Artículos de revistas
Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube
Fecha
2017-07-15Registro en:
Physical Review D, v. 96, n. 2, 2017.
2470-0029
2470-0010
10.1103/PhysRevD.96.022005
2-s2.0-85027050091
Autor
Université de Haute Alsace
Rambla Exposició
Sezione di Genova
Friedrich-Alexander-Universität Erlangen-Nürnberg
Universitat Politècnica de València
CPPM
Sorbonne Paris Cité
Universitat de València
Pôle de l'Étoile Site de Château-Gombert
Laboratori Nazionali Del Sud (LNS)
Science Park
Universiteit Leiden
Science Park 105
Sezione di Roma
Dipartimento di Fisica dell'Università la Sapienza
Institute for Space Science
Gran Sasso Science Institute
Sezione di Bologna
Sezione di Bari
Observatoire de la Côte d'Azur
Université Paris-Sud
University Mohammed i
Universität Würzburg
Astronomia dell'Università
CNRS/IN2P3
Sezione di Catania
CNRS ENSAM LSIS UMR 7296
Institut Universitaire de France
Royal Netherlands Institute for Sea Research (NIOZ)
Dipartimento di Fisica dell'Università
Leninskie Gory
Aix-Marseille University
Dipartimento di Fisica Ed Astronomia dell'Università
CEA Saclay
Sezione di Pisa
Sezione di Napoli
Università Federico II di Napoli
IPHC UMR 7178
University Mohammed v in Rabat
University of Adelaide
DESY
University of Canterbury
Université Libre de Bruxelles
University of Wisconsin
Stockholm University
Université de Genève
Marquette University
Pennsylvania State University
University of Mainz
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RWTH Aachen University
South Dakota School of Mines and Technology
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University of Wuppertal
University of Rochester
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Lawrence Berkeley National Laboratory
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Dienst ELEM
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Technische Universität München
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University of Sannio at Benevento
Max-Planck-Institut für Gravitationsphysik
Instituto Nacional de Pesquisas Espaciais
Sezione di Roma Tor Vergata
Inter-University Centre for Astronomy and Astrophysics
Tata Institute of Fundamental Research
University of Wisconsin-Milwaukee
Leibniz Universität Hannover
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California State University Fullerton
Université Paris-Saclay
Chennai Mathematical Institute
Università di Roma Tor Vergata
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RMKI
Columbia University
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Polish Academy of Sciences
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RRCAT
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Radboud University Nijmegen
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Trento Institute for Fundamental Physics and Applications
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Abilene Christian University
CNRS LSIS UMR 7296
Université du Sud Toulon-Var
Institución
Resumen
The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by Antares, within ±500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection to constrain isotropic-equivalent high-energy neutrino emission from GW151226, adopting the GW event's 3D localization, to less than 2×1051-2×1054 erg.