsky, S.
Vinuales, A. Vano
Zlochower, Y.
author_role author
author2 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.
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Coyne, D. C.
Coyne, R.
Craig, K.
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Cripe, J.
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Cumming, A.
Cunningham, L.
Cuoco, E.
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Danzmann, K.
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Daw, E. J.
Day, R.
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Fisher, R. P.
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Fletcher, M.
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Frey, R.
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Gair, J. R.
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George, J.
Gergely, L.
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Ghosh, Abhirup
Ghosh, Archisman
Ghosh, S.
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Giazotto, A.
Gill, K.
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Goetz, E.
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González, G.
Gonzalez Castro, J. M.
Gopakumar, A.
Gordon, N. A.
Gorodetsky, M. L.
Gossan, S. E.
Gosselin, M.
Gouaty, R.
Grado, A.
Graef, C.
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Granata, M.
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Gras, S.
Gray, C.
Greco, G.
Green, A. C.
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Guo, X.
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Gustafson, R.
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Hall, B. R.
Hall, E. D.
Hammond, G.
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Harms, J.
Harry, G. M.
Harry, I. W.
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Heintze, M. C.
Heitmann, H.
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Heptonstall, A. W.
Heurs, M.
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Holz, D. E.
Hopkins, P.
Hough, J.
Houston, E. A.
Howell, E. J.
Hu, Y. M.
Huang, S.
Huerta, E. A.
Huet, D.
Hughey, B.
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.
Jang, H.
Jani, K.
Jaranowski, P.
Jawahar, S.
Jian, L.
Jiménez-Forteza, F.
Johnson, W. W.
Jones, D. I.
Jones, R.
Jonker, R. J.G.
Ju, L.
Haris, K.
Kalaghatgi, C. V.
Kalogera, V.
Kandhasamy, S.
Kang, G.
Kanner, J. B.
Kapadia, S. J.
Karki, S.
Karvinen, K. S.
Kasprzack, M.
Katsavounidis, E.
Katzman, W.
Kaufer, S.
Kaur, T.
Kawabe, K.
Kéfélian, F.
Kehl, M. S.
Keitel, D.
Kelley, D. B.
Kells, W.
Kennedy, R.
Key, J. S.
Khalili, F. Y.
Khan, I.
Khan, Z.
Khazanov, E. A.
Kijbunchoo, N.
Kim, Chi-Woong
Kim, Chunglee
Kim, J.
Kim, K.
Kim, N.
Kim, W.
Kim, Y. M.
Kimbrell, S. J.
King, E. J.
King, P. J.
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Klein, B.
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Koehlenbeck, S. M.
Koley, S.
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Kontos, A.
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Kozak, D. B.
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Kumar, R.
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Kutynia, A.
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Lee, H. M.
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Maros, E.
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Martin, I. W.
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Meidam, J.
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Mikhailov, E. E.
Milano, L.
Miller, A. L.
Miller, A.
Miller, B. B.
Miller, J.
Millhouse, M.
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Ming, J.
Mirshekari, S. [UNESP]
Mishra, C.
Mitra, S.
Mitrofanov, V. P.
Mitselmakher, G.
Mittleman, R.
Moggi, A.
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Mohapatra, S. R.P.
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Moore, C. J.
Moraru, D.
Moreno, G.
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Mossavi, K.
Mours, B.
Mow-Lowry, C. M.
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Mukherjee, Arunava
Mukherjee, D.
Mukherjee, S.
Mukund, N.
Mullavey, A.
Munch, J.
Murphy, D. J.
Murray, P. G.
Mytidis, A.
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Naticchioni, L.
Nayak, R. K.
Nedkova, K.
Nelemans, G.
Nelson, T. J.N.
Neri, M.
Neunzert, A.
Newton, G.
Nguyen, T. T.
Nielsen, A. B.
Nissanke, S.
Nitz, A.
Nocera, F.
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Normandin, M. E.N.
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Oelker, E.
Ogin, G. H.
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Oppermann, P.
Oram, Richard J.
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O'Shaughnessy, R.
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Palashov, O.
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Pankow, C.
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Papa, M. A.
Paris, H. R.
Parker, W.
Pascucci, D.
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Passuello, D.
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Pedurand, R.
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Pitkin, M.
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Poggiani, R.
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Rakhmanov, M.
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Robie, R.
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Roma, V. J.
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Romano, R.
Romanov, G.
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Rüdiger, A.
Ruggi, P.
Ryan, K.
Sachdev, S.
Sadecki, T.
Sadeghian, L.
Sakellariadou, M.
Salconi, L.
Saleem, M.
Salemi, F.
Samajdar, A.
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Sanders, J. R.
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Sengupta, A. S.
Sentenac, D.
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Setyawati, Y.
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Shaffer, T.
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Shaltev, M.
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Silva, A. D.
Singer, A.
Singer, L. P.
Singh, A.
Singh, R.
Singhal, A.
Sintes, A. M.
Slagmolen, B. J.J.
Smith, J. R.
Smith, N. D.
Smith, R. J.E.
Son, E. J.
Sorazu, B.
Sorrentino, F.
Souradeep, T.
Srivastava, A. K.
Staley, A.
Steinke, M.
Steinlechner, J.
Steinlechner, S.
Steinmeyer, D.
Stephens, B. C.
Stone, R.
Strain, K. A.
Straniero, N.
Stratta, G.
Strauss, N. A.
Strigin, S.
Sturani, R. [UNESP]
Stuver, A. L.
Summerscales, T. Z.
Sun, L.
Sunil, S.
Sutton, P. J.
Swinkels, B. L.
Szczepańczyk, M. J.
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Taylor, R.
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Thomas, M.
Thomas, P.
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Vedovato, G.
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Veitch, P. J.
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Vyatchanin, S. P.
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Wade, L. E.
Wade, M.
Walker, M.
Wallace, L.
Walsh, S.
Wang, G.
Wang, H.
Wang, M.
Wang, X.
Wang, Y.
Ward, R. L.
Warner, J.
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Weinert, M.
Weinstein, A. J.
Weiss, R.
Wen, L.
Weßels, P.
Westphal, T.
Wette, K.
Whelan, J. T.
Whiting, B. F.
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.
Yablon, J.
Yam, W.
Yamamoto, H.
Yancey, C. C.
Yu, H.
Yvert, M.
Zadrożny, A.
Zangrando, L.
Zanolin, M.
Zendri, J. P.
Zevin, M.
Zhang, L.
Zhang, M.
Zhang, Y.
Zhao, C.
Zhou, M.
Zhou, Z.
Zhu, X. J.
Zucker, M. E.
Zuraw, S. E.
Zweizig, J.
Boyle, M.
Campanelli, M.
Chu, T.
Clark, M.
Fauchon-Jones, E.
Fong, H.
Healy, J.
Hemberger, D.
Hinder, I.
Husa, S.
Kalaghati, C.
Khan, S.
Kidder, L. E.
Kinsey, M.
Laguna, P.
London, L. T.
Lousto, C. O.
Lovelace, G.
Ossokine, S.
Pannarale, F.
Pfeiffer, H. P.
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Shoemaker, D. M.
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Teukolsky, S.
Vinuales, A. Vano
Zlochower, Y.
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dc.contributor.none.fl_str_mv California Institute of Technology
Louisiana State University
American University
Università di Salerno
Complesso Universitario di Monte S.Angelo
University of Florida
LIGO Livingston Observatory
CNRS/IN2P3
University of Sannio at Benevento
Max-Planck-Institut für Gravitationsphysik
Science Park
Massachusetts Institute of Technology
Instituto Nacional de Pesquisas Espaciais
Gran Sasso Science Institute
Sezione di Roma Tor Vergata
Inter-University Centre for Astronomy and Astrophysics
Tata Institute of Fundamental Research
University of Wisconsin-Milwaukee
Leibniz Universität Hannover
Università di Pisa
Sezione di Pisa
Australian National University
University of Mississippi
California State University Fullerton
Université Paris-Saclay
Chennai Mathematical Institute
Università di Roma Tor Vergata
University of Southampton
Universität Hamburg
Sezione di Roma
Max-Planck-Institut für Gravitations\-physik
Sorbonne Paris Cité
Montana State University
Università di Perugia
Sezione di Perugia
European Gravitational Observatory (EGO)
Syracuse University
University of Glasgow
LIGO Hanford Observatory
RMKI
Columbia University
Stanford University
Dipartimento di Fisica e Astronomia
Sezione di Padova
CAMK-PAN
University of Birmingham
Università degli Studi di Genova
Sezione di Genova
RRCAT
Lomonosov Moscow State University
University of the West of Scotland
University of Western Australia
Radboud University Nijmegen
Observatoire Côte d'Azur
Université de Rennes 1
Washington State University
Università degli Studi di Urbino Carlo Bo
Sezione di Firenze
University of Oregon
Collège de France
Carleton College
Astronomical Observatory Warsaw University
VU University Amsterdam
University of Maryland
Georgia Institute of Technology
Université Claude Bernard Lyon 1
Goddard Space Flight Center
University of Tokyo
Tsinghua University
Texas Tech University
Pennsylvania State University
National Tsing Hua University
Charles Sturt University
West Virginia University
University of Chicago
Caltech CaRT
Korea Institute of Science and Technology Information
Università di Roma la Sapienza
University of Brussels
Sonoma State University
Northwestern University
University of Minnesota
University of Melbourne
Institute for Plasma Research
University of Sheffield
University of Texas Rio Grande Valley
Dipartimento di Fisica
Trento Institute for Fundamental Physics and Applications
Montclair State University
Cardiff University
Lendulet Astrophysics Research Group
National Astronomical Observatory of Japan
University of Edinburgh
Indian Institute of Technology
University of Szeged
Embry-Riddle Aeronautical University
Osservatorio Astronomico di Capodimonte
University of Michigan
Rochester Institute of Technology
University of Illinois at Urbana-Champaign
University of Biał Ystok
University of Strathclyde
IEEC
CET Campus
University of Toronto
Institute of Applied Physics
Pusan National University
Hanyang University
University of Adelaide
NCBJ
IM-PAN
Monash University
Seoul National University
Chinese University of Hong Kong
University of Alabama in Huntsville
University of Massachusetts-Amherst
CNRS
A and M College
College of William and Mary
Universidade Estadual Paulista (UNESP)
University of Cambridge
IISER-Kolkata
HSIC
Whitman College
National Institute for Mathematical Sciences
Université de Lyon
Hobart and William Smith Colleges
University of Zielona Góra
University of London
Andrews University
Università di Siena
Trinity University
University of Washington
Kenyon College
Abilene Christian University
Cornell University
Sezione di Napoli
dc.contributor.author.fl_str_mv Abbott, 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.
Anderson, S. B.
Anderson, W. G.
Arai, K.
Araya, M. C.
Arceneaux, C. C.
Areeda, J. S.
Arnaud, N.
Arun, K. G.
Ascenzi, S.
Ashton, G.
Ast, M.
Aston, S. M.
Astone, P.
Aufmuth, P.
Aulbert, C.
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.
Bejger, 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.
Birch, J.
Birney, R.
Biscans, S.
Bisht, A.
Bitossi, M.
Biwer, C.
Bizouard, M. A.
Blackburn, J. K.
Blair, C. D.
Blair, D. G.
Blair, R. M.
Bloemen, S.
Bock, O.
Boer, M.
Bogaert, G.
Bogan, C.
Bohe, A.
Bond, C.
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.
Calderón Bustillo, J.
Callister, T.
Calloni, E.
Camp, J. B.
Cannon, K. C.
Cao, J.
Capano, C. D.
Capocasa, E.
Carbognani, F.
Caride, S.
Casanueva Diaz, J.
Casentini, C.
Caudill, S.
Cavaglià, M.
Cavalier, F.
Cavalieri, R.
Cella, G.
Cepeda, C. B.
Cerboni Baiardi, L.
Cerretani, G.
Cesarini, E.
Chamberlin, S. J.
Chan, M.
Chao, S.
Charlton, P.
Chassande-Mottin, E.
Cheeseboro, B. D.
Chen, H. Y.
Chen, Y.
Cheng, C.
Chincarini, A.
Chiummo, A.
Cho, H. S.
Cho, M.
Chow, J. H.
Christensen, N.
Chu, Q.
Chua, S.
Chung, S.
Ciani, G.
Clara, F.
Clark, J. A.
Cleva, F.
Coccia, E.
Cohadon, P. F.
Colla, A.
Collette, C. G.
Cominsky, L.
Constancio, M.
Conte, A.
Conti, L.
Cook, D.
Corbitt, T. R.
Cornish, N.
Corsi, A.
Cortese, S.
Costa, C. A.
Coughlin, M. W.
Coughlin, S. B.
Coulon, J. P.
Countryman, S. T.
Couvares, P.
Cowan, E. E.
Coward, D. M.
Cowart, M. J.
Coyne, D. C.
Coyne, R.
Craig, K.
Creighton, J. D.E.
Cripe, J.
Crowder, S. G.
Cumming, A.
Cunningham, L.
Cuoco, E.
Dal Canton, T.
Danilishin, S. L.
D'Antonio, S.
Danzmann, K.
Darman, N. S.
Dasgupta, A.
Da Silva Costa, C. F.
Dattilo, V.
Dave, I.
Davier, M.
Davies, G. S.
Daw, E. J.
Day, R.
De, S.
Debra, D.
Debreczeni, G.
Degallaix, J.
De Laurentis, M.
Deléglise, S.
Del Pozzo, W.
Denker, T.
Dent, T.
Dergachev, V.
De Rosa, R.
Derosa, R. T.
Desalvo, R.
Devine, R. C.
Dhurandhar, S.
Díaz, M. C.
Di Fiore, L.
Di Giovanni, M.
Di Girolamo, T.
Di Lieto, A.
Di Pace, S.
Di Palma, I.
Di Virgilio, A.
Dolique, V.
Donovan, F.
Dooley, K. L.
Doravari, S.
Douglas, R.
Downes, T. P.
Drago, M.
Drever, R. W.P.
Driggers, J. C.
Ducrot, M.
Dwyer, S. E.
Edo, T. B.
Edwards, M. C.
Effler, A.
Eggenstein, H. B.
Ehrens, P.
Eichholz, J.
Eikenberry, S. S.
Engels, W.
Essick, R. C.
Etzel, T.
Evans, M.
Evans, T. M.
Everett, R.
Factourovich, M.
Fafone, V.
Fair, H.
Fan, X.
Fang, Q.
Farinon, S.
Farr, B.
Farr, W. M.
Favata, M.
Fays, M.
Fehrmann, H.
Fejer, M. M.
Fenyvesi, E.
Ferrante, I.
Ferreira, E. C.
Ferrini, F.
Fidecaro, F.
Fiori, I.
Fiorucci, D.
Fisher, R. P.
Flaminio, R.
Fletcher, M.
Fournier, J. D.
Frasca, S.
Frasconi, F.
Frei, Z.
Freise, A.
Frey, R.
Frey, V.
Fritschel, P.
Frolov, V. V.
Fulda, P.
Fyffe, M.
Gabbard, H. A.G.
Gair, J. R.
Gammaitoni, L.
Gaonkar, S. G.
Garufi, F.
Gaur, G.
Gehrels, N.
Gemme, G.
Geng, P.
Genin, E.
Gennai, A.
George, J.
Gergely, L.
Germain, V.
Ghosh, Abhirup
Ghosh, Archisman
Ghosh, S.
Giaime, J. A.
Giardina, K. D.
Giazotto, A.
Gill, K.
Glaefke, A.
Goetz, E.
Goetz, R.
Gondan, L.
González, G.
Gonzalez Castro, J. M.
Gopakumar, A.
Gordon, N. A.
Gorodetsky, M. L.
Gossan, S. E.
Gosselin, M.
Gouaty, R.
Grado, A.
Graef, C.
Graff, P. B.
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.
Hanson, J.
Hardwick, T.
Harms, J.
Harry, G. M.
Harry, I. W.
Hart, M. J.
Hartman, M. T.
Haster, C. J.
Haughian, K.
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.
Huang, S.
Huerta, E. A.
Huet, D.
Hughey, B.
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.
Jang, H.
Jani, K.
Jaranowski, P.
Jawahar, S.
Jian, L.
Jiménez-Forteza, F.
Johnson, W. W.
Jones, D. I.
Jones, R.
Jonker, R. J.G.
Ju, L.
Haris, K.
Kalaghatgi, C. V.
Kalogera, V.
Kandhasamy, S.
Kang, G.
Kanner, J. B.
Kapadia, S. J.
Karki, S.
Karvinen, K. S.
Kasprzack, M.
Katsavounidis, E.
Katzman, W.
Kaufer, S.
Kaur, T.
Kawabe, K.
Kéfélian, F.
Kehl, M. S.
Keitel, D.
Kelley, D. B.
Kells, W.
Kennedy, R.
Key, J. S.
Khalili, F. Y.
Khan, I.
Khan, Z.
Khazanov, E. A.
Kijbunchoo, N.
Kim, Chi-Woong
Kim, Chunglee
Kim, J.
Kim, K.
Kim, N.
Kim, W.
Kim, Y. M.
Kimbrell, S. J.
King, E. J.
King, P. J.
Kissel, J. S.
Klein, B.
Kleybolte, L.
Klimenko, S.
Koehlenbeck, S. M.
Koley, S.
Kondrashov, V.
Kontos, A.
Korobko, M.
Korth, W. Z.
Kowalska, I.
Kozak, D. B.
Kringel, V.
Królak, A.
Krueger, C.
Kuehn, G.
Kumar, P.
Kumar, R.
Kuo, L.
Kutynia, A.
Lackey, B. D.
Landry, M.
Lange, J.
Lantz, B.
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.
Lenon, A.
Leonardi, M.
Leong, J. R.
Leroy, N.
Letendre, N.
Levin, Y.
Lewis, J. B.
Li, T. G.F.
Libson, A.
Littenberg, T. B.
Lockerbie, N. A.
Lombardi, A. L.
Lord, J. E.
Lorenzini, M.
Loriette, V.
Lormand, M.
Losurdo, G.
Lough, J. D.
Lück, H.
Lundgren, A. P.
Lynch, R.
Ma, Y.
Machenschalk, B.
Macinnis, M.
Macleod, D. M.
Magaña-Sandoval, F.
Zertuche, L. Magaña
Magee, R. M.
Majorana, E.
Maksimovic, I.
Malvezzi, V.
Man, N.
Mandic, V.
Mangano, V.
Mansell, G. L.
Manske, M.
Mantovani, M.
Marchesoni, F.
Marion, F.
Márka, S.
Márka, Z.
Markosyan, A. S.
Maros, E.
Martelli, F.
Martellini, L.
Martin, I. W.
Martynov, D. V.
Marx, J. N.
Mason, K.
Masserot, A.
Massinger, T. J.
Masso-Reid, M.
Mastrogiovanni, S.
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description We compare GW150914 directly to simulations of coalescing binary black holes in full general relativity, including several performed specifically to reproduce this event. Our calculations go beyond existing semianalytic models, because for all simulations - including sources with two independent, precessing spins - we perform comparisons which account for all the spin-weighted quadrupolar modes, and separately which account for all the quadrupolar and octopolar modes. Consistent with the posterior distributions reported by Abbott et al. [Phys. Rev. Lett. 116, 241102 (2016)] (at the 90% credible level), we find the data are compatible with a wide range of nonprecessing and precessing simulations. Follow-up simulations performed using previously estimated binary parameters most resemble the data, even when all quadrupolar and octopolar modes are included. Comparisons including only the quadrupolar modes constrain the total redshifted mass Mz [64 M-82 M], mass ratio 1/q=m2/m1 [0.6,1], and effective aligned spin χeff [-0.3,0.2], where χeff=(S1/m1+S2/m2)·L/M. Including both quadrupolar and octopolar modes, we find the mass ratio is even more tightly constrained. Even accounting for precession, simulations with extreme mass ratios and effective spins are highly inconsistent with the data, at any mass. Several nonprecessing and precessing simulations with similar mass ratio and χeff are consistent with the data. Though correlated, the components' spins (both in magnitude and directions) are not significantly constrained by the data: the data is consistent with simulations with component spin magnitudes a1,2 up to at least 0.8, with random orientations. Further detailed follow-up calculations are needed to determine if the data contain a weak imprint from transverse (precessing) spins. For nonprecessing binaries, interpolating between simulations, we reconstruct a posterior distribution consistent with previous results. The final black hole's redshifted mass is consistent with Mf,z in the range 64.0 M-73.5 M and the final black hole's dimensionless spin parameter is consistent with af=0.62-0.73. As our approach invokes no intermediate approximations to general relativity and can strongly reject binaries whose radiation is inconsistent with the data, our analysis provides a valuable complement to Abbott et al. [Phys. Rev. Lett. 116, 241102 (2016)].
publishDate 2016
dc.date.none.fl_str_mv 2016-09-14
2022-04-29T07:52:03Z
2022-04-29T07:52:03Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1103/PhysRevD.94.064035
Physical Review D, v. 94, n. 6, 2016.
2470-0029
2470-0010
http://hdl.handle.net/11449/228230
10.1103/PhysRevD.94.064035
2-s2.0-84990985966
url http://dx.doi.org/10.1103/PhysRevD.94.064035
http://hdl.handle.net/11449/228230
identifier_str_mv Physical Review D, v. 94, n. 6, 2016.
2470-0029
2470-0010
10.1103/PhysRevD.94.064035
2-s2.0-84990985966
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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