| Literature DB >> 29099225 |
B P Abbott1, R Abbott1, T D Abbott2, F Acernese3,4, K Ackley5,6, C Adams7, T Adams8, P Addesso9, R X Adhikari1, V B Adya10, C Affeldt10, M Afrough11, B Agarwal12, M Agathos13, K Agatsuma14, N Aggarwal15, O D Aguiar16, L Aiello17,18, A Ain19, P Ajith20, B Allen10,21,22, G Allen12, A Allocca23,24, P A Altin25, A Amato26, A Ananyeva1, S B Anderson1, W G Anderson21, S V Angelova27, S Antier28, S Appert1, K Arai1, M C Araya1, J S Areeda29, N Arnaud28,30, K G Arun31, S Ascenzi32,33, G Ashton10, M Ast34, S M Aston7, P Astone35, D V Atallah36, P Aufmuth22, C Aulbert10, K AultONeal37, C Austin2, A Avila-Alvarez29, S Babak38, P Bacon39, M K M Bader14, S Bae40, M Bailes41, P T Baker42, F Baldaccini43,44, G Ballardin30, S W Ballmer45, S Banagiri46, J C Barayoga1, S E Barclay47, B C Barish1, D Barker48, K Barkett49, F Barone3,4, B Barr47, L Barsotti15, M Barsuglia39, D Barta50, S D Barthelmy51, J Bartlett48, I Bartos5,52, R Bassiri53, A Basti23,24, J C Batch48, M Bawaj44,54, J C Bayley47, M 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Donovan15, K L Dooley11, S Doravari10, I Dorrington36, R Douglas47, M Dovale Álvarez62, T P Downes21, M Drago10, C Dreissigacker10, J C Driggers48, Z Du85, M Ducrot8, R Dudi36, P Dupej47, S E Dwyer48, T B Edo109, M C Edwards75, A Effler7, H-B Eggenstein10,38, P Ehrens1, J Eichholz1, S S Eikenberry5, R A Eisenstein15, R C Essick15, D Estevez8, Z B Etienne42, T Etzel1, M Evans15, T M Evans7, M Factourovich52, V Fafone17,32,33, H Fair45, S Fairhurst36, X Fan85, S Farinon63, B Farr94, W M Farr62, E J Fauchon-Jones36, M Favata112, M Fays36, C Fee87, H Fehrmann10, J Feicht1, M M Fejer53, A Fernandez-Galiana15, I Ferrante23,24, E C Ferreira16, F Ferrini30, F Fidecaro23,24, D Finstad45, I Fiori30, D Fiorucci39, M Fishbach94, R P Fisher45, M Fitz-Axen46, R Flaminio26,113, M Fletcher47, H Fong93, J A Font88,114, P W F Forsyth25, S S Forsyth80, J-D Fournier70, S Frasca35,100, F Frasconi24, Z Frei57, A Freise62, R Frey73, V Frey28, E M Fries1, P Fritschel15, V V Frolov7, P Fulda5, M Fyffe7, H 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Hardwick2, J Harms17,18, G M Harry125, I W Harry38, M J Hart47, C-J Haster93, K Haughian47, J Healy61, A Heidmann74, M C Heintze7, H Heitmann70, P Hello28, G Hemming30, M Hendry47, I S Heng47, J Hennig47, A W Heptonstall1, M Heurs10,22, S Hild47, T Hinderer69, W C G Ho126, D Hoak30, D Hofman26, K Holt7, D E Holz94, P Hopkins36, C Horst21, J Hough47, E A Houston47, E J Howell68, A Hreibi70, Y M Hu10, E A Huerta12, D Huet28, B Hughey37, S Husa105, S H Huttner47, T Huynh-Dinh7, N Indik10, R Inta86, G Intini35,100, H N Isa47, J-M Isac74, M Isi1, B R Iyer20, K Izumi48, T Jacqmin74, K Jani80, P Jaranowski127, S Jawahar66, F Jiménez-Forteza105, W W Johnson2, N K Johnson-McDaniel13, D I Jones126, R Jones47, R J G Jonker14, L Ju68, J Junker10, C V Kalaghatgi36, V Kalogera92, B Kamai1, S Kandhasamy7, G Kang40, J B Kanner1, S J Kapadia21, S Karki73, K S Karvinen10, M Kasprzack2, W Kastaun10, M Katolik12, E Katsavounidis15, W Katzman7, S Kaufer22, K Kawabe48, F Kéfélian70, D Keitel47, A J Kemball12, R Kennedy109, C Kent36, J S Key128, F Y Khalili65, I Khan17,33, S Khan10, Z Khan108, E A Khazanov129, N Kijbunchoo25, Chunglee Kim130, J C Kim131, K Kim96, W Kim76, W S Kim132, Y-M Kim95, S J Kimbrell80, E J King76, P J King48, M Kinley-Hanlon125, R Kirchhoff10, J S Kissel48, L Kleybolte34, S Klimenko5, T D Knowles42, P Koch10, S M Koehlenbeck10, S Koley14, V Kondrashov1, A Kontos15, M Korobko34, W Z Korth1, I Kowalska77, D B Kozak1, C Krämer10, V Kringel10, B Krishnan10, A Królak133,134, G Kuehn10, P Kumar93, R Kumar108, S Kumar20, L Kuo90, A Kutynia133, S Kwang21, B D Lackey38, K H Lai96, M Landry48, R N Lang135, J Lange61, B Lantz53, R K Lanza15, S L Larson92, A Lartaux-Vollard28, P D Lasky6, M Laxen7, A Lazzarini1, C Lazzaro56, P Leaci35,100, S Leavey47, C H Lee95, H K Lee136, H M Lee137, H W Lee131, K Lee47, J Lehmann10, A Lenon42, E Leon29, M Leonardi98,111, N Leroy28, N Letendre8, Y Levin6, T G F Li96, S D Linker110, T B Littenberg138, J Liu68, X Liu21, R K L Lo96, N A Lockerbie66, L T London36, J E Lord45, M Lorenzini17,18, V Loriette139, M Lormand7, G Losurdo24, J D Lough10, C O Lousto61, G Lovelace29, H Lück10,22, D Lumaca32,33, A P Lundgren10, R Lynch15, Y Ma49, R Macas36, S Macfoy27, B Machenschalk10, M MacInnis15, D M Macleod36, I Magaña Hernandez21, F Magaña-Sandoval45, L Magaña Zertuche45, R M Magee67, E Majorana35, I Maksimovic139, N Man70, V Mandic46, V Mangano47, G L Mansell25, M Manske21,25, M Mantovani30, F Marchesoni44,54, F Marion8, S Márka52, Z Márka52, C Markakis12, A S Markosyan53, A Markowitz1, E Maros1, A Marquina103, P Marsh128, F Martelli122,123, L Martellini70, I W Martin47, R M Martin112, D V Martynov15, J N Marx1, K Mason15, E Massera109, A Masserot8, T J Massinger1, M Masso-Reid47, S Mastrogiovanni35,100, A Matas46, F Matichard1,15, L Matone52, N Mavalvala15, N Mazumder72, R McCarthy48, D E McClelland25, S McCormick7, L McCuller15, S C McGuire140, G McIntyre1, J McIver1, D J McManus25, L McNeill6, T McRae25, S T McWilliams42, D Meacher67, G D Meadors10,38, M Mehmet10, J Meidam14, E Mejuto-Villa9, A Melatos99, G Mendell48, R A Mercer21, E L Merilh48, M Merzougui70, S Meshkov1, C Messenger47, C Messick67, R Metzdorff74, P M Meyers46, H Miao62, C Michel26, H Middleton62, E E Mikhailov141, L Milano4,82, A L Miller5,35,100, B B Miller92, J Miller15, M Millhouse104, M C Milovich-Goff110, O Minazzoli70,142, Y Minenkov33, J Ming38, C Mishra143, S Mitra19, V P Mitrofanov65, G Mitselmakher5, R Mittleman15, D Moffa87, A Moggi24, K Mogushi11, M Mohan30, S R P Mohapatra15, I Molina29, M Montani122,123, C J Moore13, D Moraru48, G Moreno48, S Morisaki84, S R Morriss106, B Mours8, C M Mow-Lowry62, G Mueller5, A W Muir36, Arunava Mukherjee10, D Mukherjee21, S Mukherjee106, N Mukund19, A Mullavey7, J Munch76, E A Muñiz45, M Muratore37, P G Murray47, A Nagar89,144,145, K Napier80, I Nardecchia32,33, L Naticchioni35,100, R K Nayak146, J Neilson110, G Nelemans14,69, T J N Nelson7, M Nery10, A Neunzert119, L 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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.Entities:
Year: 2017 PMID： 29099225 DOI： 10.1103/PhysRevLett.119.161101
Source DB: PubMed Journal: Phys Rev Lett ISSN： 0031-9007 Impact factor: 9.161