# Cosmic tau neutrino detection via Cherenkov signals from air showers from Earth-emerging taus

## TL;DR

This paper models Earth-emerging tau neutrinos and their air shower signals to evaluate the sensitivity of space-based detectors like POEMMA for high-energy neutrino detection above 10 PeV.

## Contribution

It provides a detailed flux and spectrum calculation of Earth-emerging tau leptons using a layered Earth model and assesses detector sensitivity considering systematic uncertainties.

## Key findings

- Quantifies systematic uncertainties from cross sections and energy loss models.
- Estimates neutrino sensitivity for space-based detectors above 10 PeV.
- Simulates Cherenkov signals from tau-induced air showers.

## Abstract

We perform a new, detailed calculation of the flux and energy spectrum of Earth-emerging $\tau$-leptons generated from the interactions of tau neutrinos and antineutrinos in the Earth. A layered model of the Earth is used to describe the variable density profile of the Earth. Different assumptions regarding the neutrino charged- and neutral-current cross sections as well as the $\tau$-lepton energy loss models are used to quantify the systematic uncertainty from these on the results. A baseline simulation is then used to generate the optical Cherenkov signal from upward-moving extensive air showers generated by the $\tau$-lepton decay in the atmosphere, applicable to a range of space-based instruments. We use this simulation to determine the neutrino sensitivity for $E_\nu>$ 10 PeV for a space-based experiment with performance similar to that for the Probe of Extreme MultiMessenger Astrophysics (POEMMA) mission currently under study.