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Constraints on Minute-Scale Transient Astrophysical Neutrino Sources
Journal article   Open access   Peer reviewed

Constraints on Minute-Scale Transient Astrophysical Neutrino Sources

Maryon Ahrens, Christian Bohm, Kunal Deoskar, Jonathan P. Dumm, Chad Finley, Klas Hultqvist, Erin O'Sullivan and Christian Walck
Physical review letters, v 122(5), pp 051102-051102
2019
PMID: 30822017
url
https://doi.org/10.1103/physrevlett.122.051102View
Accepted (AM)Open Access (Publisher-Specific) Open
url
https://doi.org/10.1103/PhysRevLett.122.051102View
Published, Version of Record (VoR) Open

Abstract

Fysik Naturvetenskap Natural Sciences Physical Sciences
High-energy neutrino emission has been predicted for several short-lived astrophysical transients including gamma-ray bursts (GRBs), core-collapse supernovae with choked jets, and neutron star mergers. IceCube's optical and x-ray follow-up program searches for such transient sources by looking for two or more muon neutrino candidates in directional coincidence and arriving within 100 s. The measured rate of neutrino alerts is consistent with the expected rate of chance coincidences of atmospheric background events and no likely electromagnetic counterparts have been identified in Swift follow-up observations. Here, we calculate generic bounds on the neutrino flux of short-lived transient sources. Assuming an E-2.5 neutrino spectrum, we find that the neutrino flux of rare sources, like long gamma-ray bursts, is constrained to < 5% of the detected astrophysical flux and the energy released in neutrinos (100 GeV to 10 PeV) by a median bright GRB-like source is < 10(52.5) erg. For a harder E-2.13 neutrino spectrum up to 30% of the flux could be produced by GRBs and the allowed median source energy is < 10(52) erg. A hypothetical population of transient sources has to be more common than 10(-5) Mpc(-3) yr(-1) (5 x 10(-8) Mpc(-3) yr(-1) for the E-2.13 spectrum) to account for the complete astrophysical neutrino flux.

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Collaboration types
Domestic collaboration
International collaboration
Web of Science research areas
Physics, Multidisciplinary
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