On the Tau flavor of the cosmic neutrino flux

TL;DR

This paper explores how tau neutrino flux measurements can reveal new physics beyond the Standard Model, especially interactions with ultralight dark matter, and analyzes the implications of anomalous events observed by ANITA and IceCube.

Contribution

It demonstrates the importance of tau neutrino detection in probing beyond SM physics, clarifies misconceptions about neutrino evolution in the 3+1 scheme, and links dark matter interactions to high-energy neutrino observations.

Findings

Tau flavor is crucial for understanding new physics.

Existing bounds exclude the 3+1 scheme as an explanation for ANITA events.

Interactions with ultralight dark matter can reconcile observations with theoretical models.

Abstract

Observation of high energy cosmic neutrinos by ICECUBE has ushered in a new era in exploring both cosmos and new physics beyond the Standard Model (SM). In the standard picture, although mostly $\nu_\mu$ and $\nu_e$ are produced in the source, oscillation will produce $\nu_\tau$ {\it en route}. Certain beyond SM scenarios, like interaction with ultralight DM can alter this picture. Thus, the flavor composition of the cosmic neutrino flux can open up the possibility of exploring certain beyond the SM scenarios that are inaccessible otherwise. We show that the $\tau$ flavor holds a special place among the neutrino flavors in elucidating new physics. Interpreting the two anomalous events observed by ANITA as $\nu_\tau$ events makes the tau flavor even more intriguing. We study how the detection of the two tau events by ICECUBE constrains the interaction of the neutrinos with ultralight dark matter and discuss the implications of this interaction for even higher energy cosmic neutrinos detectable by future radio telescopes such as ARA, ARIANNA and GRAND. We also revisit the $3+1$ neutrino scheme as a solution to the two anomalous ANITA events and clarify a misconception that exists in the literature about the evolution of high energy neutrinos in matter within the $3+1$ scheme with a possibility of scattering off nuclei. We show that the existing bounds on the flux of $\nu_\tau$ with energy of EeV rules out this solution for the ANITA events. We show that the $3+1$ solution can be saved from both this bound and from the bound on the extra relativistic degrees of freedom in the early universe by turning on the interaction of neutrinos with ultralight dark matter.