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  4. Lorentz invariance violation and IceCube neutrino events
 
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Lorentz invariance violation and IceCube neutrino events

Source
Journal of High Energy Physics
ISSN
11266708
Date Issued
2015-11-01
Author(s)
Tomar, Gaurav
Mohanty, Subhendra
Pakvasa, Sandip
DOI
10.1007/JHEP11(2015)022
Volume
2015
Issue
11
Abstract
Abstract: The IceCube neutrino spectrum shows a flux which falls of as E<sup>−2</sup> for sub PeV energies but there are no neutrino events observed above ∼ 3 PeV. In particular the Glashow resonance expected at 6.3 PeV is not seen. We examine a Planck scale Lorentz violation as a mechanism for explaining the cutoff of observed neutrino energies around a few PeV. By choosing the one free parameter the cutoff in neutrino energy can be chosen to be between 2 and 6.3 PeV. We assume that neutrinos (antineutrinos) have a dispersion relation E<sup>2</sup> = p<sup>2</sup> − (ξ<inf>3</inf>/M<inf>Pl</inf>) p<sup>3</sup>, and find that both π<sup>+</sup> and π<sup>−</sup> decays are suppressed at neutrino energies of order of few PeV. We find that the μ<sup>−</sup> decay being a two-neutrino process is enhanced, whereas μ<sup>+</sup> decay is suppressed. The K<sup>+</sup> → π<sup>0</sup>e<sup>+</sup>ν<inf>e</inf> is also suppressed with a cutoff neutrino energy of same order of magnitude, whereas K−→π0e−ν¯e$$ {K}^{-}\to {\pi}^0{e}^{-}{\overline{\nu}}_e $$ is enhanced. The n→p+e−ν¯e$$ n\to {p}^{+}{e}^{-}{\overline{\nu}}_e $$ decay is suppressed (while the n¯→p−e+νe$$ \overline{n}\to {p}^{-}{e}^{+}{\nu}_e $$ is enhanced). This means that the ν¯e$$ {\overline{\nu}}_e $$ expected from n decay arising from p + γ → Δ → π<sup>+</sup>n reaction will not be seen. This can explain the lack of Glashow resonance events at IceCube. If no Glashow resonance events are seen in the future then the Lorentz violation can be a viable explanation for the IceCube observations at PeV energies.
Publication link
https://link.springer.com/content/pdf/10.1007%2FJHEP11%282015%29022.pdf
URI
https://d8.irins.org/handle/IITG2025/21396
Subjects
Beyond Standard Model | Cosmology of Theories beyond the SM | Neutrino Physics
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