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Tau depolarization at very high energies for neutrino telescopes
Journal article   Open access   Peer reviewed

Tau depolarization at very high energies for neutrino telescopes

Carlos A. Arguelles, Diksha Garg, Sameer Patel, Mary Hall Reno and Ibrahim Safa
Physical review. D, Vol.106(4), 043008
08/08/2022
DOI: 10.1103/PhysRevD.106.043008
url
https://doi.org/10.1103/PhysRevD.106.043008View
Published (Version of record) Open Access

Abstract

The neutrino interaction length scales with energy, and becomes comparable to Earth's diameter above 10's of TeV energies. Over terrestrial distances, the tau's short lifetime leads to an energetic regenerated tau neutrino flux, nu(tau )-> tau -> nu(tau), within the Earth. The next generation of neutrino experiments aim to detect ultrahigh energy neutrinos. Many of them rely on detecting either the regenerated tau neutrino, or a tau decay shower. Both of these signatures can be affected by the polarization of the tau through the energy distribution of the secondary particles produced from the tau's decay. While taus produced in weak interactions are nearly 100% polarized, it is expected that taus experience some depolarization due to electromagnetic interactions in the Earth. In this paper, for the first time we quantify the depolarization of taus in electromagnetic energy loss. We find that tau depolarization has only small effects on the final energy of tau neutrinos or taus produced by high energy tau neutrinos incident on the Earth. Tau depolarization can be directly implemented in Monte Carlo simulations such as nuPyProp and TauRunner.
Physical Sciences Physics Astronomy & Astrophysics Physics, Particles & Fields Science & Technology

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