The galactic contribution to IceCube's astrophysical neutrino flux
Journal Article
·
· Journal of Cosmology and Astroparticle Physics
- Univ. of Copenhagen (Denmark). The Niels Bohr Inst.; UH High Energy Physics Group
- Univ. of Hawaii at Manoa, Honolulu, HI (United States)
- Vanderbilt Univ., Nashville, TN (United States)
High energy neutrinos have been detected by IceCube, but their origin remains a mystery. Determining the sources of this flux is a crucial first step towards multi-messenger studies. Here, we systematically compare two classes of sources with the data: Galactic and extragalactic. We assume that the neutrino sources are distributed according to a class of Galactic models. We build a likelihood function on an event by event basis including energy, event topology, absorption, and direction information. We present the probability that each high energy event with deposited energy Edep>60 TeV in the HESE sample is Galactic, extragalactic, or background. Lastly, for Galactic models considered the Galactic fraction of the astrophysical flux has a best fit value of 1.3% and is <9.5% at 90\% CL. A zero Galactic flux is allowed at <1σ.
- Research Organization:
- Univ. of Hawaii, Honolulu, HI (United States)
- Sponsoring Organization:
- Danish National Research Foundation; USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
- Grant/Contract Number:
- SC0010504; SC0011981
- OSTI ID:
- 1598576
- Alternate ID(s):
- OSTI ID: 1535569
OSTI ID: 22676046
- Journal Information:
- Journal of Cosmology and Astroparticle Physics, Journal Name: Journal of Cosmology and Astroparticle Physics Journal Issue: 08 Vol. 2017; ISSN 1475-7516
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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