Cosmic neutrino background detection in large-neutrino-mass cosmologies

Abstract

The cosmic neutrino background (CNB) is a definite prediction of the standard cosmological model and its direct discovery would represent a milestone in cosmology and neutrino physics. In this work, we consider the capture of relic neutrinos on a tritium target as a possible way to detect the CNB, as aimed for by the PTOLEMY project. Crucial parameters for this measurement are the absolute neutrino mass ${m}_{\ensuremath{\nu}}$ and the local neutrino number density ${n}_{\ensuremath{\nu}}^{\mathrm{loc}}$. Within the $\mathrm{\ensuremath{\Lambda}}\mathrm{CDM}$ model, cosmology provides a stringent upper limit on the sum of neutrino masses of $\ensuremath{\sum}{m}_{\ensuremath{\nu}}<0.12\text{ }\text{ }\mathrm{eV}$, with further improvements expected soon from galaxy surveys by DESI and EUCLID. This makes the prospects for a CNB detection and a neutrino mass measurement in the laboratory very difficult. In this context, we consider a set of nonstandard cosmological models that allow for large neutrino masses (${m}_{\ensuremath{\nu}}\ensuremath{\sim}1\text{ }\text{ }\mathrm{eV}$), potentially in reach of the KATRIN neutrino mass experiment or upcoming neutrinoless double-beta decay searches. We show that the CNB detection prospects could be much higher in some of these models compared to those in $\mathrm{\ensuremath{\Lambda}}\mathrm{CDM}$, and discuss the potential for such a detection to discriminate between cosmological scenarios. Moreover, we provide a simple rule to estimate the required values of energy resolution, exposure, and background rate for a PTOLEMY-like experiment to cover a certain region in the $({m}_{\ensuremath{\nu}},{n}_{\ensuremath{\nu}}^{\mathrm{loc}})$ parameter space. Alongside this paper, we publicly release a code to calculate the CNB sensitivity in a given cosmological model.