Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6543
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dc.contributor.authorMoharana, Reetanjali-
dc.contributor.authorRazzaque, Soebur-
dc.contributor.authorGupta, Nayantara-
dc.contributor.authorMeszaros, Peter-
dc.date.accessioned2016-12-23T12:21:48Z-
dc.date.available2016-12-23T12:21:48Z-
dc.date.issued2016-06-
dc.identifier.citationPhysical Review D, 2016, Vol.93, p 123011en_US
dc.identifier.issn2470-0010-
dc.identifier.issn2470-0029 (online)-
dc.identifier.urihttp://hdl.handle.net/2289/6543-
dc.descriptionOpen Accessen_US
dc.description.abstractHigh-energy neutrinos (HEN) and gravitational waves (GW) can probe astrophysical sources in addition to electromagnetic observations. Multimessenger studies can reveal the nature of the sources, which may not be discerned from one type of signal alone. We discuss HEN emission in connection with the Advanced Laser Interferometer Gravitational-Wave Observatory event GW150914, which could be associated with a short gamma-ray burst detected by the Fermi Gamma-Ray Burst Monitor 0.4 s after the GW event and within localization uncertainty of the GW event. We calculate HEN flux from this short gamma-ray burst, GW150914-GBM, and show that nondetection of a high-energy starting event by the IceCube Neutrino Observatory can constrain the total isotropic-equivalent jet energy of this short burst to be less than 3×1052  erg.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.relation.urihttp://arxiv.org/abs/1602.08436en_US
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevD.93.123011en_US
dc.rights2016 American Physical Societyen_US
dc.titleHigh energy neutrinos from the gravitational wave event gw150914 possibly associated with a short gamma-ray bursten_US
dc.typeArticleen_US
Appears in Collections:Research Papers (A&A)

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