Abstract

We study the effect of exotic charged current interactions on the electron energy spectrum in tritium decay, focussing on the KATRIN experiment and a possible modified setup that has access to the full spectrum. Both sub-eV and keV neutrino masses are considered. We perform a fully relativistic calculation and take all possible new interactions into account, demonstrating the possible sizable distortions in the energy spectrum.

Highlights

  • Provides an excellent opportunity to look for spectral distortions, which are characteristic for new mass states and for exotic interactions

  • Our analysis reaches beyond existing literature in the following points: (i) In our generic relativistic calculation we find that regardless of the interaction the energy spectrum can be parameterized by six functions which depend only on the involved particle masses and coupling constants, and whose precise form is specified by the interaction; (ii) we use an effective operator approach to study all possible Lorentz-invariant charged current interactions [3, 24] including right-handed sterile neutrinos; (iii) both small neutrino masses of order 0.5 eV and large masses of order keV are considered, and the significance of accessing the full electron energy spectrum is stressed

  • This allows in principle to improve the bounds on the effective operators and adds additional physics motivation to modifications of high activity neutrino mass experiments to study the full spectrum

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Summary

Fully relativistic treatment of beta decay

We consider the β-decay of a mother nucleus A to a daughter nucleus B, an electron e− and an electron antineutrino νe:. The final electron antineutrino state |νe is a superposition of mass eigenstates |νj. We will assume that apart from the three active neutrinos additional, necessarily sterile, neutrino species are present, i.e. where ns is the number of sterile neutrinos and U denotes the (3 + ns) × (3 + ns) lepton mixing matrix. We will work out general expressions for the electron energy spectrum, assuming only that the process in equation (2.1) is generated by an interaction that is mediated by particles much heavier than the nuclear scale. We make no assumption about the Lorentz structure of the interactions

Kinematics
Shape of the spectrum and corrections to the non-relativistic case
Kurie plots and the endpoint of the spectrum
Corrections from Standard Model physics
Effective operator approach
Neutrino mass and flavour eigenstates
The energy spectrum
Numerical analysis
Conclusions
Findings
B Boundaries of the Ej-integration

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