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Search for UHE neutrinos in coincidence with LIGO GW150914 event with the Pierre Auger Observatory

Published online by Cambridge University Press:  23 June 2017

Lili Yang  and
for the Pierre Auger Collaboration
Lili Yang
Affiliation:
Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
for the Pierre Auger Collaboration
Affiliation:
Observatorio Pierre Auger, Av. San Martin Norte 304, 5613 Malargue, Argentina (Full author list: http://www.auger.org/archive/authors_2016_06.html) email: Lili.Yang@ung.si
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Abstract

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The first gravitational wave transient GW150914 was observed by Advanced LIGO on September 14th, 2015 at 09:50:45 Universal Time. In addition to follow-up electromagnetic observations, the detection of neutrinos will probe deeply and more on the nature of astrophysical sources, especially in the ultra-high energy regime. Neutrinos in the EeV energy range were searched in data collected at the surface detector of the Pierre Auger Observatory within ± 500 s and 1 day after the GW150914 event. No neutrino candidates were found. Based on this non-observation, we derive the first and only neutrino fluence upper limit at EeV energies for this event at 90% CL, and report constraints on existence of accretion disk around mergers.

Keywords

gravitational wavesneutrinosblack hole physics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S324: New Frontiers in Black Hole Astrophysics , September 2016 , pp. 295 - 298
Copyright
Copyright © International Astronomical Union 2017 

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