Abstract

Compelling experimental evidences of neutrino oscillations and their implication that neutrinos are massive particles have given neutrinoless double beta decay a central role in astroparticle physics. In fact, the discovery of this elusive decay would be a major breakthrough, unveiling that neutrino and antineutrino are the same particle and that the lepton number is not conserved. It would also impact our efforts to establish the absolute neutrino mass scale and, ultimately, understand elementary particle interaction unification. All current experimental programs to search for neutrinoless double beta decay are facing with the technical and financial challenge of increasing the experimental mass while maintaining incredibly low levels of spurious background. The new concept described in this paper could be the answer which combines all the features of an ideal experiment: energy resolution, low cost mass scalability, isotope choice flexibility and many powerful handles to make the background negligible. The proposed technology is based on the use of arrays of silicon detectors cooled to 120 K to optimize the collection of the scintillation light emitted by ultra-pure crystals. It is shown that with a 54 kg array of natural CaMoO4 scintillation detectors of this type it is possible to yield a competitive sensitivity on the half-life of the neutrinoless double beta decay of 100Mo as high as ~10E24 years in only one year of data taking. The same array made of 40CaMoO4 scintillation detectors (to get rid of the continuous background coming from the two neutrino double beta decay of 48Ca) will instead be capable of achieving the remarkable sensitivity of ~10E25 years on the half-life of 100Mo neutrinoless double beta decay in only one year of measurement.

Highlights

  • Neutrinoless double beta decay is an extremely rare phenomenon hypothesized long time ago but never observed

  • We show that with a small array (∼54 kg) of such detectors it is possible to yield in only 1 year of measurement a competitive physics result in the search for the neutrinoless double beta decay of 100Mo using natural CaMoO4 scintillating crystals

  • Preliminary Monte Carlo simulations – which do not include the optical photon propagation yet – showed that among the γ interactions of initial energy equal to 3 MeV depositing the whole energy in a single CaMoO4 crystal, only 30 % would be labelled as single-site event if the threshold distance for distinguishing a multiple-site interaction is set equal to 10 mm; this fraction becomes as low as 14 % if the minimum detectable inter-site distance is 5 mm

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Summary

Introduction

Neutrinoless double beta decay is an extremely rare phenomenon hypothesized long time ago but never observed. This justifies the large number of experimental programs devoted to the search of this decay with different techniques. We show that with a small array (∼54 kg) of such detectors it is possible to yield in only 1 year of measurement a competitive physics result in the search for the neutrinoless double beta decay of 100Mo using natural CaMoO4 scintillating crystals (i.e. without enriching in 100Mo or depleting in 48Ca isotopes). This result would pave the way to a new class of ton scale experiments to search for neutrinoless double beta decay with potentially zero background, and for dark matter and neutrino charged current reactions

Neutrinoless double beta decay
Background reduction
The benefit of scintillation detectors
The measurement technique
Silicon drift detectors as photodetectors
Scintillating crystal choice
Expected detector performance
Background source
Other physics measurements with CaMoO4
Findings
Conclusions
Full Text
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