UPPER LIMITS ON THE RATES OF BINARY NEUTRON STAR AND NEUTRON STAR-BLACK HOLE MERGERS FROM ADVANCED LIGO'S FIRST OBSERVING RUN

Detalhes bibliográficos
Autor(a) principal: Abbott, B. P.
Data de Publicação: 2016
Outros Autores: Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, E., 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, E., 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., Calderon 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., Cavaglia, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. 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Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.3847/2041-8205/832/2/L21
http://hdl.handle.net/11449/162219
Resumo: We report here the non-detection of gravitational waves from the merger of binary-neutron star systems and neutron star-black hole systems during the first observing run of the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO). In particular, we searched for gravitational-wave signals from binary-neutron star systems with component masses is an element of[1, 3] M-circle dot and component dimensionless spins <0.05. We also searched for neutron star-black hole systems with the same neutron star parameters, black hole mass is an element of[2, 99] M-circle dot, and no restriction on the black hole spin magnitude. We assess the sensitivity of the two LIGO detectors to these systems and find that they could have detected the merger of binary-neutron star systems with component mass distributions of 1.35 +/- 0.13 M-circle dot at a volume-weighted average distance of similar to 70 Mpc, and for neutron star-black hole systems with neutron star masses of 1.4 M-circle dot and black hole masses of at least 5 M-circle dot, a volume-weighted average distance of at least similar to 110 Mpc. From this we constrain with 90% confidence the merger rate to be less than 12,600 Gpc(-3) yr(-1) for binary-neutron star systems and less than 3600 Gpc(-3) yr(-1) for neutron star-black hole systems. We discuss the astrophysical implications of these results, which we find to be in conflict with only the most optimistic predictions. However, we find that if no detection of neutron star-binary mergers is made in the next two Advanced LIGO and Advanced Virgo observing runs we would place significant constraints on the merger rates. Finally, assuming a rate of 10(-7)(+20) Gpc(-3) yr(-1), short gamma-ray bursts beamed toward the Earth, and assuming that all short gamma-ray bursts have binary-neutron star (neutron star-black hole) progenitors, we can use our 90% confidence rate upper limits to constrain the beaming angle of the gamma-ray burst to be greater than. 2.degrees 3(-1.1)(+1.7)(4.degrees 3(-1.9)(+3.1)).
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spelling UPPER LIMITS ON THE RATES OF BINARY NEUTRON STAR AND NEUTRON STAR-BLACK HOLE MERGERS FROM ADVANCED LIGO'S FIRST OBSERVING RUNbinaries: generalgamma-ray burst: generalgravitational wavesstars: black holesstars: neutronWe report here the non-detection of gravitational waves from the merger of binary-neutron star systems and neutron star-black hole systems during the first observing run of the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO). In particular, we searched for gravitational-wave signals from binary-neutron star systems with component masses is an element of[1, 3] M-circle dot and component dimensionless spins <0.05. We also searched for neutron star-black hole systems with the same neutron star parameters, black hole mass is an element of[2, 99] M-circle dot, and no restriction on the black hole spin magnitude. We assess the sensitivity of the two LIGO detectors to these systems and find that they could have detected the merger of binary-neutron star systems with component mass distributions of 1.35 +/- 0.13 M-circle dot at a volume-weighted average distance of similar to 70 Mpc, and for neutron star-black hole systems with neutron star masses of 1.4 M-circle dot and black hole masses of at least 5 M-circle dot, a volume-weighted average distance of at least similar to 110 Mpc. From this we constrain with 90% confidence the merger rate to be less than 12,600 Gpc(-3) yr(-1) for binary-neutron star systems and less than 3600 Gpc(-3) yr(-1) for neutron star-black hole systems. We discuss the astrophysical implications of these results, which we find to be in conflict with only the most optimistic predictions. However, we find that if no detection of neutron star-binary mergers is made in the next two Advanced LIGO and Advanced Virgo observing runs we would place significant constraints on the merger rates. Finally, assuming a rate of 10(-7)(+20) Gpc(-3) yr(-1), short gamma-ray bursts beamed toward the Earth, and assuming that all short gamma-ray bursts have binary-neutron star (neutron star-black hole) progenitors, we can use our 90% confidence rate upper limits to constrain the beaming angle of the gamma-ray burst to be greater than. 2.degrees 3(-1.1)(+1.7)(4.degrees 3(-1.9)(+3.1)).United States National Science Foundation (NSF)Science and Technology Facilities Council (STFC) of the United KingdomMax-Planck-Society (MPS)State of Niedersachsen/GermanyAustralian Research CouncilNetherlands Organisation for Scientific ResearchCouncil of Scientific and Industrial Research of IndiaDepartment of Science and Technology, IndiaScience & Engineering Research Board (SERB), IndiaMinistry of Human Resource Development, IndiaSpanish Ministerio de Economia y CompetitividadConselleria d'Economia i Competitivitat and Conselleria d'Educacio Cultura i Universitats of the Govern de les Illes BalearsNational Science Centre of PolandEuropean CommissionRoyal SocietyScottish Funding CouncilScottish Universities Physics AllianceHungarian Scientific Research Fund (OTKA)Lyon Institute of Origins (LIO)National Research Foundation of Korea, Industry CanadaProvince of Ontario through the Ministry of Economic Development and InnovationNatural Science and Engineering Research Council CanadaCanadian Institute for Advanced ResearchBrazilian Ministry of Science, Technology, and InnovationFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Russian Foundation for Basic ResearchLeverhulme TrustResearch CorporationMinistry of Science and Technology (MOST), TaiwanKavli FoundationNSFSTFCMPSINFNCNRSScience and Technology Facilities CouncilLIGO, Calif Inst Technol, Pasadena, CA 91125 USALouisiana State Univ, Baton Rouge, LA 70803 USAAmer Univ, Washington, DC 20016 USAUniv Salerno, I-84084 Salerno, ItalyComplesso Univ Monte S Angelo, INFN, Sez Napoli, I-80126 Naples, ItalyUniv Florida, Gainesville, FL 32611 USALIGO Livingston Observ, Livingston, LA 70754 USALab Annecy Le Vieux Phys Particules, Univ Savoic Mt Blanc, CNRS IN2P3, F-74941 Annecy Le Vieux, FranceUniv Sannio Benevento, I-82100 Benevento, ItalyINFN, Sez Napoli, I-80100 Naples, ItalyMax Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, GermanyNikhef, Sci Pk, NL-1098 XG Amsterdam, NetherlandsMIT, LIGO, Cambridge, MA 02139 USAInst Nacl Pesquisas Espaciais, BR-12227010 Sao Jose Dos Campos, SP, BrazilINFN, Gran Sasso Sci Inst, I-67100 Laquila, ItalyINFN, Sezione Roma Tor Vergata, I-00133 Rome, ItalyInter Univ Ctr Astron & Astrophys, Pune 411007, Maharashtra, IndiaInt Ctr Theoret Sci, Tata Inst Fundamental Res, Bangalore 560012, Karnataka, IndiaUniv Wisconsin Milwaukee, Milwaukee, WI 53201 USALeibniz Univ Hannover, D-30167 Hannover, GermanyUniv Pisa, I-56127 Pisa, ItalyINFN, Sez Pisa, I-56127 Pisa, ItalyAustralian Natl Univ, Canberra, ACT 0200, AustraliaUniv Mississippi, University, MS 38677 USACalif State Univ Fullerton, Fullerton, CA 92831 USAUniv Paris 11, Univ Paris Saclay, CNRS IN2P3, LAL, Orsay, FranceChennai Math Inst, Madras 603103, Tamil Nadu, IndiaUniv Roma Tor Vergata, I-00133 Rome, ItalyUniv Southampton, Southampton SO17 1BJ, Hants, EnglandUniv Hamburg, D-22761 Hamburg, GermanyINFN, Sez Roma, I-00185 Rome, ItalyMax Planck Inst Gravitat Phys, Alber Einstein Inst, D-14476 Potsdam, GermanyUniv Paris Diderot, Sorbonne Paris Cite, CNRS IN2P3, Observatoire Paris,CEA Irfu,APC, F-75205 Paris 13, FranceMontana State Univ, Bozeman, MT 59717 USAUniv Perugia, I-06123 Perugia, ItalyINFN, Sez Perugia, I-06123 Perugia, ItalyEGO, I-56021 Pisa, ItalySyracuse Univ, Syracuse, NY 13244 USAUniv Glasgow, SUPA, Glasgow G12 8QQ, Lanark, ScotlandLIGO Hanford Observ, Richland, WA 99352 USAWigner RCP, RMKI, Konkoly Thege Miklos 29-33, H-1121 Budapest, HungaryColumbia Univ, New York, NY 10027 USAStanford Univ, Stanford, CA 94305 USAUniv Padua, Dipartimento Fis & Astron, I-35131 Padua, 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Bristol: Iop Publishing Ltd, v. 832, n. 2, 15 p., 2016.2041-8205http://hdl.handle.net/11449/16221910.3847/2041-8205/832/2/L21WOS:000389176100001WOS000389176100001.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengAstrophysical Journal Letters3,186info:eu-repo/semantics/openAccess2023-12-27T06:17:54Zoai:repositorio.unesp.br:11449/162219Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462023-12-27T06:17:54Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv UPPER LIMITS ON THE RATES OF BINARY NEUTRON STAR AND NEUTRON STAR-BLACK HOLE MERGERS FROM ADVANCED LIGO'S FIRST OBSERVING RUN
title UPPER LIMITS ON THE RATES OF BINARY NEUTRON STAR AND NEUTRON STAR-BLACK HOLE MERGERS FROM ADVANCED LIGO'S FIRST OBSERVING RUN
spellingShingle UPPER LIMITS ON THE RATES OF BINARY NEUTRON STAR AND NEUTRON STAR-BLACK HOLE MERGERS FROM ADVANCED LIGO'S FIRST OBSERVING RUN
Abbott, B. P.
binaries: general
gamma-ray burst: general
gravitational waves
stars: black holes
stars: neutron
title_short UPPER LIMITS ON THE RATES OF BINARY NEUTRON STAR AND NEUTRON STAR-BLACK HOLE MERGERS FROM ADVANCED LIGO'S FIRST OBSERVING RUN
title_full UPPER LIMITS ON THE RATES OF BINARY NEUTRON STAR AND NEUTRON STAR-BLACK HOLE MERGERS FROM ADVANCED LIGO'S FIRST OBSERVING RUN
title_fullStr UPPER LIMITS ON THE RATES OF BINARY NEUTRON STAR AND NEUTRON STAR-BLACK HOLE MERGERS FROM ADVANCED LIGO'S FIRST OBSERVING RUN
title_full_unstemmed UPPER LIMITS ON THE RATES OF BINARY NEUTRON STAR AND NEUTRON STAR-BLACK HOLE MERGERS FROM ADVANCED LIGO'S FIRST OBSERVING RUN
title_sort UPPER LIMITS ON THE RATES OF BINARY NEUTRON STAR AND NEUTRON STAR-BLACK HOLE MERGERS FROM ADVANCED LIGO'S FIRST OBSERVING RUN
author Abbott, B. P.
author_facet Abbott, B. P.
Abbott, R.
Abbott, T. D.
Abernathy, M. R.
Acernese, E.
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, E.
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.
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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'Deill, J.
Oelker, E.
Ogin, G. H.
Oh, J. J.
Oh, S. H.
Ohme, F.
Oliver, M.
Oppermann, P.
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Pai, A.
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Palamos, J. R.
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Pierro, V.
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Popolizio, P.
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Qi, H.
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Quitzow-James, R.
Raab, E. 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.
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Reitze, D. H.
Rew, H.
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Ricci, F.
Riles, K.
Rizzo, M.
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Robie, R.
Robinet, F.
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Rolland, L.
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Roma, V. J.
Romano, R.
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Romie, J. H.
Rosinska, D.
Rowan, S.
Rudiger, 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.
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Saulson, P. R.
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Savage, R. L.
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Schale, P.
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Schmidt, J.
Schmidt, P.
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Schofield, R. M. S.
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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.
Shaltevi, M.
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.
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Singh, R.
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Sintes, A. M.
Slagmolen, B. J. J.
Smith, J. R.
Smith, N. D.
Smith, R. J. E.
Son, E. J.
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Sorrentino, F.
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Srivastava, A. K.
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Steinke, M.
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Steinlechner, S.
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Stephens, B. C.
Stone, R.
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Stuver, A. L.
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Sun, L.
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Tapai, M.
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Taracchini, A.
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Thirugnanasambandam, M. P.
Thomas, E. G.
Thomas, M.
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Tiwari, V.
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Toland, K.
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Tuyenbayev, D.
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Unnikrishnan, C. S.
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Usman, S. A.
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Vajente, G.
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van Beuzekom, M.
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Van Den Broeck, C.
Vander-Hyde, D. C.
van der Schaaf, L.
van Heuningen, J. V.
van Veggel, A. A.
Vardaro, M.
Vass, S.
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Vaulin, R.
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Vedovato, G.
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Venkateswara, K.
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Vinet, J. -Y.
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Vo, T.
Vocca, H.
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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.
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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.
Yablong, J.
Yam, W.
Yamamoto, H.
Yancey, C. C.
Yu, H.
Yvert, M.
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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.
LIGO Scientific Collaboration
Virgo Collaboration
author_role author
author2 Abbott, R.
Abbott, T. D.
Abernathy, M. R.
Acernese, E.
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, E.
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.
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Byer, R. L.
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Cadonati, L.
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Calderon Bustillo, J.
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Calloni, E.
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Capocasa, E.
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Caride, S.
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Casentini, C.
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Cella, G.
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Cerboni Baiardi, L.
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Cesarini, E.
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Chan, M.
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Cheeseboro, B. D.
Chen, H. Y.
Cheng, C.
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Chiummo, A.
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Cho, M.
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Colla, A.
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Constancio, M.
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Coughlin, S. B.
Coulon, J. -P
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Couvares, P.
Cowan, E. E.
Coward, D. M.
Cowart, M. J.
Coyne, D. C.
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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.
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Debreczeni, G.
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De laurentis, M.
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Del Pozzo, W.
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Dent, T.
Dergachev, V.
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DeRosa, R. T.
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Devine, R. C.
Dhurandhar, S.
Diaz, M. C.
Di Fiore, L.
Di Giovanni, M.
Di Girolamo, T.
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Di Pace, S.
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Dolique, V.
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Dooley, K. L.
Doravari, S.
Douglas, R.
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Edo, T. B.
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Effler, A.
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Evans, T. M.
Everett, R.
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Fafone, V.
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Fairhurst, S.
Fan, X.
Fang, Q.
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Fiori, I.
Fiorucci, D.
Fisher, R. P.
Flaminio, R.
Fletcher, M.
Fournier, J. -D.
Frasca, S.
Frasconi, F.
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Frey, R.
Frey, V.
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Frolov, V. V.
Fulda, P.
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Gair, J. R.
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Garunfi, E.
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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.
Gonzalez, 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.
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.
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.
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.
Jang, H.
Jani, K.
Jaranowski, P.
Jawahar, S.
Jian, L.
Jimenez-Forteza, E.
Johnson, W. W.
Jones, D. I.
Jones, R.
Jonker, R. J. G.
Ju, L.
Haris
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.
Kefelian, F.
Kehl, M. S.
Keitel, D.
Kelley, D. B.
Kells, W.
Kennedy, R.
Key, J. S.
Khalili, F. Y.
Khan, I.
Khan, S.
Khan, Z.
Khazanov, E. A.
Kusunchoo, 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.
Krishnan, B.
Krolak, 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.
Lazzar, 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.
London, L. T.
Lord, J. E.
Lorenzini, M.
Loriette, V.
Lormand, M.
Losurdo, G.
Lough, J. D.
Luck, H.
Lundgren, A. P.
Lynch, R.
Ma, Y.
Machenschalk, B.
MacInnis, M.
Macleod, D. M.
Magana-Sandoval, F.
Zertuche, L. Magana
Magee, R. M.
Majorana, E.
Maksimovic, I.
Malvezzi, V.
Man, N.
Mandic, V.
Mangano, V.
Mansell, G. L.
Manske, M.
Mantovani, M.
Marchesoni, E.
Marion, F.
Marka, S.
Marka, Z.
Markosyan, A. S.
Maros, E.
Martelli, E.
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.
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Moore, C. J.
Moraru, D.
Moreno, G.
Morriss, S. R.
Mossavi, K.
Mours, B.
Mow-Lowry, C. M.
Mueller, G.
Muir, A. W.
Mukherjee, Arunava
Mukherjee, 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'Deill, 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.
Pannarale, F.
Pant, B. C.
Paoletti, E.
Paoli, A.
Papa, M. A.
Paris, H. R.
Parker, W.
Pascucci, D.
Pasqualetti, A.
Passahieti, 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.
Prix, R.
Prodi, G. A.
Proxhorov, L.
Puncken, O.
Punturo, M.
Puppo, P.
Purrer, M.
Qi, H.
Qin, J.
Qiu, S.
Quetschke, V.
Quintero, E. A.
Quitzow-James, R.
Raab, E. 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, R.
Romanov, G.
Romie, J. H.
Rosinska, D.
Rowan, S.
Rudiger, 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.
Sathyaprakash, B. S.
Saulson, P. R.
Sauter, O. E. S.
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Sawadsky, A.
Schale, P.
Schilling, R.
Schmidt, J.
Schmidt, P.
Schnabel, R.
Schofield, R. M. S.
Schonbecx, A.
Schreiber, E.
Schuette, D.
Schutz, B. F.
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Scott, S. M.
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Sengupta, A. S.
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Sequino, V.
Sergeev, A.
Setyawati, Y.
Shaddock, D. A.
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Shahriar, M. S.
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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, 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]
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Summerscales, T. Z.
Sun, L.
Sunil, S.
Sutton, P. J.
Swinkels, B. L.
Szczepanczyk, M. J.
Tacca, M.
Talukder, D.
Tanner, D. B.
Tapai, M.
Tarabrin, S. P.
Taracchini, A.
Taylor, R.
Theeg, T.
Thirugnanasambandam, M. P.
Thomas, E. G.
Thomas, M.
Thomas, P.
Thorne, K. A.
Thrane, E.
Tiwari, S.
Tiwari, V.
Toxmakov, K. V.
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Tomlinson, C.
Tonelli, M.
Tornasi, Z.
Torres, C. V.
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Toyra, D.
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Traylor, G.
Trifiro, D.
Tringali, M. C.
Trozzo, L.
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Turconi, M.
Tuyenbayev, D.
Ugolini, D.
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Urban, A. L.
Usman, S. A.
Vahlbruch, H.
Vajente, G.
Valdes, G.
van Bakel, N.
van Beuzekom, M.
van den Brand, J. E. J.
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Vander-Hyde, D. C.
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van Heuningen, J. V.
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Vasuth, M.
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Vecchio, A.
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Veitch, P. J.
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Vicere, A.
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Williamson, A. R.
Willis, J. L.
Willke, B.
Wimmer, M. H.
Winkler, W.
Wipf, C. C.
Wittel, H.
Woan, G.
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Worden, J.
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Yam, W.
Yamamoto, H.
Yancey, C. C.
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Yvert, M.
Zadrozny, A.
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Zanolin, M.
Zendri, J. -P.
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Zhang, Y.
Zhao, C.
Zhou, M.
Zhou, Z.
Zhu, X. J.
Zucker, M. E.
Zuraw, S. E.
Zweizig, J.
LIGO Scientific Collaboration
Virgo Collaboration
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dc.contributor.none.fl_str_mv LIGO
Louisiana State Univ
Amer Univ
Univ Salerno
Complesso Univ Monte S Angelo
Univ Florida
LIGO Livingston Observ
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CAMK PAN
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dc.contributor.author.fl_str_mv Abbott, B. P.
Abbott, R.
Abbott, T. D.
Abernathy, M. R.
Acernese, E.
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, E.
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.
Calderon 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.
Cavaglia, M.
Cavalier, F.
Cavalieri, R.
Cella, G.
Cepeda, C. B.
Cerboni Baiardi, L.
Cerretani, G.
Cesarini, E.
Chamberlin, S. J.
Chan, M.
Chao, S.
Chen, Y.
Chassande-Mottin, E.
Cheeseboro, B. D.
Chen, H. 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, E.
Clark, J. A.
Cleva, E.
Coccia, E.
Cohadon, P. -E
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.
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Yu, H.
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Zadrozny, A.
Zangrando, L.
Zanolin, M.
Zendri, J. -P.
Zevin, M.
Zhang, L.
Zhang, M.
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LIGO Scientific Collaboration
Virgo Collaboration
dc.subject.por.fl_str_mv binaries: general
gamma-ray burst: general
gravitational waves
stars: black holes
stars: neutron
topic binaries: general
gamma-ray burst: general
gravitational waves
stars: black holes
stars: neutron
description We report here the non-detection of gravitational waves from the merger of binary-neutron star systems and neutron star-black hole systems during the first observing run of the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO). In particular, we searched for gravitational-wave signals from binary-neutron star systems with component masses is an element of[1, 3] M-circle dot and component dimensionless spins <0.05. We also searched for neutron star-black hole systems with the same neutron star parameters, black hole mass is an element of[2, 99] M-circle dot, and no restriction on the black hole spin magnitude. We assess the sensitivity of the two LIGO detectors to these systems and find that they could have detected the merger of binary-neutron star systems with component mass distributions of 1.35 +/- 0.13 M-circle dot at a volume-weighted average distance of similar to 70 Mpc, and for neutron star-black hole systems with neutron star masses of 1.4 M-circle dot and black hole masses of at least 5 M-circle dot, a volume-weighted average distance of at least similar to 110 Mpc. From this we constrain with 90% confidence the merger rate to be less than 12,600 Gpc(-3) yr(-1) for binary-neutron star systems and less than 3600 Gpc(-3) yr(-1) for neutron star-black hole systems. We discuss the astrophysical implications of these results, which we find to be in conflict with only the most optimistic predictions. However, we find that if no detection of neutron star-binary mergers is made in the next two Advanced LIGO and Advanced Virgo observing runs we would place significant constraints on the merger rates. Finally, assuming a rate of 10(-7)(+20) Gpc(-3) yr(-1), short gamma-ray bursts beamed toward the Earth, and assuming that all short gamma-ray bursts have binary-neutron star (neutron star-black hole) progenitors, we can use our 90% confidence rate upper limits to constrain the beaming angle of the gamma-ray burst to be greater than. 2.degrees 3(-1.1)(+1.7)(4.degrees 3(-1.9)(+3.1)).
publishDate 2016
dc.date.none.fl_str_mv 2016-12-01
2018-11-26T17:12:17Z
2018-11-26T17:12:17Z
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/10.3847/2041-8205/832/2/L21
Astrophysical Journal Letters. Bristol: Iop Publishing Ltd, v. 832, n. 2, 15 p., 2016.
2041-8205
http://hdl.handle.net/11449/162219
10.3847/2041-8205/832/2/L21
WOS:000389176100001
WOS000389176100001.pdf
url http://dx.doi.org/10.3847/2041-8205/832/2/L21
http://hdl.handle.net/11449/162219
identifier_str_mv Astrophysical Journal Letters. Bristol: Iop Publishing Ltd, v. 832, n. 2, 15 p., 2016.
2041-8205
10.3847/2041-8205/832/2/L21
WOS:000389176100001
WOS000389176100001.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Astrophysical Journal Letters
3,186
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 15
application/pdf
dc.publisher.none.fl_str_mv Iop Publishing Ltd
publisher.none.fl_str_mv Iop Publishing Ltd
dc.source.none.fl_str_mv Web of Science
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
_version_ 1797790120413233152