New limits on neutrino decay from the Glashow resonance of high-energy cosmic neutrinos

Abstract

Discovering neutrino decay would be strong evidence of physics beyond the Standard Model. Presently, there are only lax lower limits on the lifetime $\tau$ of neutrinos, of $\tau /m\sim 10^{-3}$ s eV${}^{-1}$ or worse, where $m$ is the unknown neutrino mass. High-energy cosmic neutrinos, with TeV-PeV energies, offer superior sensitivity to decay due to their cosmological-scale baselines. To tap into it, we employ a promising method, recently proposed, that uses the Glashow resonance ${\bar{\nu }}_e+e\to W$, triggered by ${\bar{\nu }}_e$ of 6.3 PeV, to test decay with only a handful of detected events. If most of the ${\nu }_1$ and ${\nu }_2$ decay into ${\nu }_3$ en route to Earth, no Glashow resonance would occur in neutrino telescopes, because the remaining ${\nu }_3$ have only a tiny electron-flavor content. We turn this around and use the recent first detection of a Glashow resonance candidate in IceCube to place new lower limits on the lifetimes of ${\nu }_1$ and ${\nu }_2$. For ${\nu }_2$, our limit is the current best. For ${\nu }_1$, our limit is close to the current best and, with the imminent detection of a second Glashow resonance, will vastly surpass it.

Comments: 5 pages, 2 figures, technical appendices