Ultra-High Energy Astrophysical Neutrino Detection, and the Search for Lorentz Invariance Violations

A growing class of ultra-high energy neutrino (UHE-nu) observatories based on the Askaryan effect and Antarctic ice is able to search for Lorentz invariance violation (LIV). The ARA, ARIANNA, ANITA and EVA collaborations have the power to constrain the Standard Model Extension (SME) by measuring the...

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Bibliographic Details
Main Author: Hanson, J. C.
Format: Report
Language:unknown
Published: arXiv 2016
Subjects:
High Energy Astrophysical Phenomena astro-ph.HE
High Energy Physics - Phenomenology hep-ph
FOS Physical sciences
Antarctic
South Pole
Antarc*
South pole
Online Access:https://dx.doi.org/10.48550/arxiv.1607.05745
https://arxiv.org/abs/1607.05745
Description
Summary:A growing class of ultra-high energy neutrino (UHE-nu) observatories based on the Askaryan effect and Antarctic ice is able to search for Lorentz invariance violation (LIV). The ARA, ARIANNA, ANITA and EVA collaborations have the power to constrain the Standard Model Extension (SME) by measuring the flux and energy distribution of neutrinos created through the GZK process. The future expansion of ARA, at the South Pole, pushes the discovery potential further. : Presented at the Seventh Meeting on CPT and Lorentz Symmetry, Bloomington, Indiana, June 20-24, 2016

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