Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

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dc.identifier.uri http://dx.doi.org/10.15488/2271
dc.identifier.uri http://www.repo.uni-hannover.de/handle/123456789/2297
dc.contributor.author Abbott, B.P.
dc.contributor.author Abbott, R.
dc.contributor.author Abbott, T.D.
dc.contributor.author Acernese, F.
dc.contributor.author Ackley, K.
dc.contributor.author et al.
dc.contributor.author LIGO Scientific Collaboration
dc.contributor.author Virgo Collaboration
dc.date.accessioned 2017-11-13T08:18:11Z
dc.date.available 2017-11-13T08:18:11Z
dc.date.issued 2017
dc.identifier.citation Abbott, B.P.; Abbott, R.; Abbott, T.D.; Acernese, F.; Ackley, K.et, al., (LIGO Scientific Collaboration and Virgo Collaboration, Fermi Gamma-ray Burst Monitor, and INTEGRAL): Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A. In: Astrophysical Journal Letters 848 (2017), Nr. 2, L13. DOI: https://doi.org/10.3847/2041-8213/aa920c
dc.description.abstract On 2017 August 17, the gravitational-wave event GW170817 was observed by the Advanced LIGO and Virgo detectors, and the gamma-ray burst (GRB) GRB 170817A was observed independently by the Fermi Gamma-ray Burst Monitor, and the Anti-Coincidence Shield for the Spectrometer for the International Gamma-Ray Astrophysics Laboratory. The probability of the near-simultaneous temporal and spatial observation of GRB 170817A and GW170817 occurring by chance is . We therefore confirm binary neutron star mergers as a progenitor of short GRBs. The association of GW170817 and GRB 170817A provides new insight into fundamental physics and the origin of short GRBs. We use the observed time delay of between GRB 170817A and GW170817 to: (i) constrain the difference between the speed of gravity and the speed of light to be between and times the speed of light, (ii) place new bounds on the violation of Lorentz invariance, (iii) present a new test of the equivalence principle by constraining the Shapiro delay between gravitational and electromagnetic radiation. We also use the time delay to constrain the size and bulk Lorentz factor of the region emitting the gamma-rays. GRB 170817A is the closest short GRB with a known distance, but is between 2 and 6 orders of magnitude less energetic than other bursts with measured redshift. A new generation of gamma-ray detectors, and subthreshold searches in existing detectors, will be essential to detect similar short bursts at greater distances. Finally, we predict a joint detection rate for the Fermi Gamma-ray Burst Monitor and the Advanced LIGO and Virgo detectors of 0.1–1.4 per year during the 2018–2019 observing run and 0.3–1.7 per year at design sensitivity. eng
dc.language.iso eng
dc.publisher Bristol : Institute of Physics Publishing
dc.relation.ispartofseries Astrophysical Journal Letters 848 (2017), Nr. 2
dc.rights CC BY 3.0 Unported
dc.rights.uri https://creativecommons.org/licenses/by/3.0/
dc.subject binaries: close eng
dc.subject gamma-ray burst: general eng
dc.subject gravitational waves eng
dc.subject Gravitationswelle ger
dc.subject.ddc 520 | Astronomie, Kartographie ger
dc.title Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
dc.type article
dc.type Text
dc.relation.essn 2041-8213
dc.relation.issn 2041-8205
dc.relation.doi https://doi.org/10.3847/2041-8213/aa920c
dc.bibliographicCitation.issue 2
dc.bibliographicCitation.volume 848
dc.bibliographicCitation.firstPage L13
dc.description.version publishedVersion
tib.accessRights frei zug�nglich


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