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GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

Title
GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
Authors
Abbott, B. P.Abbott, R.Abbott, T. D.Acernese, F.Ackley, K.Adams, C.Adams, T.Addesso, P.Adhikari, R. X.Adya, V. B.Affeldt, C.Afrough, M.Agarwal, B.Agathos, M.Agatsuma, K.Aggarwal, N.Aguiar, O. D.Aiello, L.Ain, A.Ajith, P.Allen, B.Allen, G.Allocca, A.Altin, P. A.Amato, A.Ananyeva, A.Anderson, S. B.Anderson, W. G.Angelova, S. V.Antier, S.Appert, S.Arai, K.Araya, M. C.Areeda, J. S.Arnaud, N.Arun, K. G.Ascenzi, S.Ashton, G.Ast, M.Aston, S. M.Astone, P.Atallah, D. V.Aufmuth, P.Aulbert, C.AultONeal, K.Austin, C.Avila-Alvarez, A.Babak, S.Bacon, P.Bader, M. K. M.Bae, S.Bailes, M.Baker, P. T.Baldaccini, F.Ballardin, G.Ballmer, S. W.Banagiri, S.Barayoga, J. C.Barclay, S. E.Barish, B. C.Barker, D.Barkett, K.Barone, F.Barr, B.Barsotti, L.Barsuglia, M.Barta, D.Barthelmy, S. D.Bartlett, J.Bartos, I.Bassiri, R.Basti, A.Batch, J. C.Bawaj, M.Bayley, J. C.Bazzan, M.Becsy, B.Beer, C.Bejger, M.Belahcene, I.Bell, A. S.Berger, B. K.Bergmann, G.Bernuzzi, S.Bero, J. J.Berry, C. P. L.Bersanetti, D.Bertolini, A.Betzwieser, J.Bhagwat, S.Bhandare, R.Bilenko, I. A.Billingsley, G.Billman, C. R.Birch, J.Birney, R.Birnholtz, O.Biscans, S.Biscoveanu, S.Bisht, A.Bitossi, M.Biwer, C.Bizouard, M. A.Blackburn, J. K.Blackman, J.Blair, C. D.Blair, D. G.Blair, R. M.Bloemen, S.Bock, O.Bode, N.Boer, M.Bogaert, G.Bohe, A.Bondu, F.Bonilla, E.Bonnand, R.Boom, B. A.Bork, R.Boschi, V.Bose, S.Bossie, K.Bouffanais, Y.Bozzi, A.Bradaschia, C.Brady, P. R.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.Brunett, S.Buchanan, C. C.Buikema, A.Bulik, T.Bulten, H. J.Buonanno, A.Buskulic, D.Buy, C.Byer, R. L.Cabero, M.Cadonati, L.Cagnoli, G.Cahillane, C.Bustillo, J. CalderonCallister, T. A.Calloni, E.Camp, J. B.Canepa, M.Canizares, P.Cannon, K. C.Cao, H.Cao, J.Capano, C. D.Capocasa, E.Carbognani, F.Caride, S.Carney, M. F.Carullo, G.Diaz, J. CasanuevaCasentini, C.Caudill, S.Cavagli, M.Cavalier, F.Cavalieri, R.Cella, G.Cepeda, C. B.Cerda-Duran, P.Cerretani, G.Cesarini, E.Chamberlin, S. J.Chan, M.Chao, S.Charlton, P.Chase, E.Chassande-Mottin, E.Chatterjee, D.Chatziioannou, K.Cheeseboro, B. D.Chen, H. Y.Chen, X.Chen, Y.Cheng, H. -P.Chia, H.Chincarini, A.Chiummo, A.Chmiel, T.Cho, H. S.Cho, M.Chow, J. H.Christensen, N.Chu, Q.Chua, A. J. K.Chua, S.Chung, A. K. W.Chung, S.Ciani, G.Ciolfi, R.Cirelli, C. E.Cirone, A.Clara, F.Clark, J. A.Clearwater, P.Cleva, F.Cocchieri, C.Coccia, E.Cohadon, P. -F.Cohen, D.Colla, A.Collette, C. G.Cominsky, L. R.Constancio, M., Jr.Conti, L.Cooper, S. J.Corban, P.Corbitt, T. R.Cordero-Carrion, I.Corley, K. R.Cornish, N.Corsi, A.Cortese, S.Costa, C. A.Coughlin, M. W.Coughlin, S. B.Coulon, J. -P.Countryman, S. T.Couvares, P.Covas, P. B.Cowan, E. E.Coward, D. M.Cowart, M. J.Coyne, D. C.Coyne, R.Creighton, J. D. E.Creighton, T. D.Cripe, J.Crowder, S. G.Cullen, T. 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J.Favata, M.Fays, M.Fee, C.Fehrmann, H.Feicht, J.Fejer, M. M.Fernandez-Galiana, A.Ferrante, I.Ferreira, E. C.Ferrini, F.Fidecaro, F.Finstad, D.Fiori, I.Fiorucci, D.Fishbach, M.Fisher, R. P.Fitz-Axen, M.Flaminio, R.Fletcher, M.Fong, H.Font, J. A.Forsyth, P. W. F.Forsyth, S. S.Fournier, J. -D.Frasca, S.Frasconi, F.Frei, Z.Freise, A.Frey, R.Frey, V.Fries, E. M.Fritschel, P.Frolov, V. V.Fulda, P.Fyffe, M.Gabbard, H.Gadre, B. U.Gaebel, S. M.Gair, J. R.Gammaitoni, L.Ganija, M. R.Gaonkar, S. G.Garcia-Quiros, C.Garufi, F.Gateley, B.Gaudio, S.Gaur, G.Gayathri, V.Gehrels, N.Gemme, G.Genin, E.Gennai, A.George, D.George, J.Gergely, L.Germain, V.Ghonge, S.Ghosh, AbhirupGhosh, ArchismanGhosh, S.Giaime, J. A.Giardina, K. D.Giazotto, A.Gill, K.Glover, L.Goetz, E.Goetz, R.Gomes, S.Goncharov, B.Gonzalez, G.Castro, J. M. GonzalezGopakumar, A.Gorodetsky, M. L.Gossan, S. E.Gosselin, M.Gouaty, R.Grado, A.Graef, C.Granata, M.Grant, A.Gras, S.Gray, C.Greco, G.Green, A. C.Gretarsson, E. 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Ewha Authors
김정리
SCOPUS Author ID
김정리scopus
Issue Date
2017
Journal Title
PHYSICAL REVIEW LETTERS
ISSN
0031-9007JCR Link

1079-7114JCR Link
Citation
PHYSICAL REVIEW LETTERS vol. 119, no. 16
Publisher
AMER PHYSICAL SOC
Indexed
SCIE; SCOPUS WOS
Document 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 x 10(4) years. We infer the component masses of the binary to be between 0.86 and 2.26 M-circle dot, 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-circle dot, with the total mass of the system 2.74(-0.01)(+0.04) M-circle dot. 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 gamma-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 gamma-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.
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DOI
10.1103/PhysRevLett.119.161101
Appears in Collections:
자연과학대학 > 물리학전공 > Journal papers
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