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

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.

24 pages, 1 figure. v2: title changed, section 4 modified, Appendix B added, references added. v3: section 4 slightly expanded; eq. (B.7) corrected. Final version to be published in JCAP

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Cited by in corpus (7)

• Grand Unified Neutrino Spectrum at Earth: Sources and Spectral Components
• Limits on the cosmic neutrino background
• Empirical capture cross sections for cosmic neutrino detection with ${}^{151}\mathbf{Sm}$ and ${}^{171}\mathbf{Tm}$
• Multi-Messenger Astrophysics with the Cosmic Neutrino Background
• Status and Perspectives of Neutrino Physics
• Cosmic neutrino background detection in the minimally extended Standard Model
• Numerical treatment of annual modulation of relic neutrinos