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Search for neutrinos in Super-Kamiokande associated with gravitational-wave events GW150914 and GW151226

Author
Abe, K.; Labarga Echeverría, Luis Alfonsountranslated; Fernandez, P.; The Super-Kamiokande Collaboration
Entity
UAM. Departamento de Física Teórica
Publisher
Institute of Physics Publishing
Date
2016-10-06
Citation
10.3847/2041-8205/830/1/L11
Astrophysical Journal Letters 830.1 (2016): L11
 
 
 
ISSN
2041-8205 (print); 2041-8213 (online)
DOI
10.3847/2041-8205/830/1/L11
Funded by
The Super-Kamiokande experiment has been built and operated from funding by the Japanese Ministry of Education, Culture, Sports, Science and Technology, the U.S. Department of Energy, and the U.S. National Science Foundation. Some of us have been supported by funds from the Korean Research Foundation (BK21 and KNRC), the National Research Foundation of Korea (NRF-20110024009), the European Union (H2020 RISE-GA641540-SKPLUS), the Japan Society for the Promotion of Science, the National Natural Science Foundation of China under grant No. 11235006, and the Scinet and Westgrid consortia of Compute Canada
Project
info:eu-repo/grantAgreement/EC/H2020/641540/EU//SKPLUS
Editor's Version
http://dx.doi.org/10.3847/2041-8205/830/1/L11
Subjects
Astroparticle physics; Gravitational waves; Neutrinos; Física
URI
http://hdl.handle.net/10486/677235
Note
Astrophysical Journal Letters 830.1 (2016): L11 reproduced by permission of the AAS
Rights
© 2016. The American Astronomical Society

Abstract

We report the results from a search in Super-Kamiokande for neutrino signals coincident with the first detected gravitational-wave events, GW150914 and GW151226, as well as LVT151012, using a neutrino energy range from 3.5 MeV to 100 PeV. We searched for coincident neutrino events within a time window of ±500 s around the gravitational-wave detection time. Four neutrino candidates are found for GW150914, and no candidates are found for GW151226. The remaining neutrino candidates are consistent with the expected background events. We calculated the 90% confidence level upper limits on the combined neutrino fluence for both gravitational-wave events, which depends on event energy and topologies. Considering the upward-going muon data set (1.6 GeV-100 PeV), the neutrino fluence limit for each gravitational-wave event is 14-37 (19-50) cm-2 for muon neutrinos (muon antineutrinos), depending on the zenith angle of the event. In the other data sets, the combined fluence limits for both gravitational-wave events range from 2.4 ×104 to 7.0 ×109 cm-2
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Google™ Scholar:Abe, K. - Labarga Echeverría, Luis Alfonso - Fernandez, P. - The Super-Kamiokande Collaboration

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  • Producción científica en acceso abierto de la UAM [18079]

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