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GW170104: Observation of a 50-solar-mass binary black hole coalescence at redshift 0.2
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- المؤلفون: Abbott, Benjamin P.; Abbott, Rich; Abbott, Thomas D.; Acernese, Fausto; Ackley, Kendall; Adams, Carl; Adams, Thomas; Addesso, Paolo; Adhikari, Rana X.; Adya, Vaishali B.; Affeldt, Christoph; Afrough, Mohammad; Agarwal, Bhanu; Agathos, Michalis; Agatsuma, Kazuhiro; Aggarwal, Nancy; Aguiar, Odylio D.; Aiello, Lorenzo; Ain, Anirban; Ajith, P.; Allen, Bruce; Allen, Gabrielle; Allocca, Annalisa; Altin, Paul A.; Amato, A.; Ananyeva, Alena; Anderson, Stuart B.; Anderson, Warren G.; Antier, Sarah; Appert, Stephen; Arai, Koji; Araya, Melody C.; Areeda, Joseph S.; Arnaud, Nicolas; Arun, Kg G.; Ascenzi, Stefano; Ashton, Gregory; Ast, M.; Aston, Stuart M.; Astone, Pia; Aufmuth, Peter; Aulbert, Carsten; Aultoneal, K.; Avila-Alvarez, A.; Babak, Stanislav; Bacon, Philippe; Bader, Maria K.M.; Bae, Sangwook; Baker, Paul T.; Baldaccini, Francesca; Ballardin, Giulio; Ballmer, Stefan W.; Banagiri, Sharan; Barayoga, Juan C.; Barclay, Sheena E.; Barish, Barry C.; Barker, David; Barone, Fabrizio; 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- المصدر:
ISSN: 0031-9007.- الموضوع:
black hole: spin; black hole: mass; black hole: binary: coalescence; mass: gravitation; graviton: mass; particle: massive; gravitational radiation; gravitational radiation: emission; gravitational radiation: direct detection; gravitational radiation detector; general relativity; dispersion relation; angular momentum; detector: network; LIGO; G033M; [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]; [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]- نوع التسجيلة:
article in journal/newspaper- اللغة:
English - المصدر:
- معلومة اضافية
- Contributors: Laboratoire d'Annecy de Physique des Particules (LAPP); Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS); Laboratoire des matériaux avancés (LMA); Université Claude Bernard Lyon 1 (UCBL); Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS); Laboratoire de l'Accélérateur Linéaire (LAL); Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS); AstroParticule et Cosmologie (APC (UMR_7164)); Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris; Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité); Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS); Université Nice Sophia Antipolis (1965 - 2019) (UNS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur; Université Côte d'Azur (UniCA)-Université Côte d'Azur (UniCA)-Centre National de la Recherche Scientifique (CNRS); Institut de Physique de Rennes (IPR); Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS); Laboratoire Kastler Brossel (LKB Collège de France ); Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS); École normale supérieure - Paris (ENS-PSL); Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL); Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF (institution))-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS); Université de Lyon; Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris); Université Paris Sciences et Lettres (PSL); LIGO Scientific; VIRGO
- بيانات النشر: HAL CCSD
American Physical Society - الموضوع: 2017
- Collection: HAL Lyon 1 (University Claude Bernard Lyon 1)
- نبذة مختصرة : International audience ; We describe the observation of GW170104, a gravitational-wave signal produced by the coalescence of a pair of stellar-mass black holes. The signal was measured on January 4, 2017 at 10∶11:58.6 UTC by the twin advanced detectors of the Laser Interferometer Gravitational-Wave Observatory during their second observing run, with a network signal-to-noise ratio of 13 and a false alarm rate less than 1 in 70 000 years. The inferred component black hole masses are 31. 2 + 8.4 − 6.0 M ⊙ and 19. 4 + 5.3 − 5.9 M ⊙ (at the 90% credible level). The black hole spins are best constrained through measurement of the effective inspiral spin parameter, a mass-weighted combination of the spin components perpendicular to the orbital plane, χ eff = − 0.1 2 + 0.21 − 0.30 . This result implies that spin configurations with both component spins positively aligned with the orbital angular momentum are disfavored. The source luminosity distance is 88 0 + 450 − 390 Mpc corresponding to a redshift of z = 0.1 8 + 0.08 − 0.07 . We constrain the magnitude of modifications to the gravitational-wave dispersion relation and perform null tests of general relativity. Assuming that gravitons are dispersed in vacuum like massive particles, we bound the graviton mass to m g ≤ 7.7 × 10 − 23 eV / c 2 . In all cases, we find that GW170104 is consistent with general relativity.
- Relation: info:eu-repo/semantics/altIdentifier/arxiv/1706.01812; hal-01645700; https://hal.science/hal-01645700; https://hal.science/hal-01645700/document; https://hal.science/hal-01645700/file/PhysRevLett.118.221101; ARXIV: 1706.01812; INSPIRE: 1602334
- الرقم المعرف: 10.1103/PhysRevLett.118.221101
- Rights: info:eu-repo/semantics/OpenAccess
- الرقم المعرف: edsbas.B47CECEB
- Contributors:
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