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The galactic contribution to IceCube's astrophysical neutrino flux

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1];  [2];  [3]
  1. Univ. of Copenhagen (Denmark). The Niels Bohr Inst.; UH High Energy Physics Group
  2. Univ. of Hawaii at Manoa, Honolulu, HI (United States)
  3. 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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Cited By (22)

The Bright and Choked Gamma-Ray Burst Contribution to the IceCube and ANTARES Low-Energy Excess text January 2018
Fundamental Physics with High-Energy Cosmic Neutrinos text January 2019
Astrophysics Uniquely Enabled by Observations of High-Energy Cosmic Neutrinos text January 2019
Neutrino Non-Standard Interactions: A Status Report text January 2019
Testing Lorentz Invariance with Neutrinos preprint January 2022
Interactions of astrophysical neutrinos with dark matter: a model building perspective journal January 2019
A multi-component model for observed astrophysical neutrinos journal July 2018
A combined astrophysical and dark matter interpretation of the IceCube HESE and throughgoing muon events journal July 2018
A multi-messenger study of the total galactic high-energy neutrino emission journal August 2018
Comprehensive approach to tau-lepton production by high-energy tau neutrinos propagating through the Earth journal January 2018
Constraints on inflation with an extended neutrino sector journal April 2019
Invisible Neutrino Decay Could Resolve IceCube’s Track and Cascade Tension journal September 2018
Extracting the Energy-Dependent Neutrino-Nucleon Cross Section above 10 TeV Using IceCube Showers journal January 2019
Inferring the Flavor of High-Energy Astrophysical Neutrinos at Their Sources journal June 2019
Neutrino non-standard interactions: A status report journal January 2019
A multi-component model for observed astrophysical neutrinos text January 2018
A multi-component model for observed astrophysical neutrinos text January 2018
Exploring the Properties of Choked Gamma-ray Bursts with IceCube’s High-energy Neutrinos journal March 2018
A multi-messenger study of the total galactic high-energy neutrino emission text January 2017
Exploring the Properties of Choked Gamma-Ray Bursts with IceCube's High Energy Neutrinos text January 2017
A Multi-Component Model for the Observed Astrophysical Neutrinos text January 2018
Interactions of Astrophysical Neutrinos with Dark Matter: A model building perspective text January 2018

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