# Relic neutrino detection through angular correlations in inverse $\beta$-decay

## TL;DR

This paper proposes a novel method to detect cosmic background neutrinos by observing periodic angular correlation variations in inverse beta decay, which does not require extremely high energy resolution.

## Contribution

It introduces an alternative detection approach based on angular correlation variations caused by Earth's and Sun's motion, reducing dependence on energy resolution.

## Key findings

- Angular correlations vary periodically due to Earth's and Sun's motion.
- Method can work even with energy resolution exceeding neutrino mass.
- Potential for detection without ultra-high energy resolution.

## Abstract

Neutrino capture on beta-decaying nuclei is currently the only known potentially viable method of detection of cosmic background neutrinos. It is based on the idea of separation of the spectra of electrons or positrons produced in captures of relic neutrinos on unstable nuclei from those from the usual $\beta$-decay and requires very high energy resolution of the detector, comparable to the neutrino mass. In this paper we suggest an alternative method of discrimination between neutrino capture and $\beta$-decay, based on periodic variations of angular correlations in inverse beta decay transitions induced by relic neutrino capture. The time variations are expected to arise due to the peculiar motion of the Sun with respect to the C$\nu$B rest frame and the rotation of the Earth about its axis and can be observed in experiments with both polarized and unpolarized nuclear targets. The main advantage of the suggested method is that it does not depend crucially on the energy resolution of detection of the produced $\beta$-particles and can be operative even if this resolution exceeds the largest neutrino mass.