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Title: Two-component flux explanation for the high energy neutrino events at IceCube

Journal Article · · Physical Review. D, Particles, Fields, Gravitation and Cosmology
 [1];  [2];  [1]
  1. Brookhaven National Lab. (BNL), Upton, NY (United States). Dept. of Physics
  2. Univ. of Manchester (United Kingdom). Consortium for Fundamental Physics

In understanding the spectral and flavor composition of the astrophysical neutrino flux responsible for the recently observed ultrahigh-energy events at IceCube we see how important both astrophysics and particle physics are. Here, we perform a statistical likelihood analysis to the three-year IceCube data and derive the allowed range of the spectral index and flux normalization for various well-motivated physical flavor compositions at the source. While most of the existing analyses so far assume the flavor composition of the neutrinos at an astrophysical source to be (1:2:0), it seems rather unnatural to assume only one type of source, once we recognize the possibility of at least two physical sources. Bearing this in mind, we entertain the possibility of a two-component source for the analysis of IceCube data. It appears that our two-component hypothesis explains some key features of the data better than a single-component scenario; i.e. it addresses the apparent energy gap between 400 TeV and about 1 PeV and easily accommodates the observed track-to-shower ratio. Given the extreme importance of the flavor composition for the correct interpretation of the underlying astrophysical processes as well as for the ramification for particle physics, this two-component flux should be tested as more data is accumulated.

Research Organization:
Brookhaven National Laboratory (BNL), Upton, NY (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
SC0012704; AC02-98CH10886
OSTI ID:
1412635
Alternate ID(s):
OSTI ID: 1222515
Report Number(s):
BNL-113788-2017-JA; PRVDAQ; KA2401012; TRN: US1800307
Journal Information:
Physical Review. D, Particles, Fields, Gravitation and Cosmology, Vol. 92, Issue 7; ISSN 1550-7998
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 60 works
Citation information provided by
Web of Science

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Cited By (22)

A multi-component model for observed astrophysical neutrinos journal July 2018
Heavy right-handed neutrino dark matter and PeV neutrinos at IceCube journal August 2016
On the IceCube spectral anomaly journal December 2016
A combined astrophysical and dark matter interpretation of the IceCube HESE and throughgoing muon events journal July 2018
Neutrinophilic Dark Matter in the epoch of IceCube and Fermi-LAT journal December 2018
Multi-PeV Signals from a New Astrophysical Neutrino Flux beyond the Glashow Resonance journal June 2018
The flavor composition of astrophysical neutrinos after 8 years of IceCube: an indication of neutron decay scenario? journal June 2019
Neutrino Telescopes and High-Energy Cosmic Neutrinos text January 2020
A multi-component model for observed astrophysical neutrinos text January 2018
The flavor composition of astrophysical neutrinos after 8 years of IceCube: an indication of neutron decay scenario? text January 2019
Astrophysical neutrinos flavored with Beyond the Standard Model physics text January 2017
Neutrino Telescopes and High-Energy Cosmic Neutrinos journal February 2020
A multi-component model for observed astrophysical neutrinos text January 2018
Astrophysical neutrinos flavored with beyond the Standard Model physics text January 2017
Galactic Neutrinos in the TeV to PeV Range text January 2015
Hidden Cosmic-Ray Accelerators as an Origin of TeV-PeV Cosmic Neutrinos text January 2015
Heavy right-handed neutrino dark matter and PeV neutrinos at IceCube text January 2016
On the IceCube spectral anomaly text January 2016
Astrophysical neutrinos flavored with Beyond the Standard Model physics text January 2017
A Multi-Component Model for the Observed Astrophysical Neutrinos text January 2018
Neutrinophilic Dark Matter in the epoch of IceCube and Fermi-LAT text January 2018
Neutrino telescopes and high-energy cosmic neutrinos text January 2020

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