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Visible decay of astrophysical neutrinos at IceCube

Abdullahi, Asli; Denton, Peter B.

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Authors

Profile image of Asli Abdullahi

Asli Abdullahi asli.abdullahi@durham.ac.uk
PGR Student Doctor of Philosophy

Peter B. Denton



Abstract

Neutrino decay modifies neutrino propagation in a unique way; not only is there flavor changing as there is in neutrino oscillations, there is also energy transport from initial to final neutrinos. The most sensitive direct probe of neutrino decay is currently IceCube which can measure the energy and flavor of neutrinos traveling over extragalactic distances. For the first time, we calculate the flavor transition probability for the cases of visible and invisible neutrino decay, including the effects of the expansion of the Universe, and consider the implications for IceCube. As an example, we demonstrate how neutrino decay addresses a tension in the IceCube data.

Citation

Abdullahi, A., & Denton, P. B. (2020). Visible decay of astrophysical neutrinos at IceCube. Physical Review D, 102(2), Article 023018. https://doi.org/10.1103/physrevd.102.023018

Journal Article Type Article
Acceptance Date Jul 1, 2020
Online Publication Date Jul 14, 2020
Publication Date 2020-07
Deposit Date Jul 17, 2020
Publicly Available Date Jul 17, 2020
Journal Physical Review D
Print ISSN 2470-0010
Electronic ISSN 2470-0029
Publisher American Physical Society
Peer Reviewed Peer Reviewed
Volume 102
Issue 2
Article Number 023018
DOI https://doi.org/10.1103/physrevd.102.023018
Public URL https://durham-repository.worktribe.com/output/1266329

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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.






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