Year: 2017
Type: article
Abstract: On August 17, 2017 at 12∶41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×10^{4} years. We infer the component masses of the binary to be between 0.86 and 2.26 M_{⊙}, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M_{⊙}, with the total mass of the system 2.74_{-0.01}^{+0.04}M_{⊙}. The source was localized within a sky region of 28 deg^{2} (90% probability) and had a luminosity distance of 40_{-14}^{+8} Mpc, the closest and most precisely localized gravitational-wave signal yet. The association with the γ-ray burst GRB 170817A, detected by Fermi-GBM 1.7 s after the coalescence, corroborates the hypothesis of a neutron star merger and provides the first direct evidence of a link between these mergers and short γ-ray bursts. Subsequent identification of transient counterparts across the electromagnetic spectrum in the same location further supports the interpretation of this event as a neutron star merger. This unprecedented joint gravitational and electromagnetic observation provides insight into astrophysics, dense matter, gravitation, and cosmology.
Source: Physical Review Letters
Authors: B. P. Abbott, R. Abbott, T. D. Abbott, F. Acernese, K. Ackley, C. Adams, T. Adams, P. Addesso, R. X. Adhikari, V. B. Adya, C. Affeldt, M. Afrough, B. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, B. Allen, G. Allen, A. Allocca, P. A. Altin, A. Amato, A. Ananyeva, S. B. Anderson, W. G. Anderson, S. V. Angelova, S. Antier, S. Appert, K. Arai, M. C. Araya, J. S. Areeda, N. Arnaud, K. G. Arun, S. Ascenzi, G. Ashton, M. Ast, S. M. Aston, P. Astone, D. V. Atallah, P. Aufmuth, C. Aulbert, K. AultONeal, C. Austin, A. Avila-Alvarez, S. Babak, P. Bacon, M. K. M. Bader, S. Bae, M. Bailes, P. T. Baker, F. Baldaccini, G. Ballardin, S. W. Ballmer, S. Banagiri, J. C. Barayoga, S. E. Barclay, B. C. Barish, D. Barker, K. Barkett, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, S. D. Barthelmy, J. Bartlett, I. Bartos, R. Bassiri, A. Basti, J. C. Batch, M. Bawaj, J. C. Bayley, M. Bazzan, B. Bécsy, C. Beer, M. Bejger, I. Belahcene, A. S. Bell, B. K. Berger, G. Bergmann, S. Bernuzzi, J. J. Bero, C. P. L. Berry, D. Bersanetti, A. Bertolini, J. Betzwieser, S. Bhagwat, R. Bhandare, I. A. Bilenko, G. Billingsley, C. R. Billman, J. Birch, I. A. Birney, O. Birnholtz, S. Biscans, S. Biscoveanu, A. Bisht, M. Bitossi, C. Biwer, M. A. Bizouard, J. K. Blackburn, J. Blackman, C. D. Blair, D. G. Blair, R. M. Blair, S. Bloemen, O. Bock, N. Bode, M. Boer, G. Bogaert, A. Bohe, F. Bondu, E. Bonilla, R. Bonnand, B. A. Boom, R. Bork, V. Boschi, S. Bose, K. Bossie, Y. Bouffanais, A. Bozzi, C. Bradaschia, P. R. Brady, M. Branchesi, J. E. Brau, T. Briant, A. Brillet, M. Brinkmann, V. Brisson, P. Brockill, J. E. Broida, A. F. Brooks, D. A. Brown, D. D. Brown, S. Brunett, C. C. Buchanan, A. Buikema, T. Bulik, H. J. Bulten, A. Buonanno, D. Buskulic, C. Buy, R. L. Byer, M. Cabero, L. Cadonati, G. Cagnoli, C. Cahillane, J. Calderón Bustillo, T. A. Callister, E. Calloni, J. B. Camp, M. Canepa, P. Canizares, K. C. Cannon, H. Cao, J. Cao, C. D. 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Institutions: California Institute of Technology, Louisiana State University, University of Salerno, Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, University of Florida, ARC Centre of Excellence for Gravitational Wave Discovery, Monash University, LIGO Scientific Collaboration, Université Savoie Mont Blanc, University of Sannio, Max Planck Institute for Gravitational Physics, University of Mississippi, University of Illinois Urbana-Champaign, National Center for Supercomputing Applications, University of Cambridge, National Institute for Subatomic Physics, Massachusetts Institute of Technology, Instituto Nacional de Pesquisas Espaciais, Istituto Nazionale di Fisica Nucleare, Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso, Gran Sasso Science Institute, Inter-University Centre for Astronomy and Astrophysics, Tata Institute of Fundamental Research, International Centre for Theoretical Sciences, Leibniz University Hannover, University of Wisconsin–Milwaukee, University of Pisa, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Australian National University, Laboratoire des Matériaux Avancés, University of the West of Scotland, Université Paris-Sud, California State University, Fullerton, European Gravitational Observatory, Chennai Mathematical Institute, University of Rome Tor Vergata, Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata, Universität Hamburg, Istituto Nazionale di Fisica Nucleare, Sezione di Roma I, Cardiff University, Embry-Riddle Aeronautical University Prescott Arizona Campus, Embry–Riddle Aeronautical University, Université Paris Diderot, Korea Institute of Science & Technology Information, Swinburne University of Technology, West Virginia University, University of Perugia, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Syracuse University, University of Minnesota, Scottish Universities Physics Alliance, University of Glasgow, HUN-REN Wigner Research Centre for Physics, Goddard Space Flight Center, Columbia University, Stanford University, Università di Camerino, University of Padua, Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Eötvös Loránd University, Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, University of Parma, Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca, Istituto Nazionale di Fisica Nucleare, Gruppo Collegato di Parma, Rochester Institute of Technology, University of Birmingham, Istituto Nazionale di Fisica Nucleare, Sezione di Genova, Raja Ramanna Centre for Advanced Technology, Lomonosov Moscow State University, University of Strathclyde, Pennsylvania State University, The University of Western Australia, Radboud University Nijmegen, Université Côte d'Azur, Communauté d'universités et d'établissements Université Côte d'Azur, Fonctions Optiques pour les Technologies de l’information, Washington State University, University of Oregon, Laboratoire Kastler Brossel, Carleton College, The University of Adelaide, University of Warsaw, Vrije Universiteit Amsterdam, University of Maryland, College Park, Georgia Institute of Technology, Lyon 1 Université, University of Naples Federico II, University of Genoa, The University of Tokyo, Tsinghua University, Texas Tech University, Kenyon College, Universitat de València, Centro Ricerche Enrico Fermi, National Tsing Hua University, Charles Sturt University, Northwestern University, University of Toronto, Canadian Institute for Theoretical Astrophysics, University of Chicago, Pusan National University, Chinese University of Hong Kong, Istituto Nazionale di Fisica Nucleare, Trento Institute for Fundamental Physics And Applications, Osservatorio Astronomico di Padova, National Institute for Astrophysics, The University of Melbourne, Sapienza University of Rome, Université Libre de Bruxelles, Sonoma State University, Montana State University, Universitat de les Illes Balears, The University of Texas Rio Grande Valley, Bellevue College, Bellevue University, Institute for Plasma Research, University of Sheffield, California State University System, California State University Los Angeles, University of Trento, Montclair State University, National Astronomical Observatory of Japan, University of Edinburgh, Indian Institute of Science Education and Research, Tirupati, Indian Institute of Science Education and Research Thiruvananthapuram, University of Szeged, University of Michigan, Astronomical Observatory of Capodimonte, University of Urbino, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, University of Zurich, American University, University of Southampton, University of Białystok, University of Washington Bothell, Institute of Applied Physics, Korea Astronomy and Space Science Institute, Inje University, National Institute for Mathematical Sciences, National Centre for Nuclear Research, Institute of Mathematics, Hillsdale College, Seoul National University, Hanyang University, Marshall Space Flight Center, National Aeronautics and Space Administration, Centre National de la Recherche Scientifique, ESPCI Paris, Southern University and Agricultural and Mechanical College, William & Mary, Scientific Centre of Monaco, Indian Institute of Technology Madras, Istituto Nazionale di Fisica Nucleare, Sezione di Torino, Institut des Hautes Études Scientifiques, Indian Institute of Science Education and Research Kolkata, Whitman College, Indian Institute of Technology Bombay, Scuola Normale Superiore, Université de Lyon, Hobart and William Smith Colleges, University of Zielona Góra, University of Washington, University of London, King's College London, Indian Institute of Technology Gandhinagar, Indian Institute of Technology Hyderabad, Universidade Federal do Rio Grande do Norte, Andrews University, University of Siena, Trinity University, Abilene Christian University, Colorado State University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Estimated APC paid: $3,750
Funders: National Science Foundation, National Aeronautics and Space Administration, Kavli Foundation, California Institute of Technology, Canadian Institute for Advanced Research, Institut des Origines de Lyon, Ontario Ministry of Economic Development and Innovation, Leverhulme Trust, Royal Society, Scottish Funding Council, Scottish Universities Physics Alliance, European Commission, National Research Foundation, Department of Science and Technology, Ministry of Science and Technology, India, Council of Scientific and Industrial Research, India, Abdus Salam International Centre for Theoretical Physics, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Stichting voor Fundamenteel Onderzoek der Materie, National Natural Science Foundation of China, Russian Foundation for Basic Research, Ministry of Science and Technology of the People's Republic of China, Research Grants Council, University Grants Committee, Industry Canada, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Generalitat Valenciana, Ministério da Ciência, Tecnologia e Inovação, Hungarian Scientific Research Fund, National Research Foundation of Korea, Max-Planck-Gesellschaft, Narodowe Centrum Nauki, Ministry of Education, India, Centre National de la Recherche Scientifique, Russian Science Foundation, Ministero dello Sviluppo Economico, Universitat de les Illes Balears, Nemzeti Kutatási Fejlesztési és Innovációs Hivatal, Istituto Nazionale di Fisica Nucleare, ICTP South American Institute for Fundamental Research, Govern de les Illes Balears, Jet Propulsion Laboratory, Natural Sciences and Engineering Research Council of Canada, Science and Technology Facilities Council, Australian Research Council, Japan Society for the Promotion of Science, Science and Engineering Research Board, Instituto Nazionale di Fisica Nucleare, European Regional Development Fund, Agencia Estatal de Investigación, Conselleria d'Educació, Investigació, Cultura i Esport, National Research, Development and Innovation Office, Division of Human Resource Development
Awards: G1006713238, G1239773027, Investigations in Gravitational Radiation, G1338097928, Breaking the seismic wall: How to improve gravitational waves at low frequency, G1508433701, G1510748143, UK Involvement in the Operation of Advanced LIGO, G1643540916, Constraining compact binary formation with gravitational wave observations, G1706433362, G1934966033, Investigations in gravitational radiation, G1993359131, Investigations in Gravitational Radiation, G2068338807, Developing multiwavelength gravitational wave astrophysics, Proposal for UK Involvement in the Operation of Advanced LIGO, Equipment in support of Investigations in Gravitational Radiation, Investigations in Gravitational Radiation, Suspension and advance material for future gravitation wave detectors, Exploring quantum aspects of gravitational-wave detectors, Investigations in Gravitational Radiation, Proposal for UK Involvement in the Operation of Advanced LIGO, G289284436, G2961063521, G3048158438, G3139561911, G3235010149, UK Involvement in the Operation of Advanced LIGO, Low-Latency Compact Object Searches with LIGO, Virgo and KAGRA in O2 and O3, From massive stars to neutron stars and black holes as gravitational wave sources, Fundamental Physics from the Planck Scale to the LHC, G3599894334, G3650528599, G3825855354, Data analysis for gravitational wave detectors, G406209335, Investigations in Gravitational radiation, Investigations in Gravitational Radiation, Proposal for UK Involvement in the Operation of Advanced LIGO, Gravity beyond the apple, Investigations in Gravitational Radiation, Investigations in Gravitational Radiation, G425118790, G436248402, Enhance speed meters for gravitation wave detection, Investigations in Gravitational Radiation, G4655137926, G4794108926, Surveying black holes and neutron stars with gravitational waves, G4926523277, UK Involvement in the advanced LIGO Gravitational Wave Project, G500372278, G5027012758, G5426102616, G5454877379, Investigations in Gravitational Radiation, Investigations in Gravitational Radiation, G5566666545, G5624451344, G5730887123, Surveying black holes and neutron stars with gravitational waves, G6080433432, G6162394363, Nationalist mobilization, civil society and the transnationalization of claims for political self-determination in the EU, G6225947758, Birmingham Astrophysics- Rolling Grant 2010-2015, Investigations in Gravitational Radiation, Black-hole-binary simulations for gravitational-wave astronomy, G638338023, UK Involvement in the Operation of Advanced LIGO, Investigations in Gravitational Radiation, G6628833526, G6721355244, Developing low noise coatings for GW detectors, using next generation techniques such as ECR ion-beam deposition, and plasma-assisted deposition., G6979865909, G7053373622, General Relativistic Astrophysics, G7201779739, G7213046781, Proposal for UK Involvement in the Operation of Advanced LIGO, G7315994006, G7364495178, G7422912066, G7508136664, G7632615682, Investigations in Gravitational Radiation, Characterisation of optical materials for next generation gravitational wave detectors, G7706638305, G7799948282, Capital Equipment in support of 'Investigations in Gravitational Radiation', 2014, G7902306514, G8156222622, Constraining compact binary formation with gravitational wave observations, G8233711064, Investigations in Gravitational Radiation, Astrophysics at the University of Birmingham: Consolidated Grant 2016-2019, G8444912688, G8544846704, Investigations in Gravitational Radiation, Birmingham Astrophysics: Consolidated Grant 2013-2016, G8648593922, Gravitational Wave Astronomy: A New Window onto the Universe, G8829743996, UK Involvement in the Operation of Advanced LIGO, Investigations in Gravitational Radiation, G8992648555, G9000024963, G9000068029, G9000099665, G9000147322, G9000157696, G9000169693, G9000173921, G9000293111, G9000303728, G9000336776, Bringing Advanced LIGO to Design Performance and Further Sensitivity Enhancements
OpenAlex ID: W2765081049