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The nEXO neutrinoless double beta decay experiment is designed to use a time projection chamber and 5000 kg of isotopically enriched liquid xenon to search for the decay in $^{136}$Xe. Progress in the detector design, paired with higher fidelity in its simulation and an advanced data analysis, based on the one used for the final results of EXO-200, produce a sensitivity prediction that exceeds the half-life of $10^{28}$ years. Specifically, improvements have been made in the understanding of production of scintillation photons and charge as well as of their transport and reconstruction in the detector. The more detailed knowledge of the detector construction has been paired with more assays for trace radioactivity in different materials. In particular, the use of custom electroformed copper is now incorporated in the design, leading to a substantial reduction in backgrounds from the intrinsic radioactivity of detector materials. Furthermore, a number of assumptions from previous sensitivity projections have gained further support from interim work validating the nEXO experiment concept. Together these improvements and updates suggest that the nEXO experiment will reach a half-life sensitivity of $1.35times 10^{28}$ yr at 90% CL in 10 years of data taking, covering the parameter space associated with the inverted neutrino mass ordering, along with a significant portion of the parameter space for the normal ordering scenario, for almost all nuclear matrix elements. The effects of backgrounds deviating from the nominal values used for the projections are also illustrated, concluding that the nEXO design is robust against a number of imperfections of the model.
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The next-generation Enriched Xenon Observatory (nEXO) is a proposed experiment to search for neutrinoless double beta ($0 ubetabeta$) decay in $^{136}$Xe with a target half-life sensitivity of approximately $10^{28}$ years using $5times10^3$ kg of isotopically enriched liquid-xenon in a time projection chamber. This improvement of two orders of magnitude in sensitivity over current limits is obtained by a significant increase of the $^{136}$Xe mass, the monolithic and homogeneous configuration of the active medium, and the multi-parameter measurements of the interactions enabled by the time projection chamber. The detector concept and anticipated performance are presented based upon demonstrated realizable background rates.
In the global landscape of neutrinoless double beta ($0 ubetabeta$) decay search, the use of semiconductor germanium detectors provides many advantages. The excellent energy resolution, the negligible intrinsic radioactive contamination, the possibility of enriching the crystals up to 88% in the $^{76}$Ge isotope as well as the high detection efficiency, are all key ingredients for highly sensitive $0 ubetabeta$ decay search. The MAJORANA and GERDA experiments successfully implemented the use of germanium (Ge) semiconductor detectors, reaching an energy resolution of $2.53 pm 0.08$ keV at the Q$_{betabeta}$ and an unprecedented low background level of $5.2 times 10^{-4}$ cts/(keV$cdot$kg$cdot$yr), respectively. In this paper, we will review the path of $0 ubetabeta$ decay search with Ge detectors from the original idea of E. Fiorini et al. in 1967, to the final recent results of the GERDA experiment setting a limit on the half-life of $^{76}$Ge $0 ubetabeta$ decay at $T_{1/2} > 1.8 times 10^{26}$ yr (90% C.L.). We will then present the LEGEND project designed to reach a sensitivity to the half-life up to $10^{28}$ yr and beyond, opening the way to the exploration of the normal ordering region.
The Gerda experiment designed to search for the neutrinoless double beta decay in 76Ge has successfully completed the first data collection. No signal excess is found, and a lower limit on the half life of the process is set, with T1/2 > 2.1x10^25 yr (90% CL). After a review of the experimental setup and of the main Phase I results, the hardware upgrade for Gerda Phase II is described, and the physics reach of the new data collection is reported.
Despite being the feeblest and lightest of the known particles, the neutrino is one of the most abundant particles in the Universe and has played a critical role in its evolution. Within standard cosmological models, most of the neutrinos were produced in the Big Bang and completely decoupled from matter after the first second. During that short time it is possible that through the process of Leptogenesis neutrinos helped to produce the matter/anti-matter asymmetry that sets the stage for all of the structures that we see in the universe today. However, these theories generally require the condition that the neutrino is a so-called Majorana particle, acting as its own anti-particle. The search for the extremely rare neutrinoless double-beta $(0 ubetabeta)$ decay is currently the most practical way to address this question. Here we present the results of the first tonne-year exposure search for $0 ubetabeta$ decay of $^{130}$Te with CUORE. With a median half-life exclusion sensitivity of $2.8times10^{25}$ yr, this is the most sensitive search for $0 ubetabeta$ decay in $^{130}$Te to date. We find no evidence for $0 ubetabeta$ decay and set a lower bound of $T_{1/2} > 2.2times10^{25}$ yr at a 90% credibility interval. CUORE is the largest, coldest solid-state detector operating below 100mK in the world. The achievement of 1 tonne-year of exposure demonstrates the long-term reliability and potential of cryogenic technology at this scale, with wide ranging applications to next-generation rare-event searches, dark matter searches, and even large-scale quantum computing.
Neutrinoless double-beta decay is a hypothesized process where in some even-even nuclei it might be possible for two neutrons to simultaneously decay into two protons and two electrons without emitting neutrinos. This is possible only if neutrinos are Majorana particles, i.e. fermions that are their own antiparticles. Neutrinos being Majorana particles would explicitly violate lepton number conservation, and might play a role in the matter-antimatter asymmetry in the universe. The observation of neutrinoless double-beta decay would also provide complementary information related to neutrino masses. The Majorana Collaboration is constructing the Majorana Demonstrator, a 40-kg modular germanium detector array, to search for the Neutrinoless double-beta decay of 76Ge and to demonstrate a background rate at or below 3 counts/(ROI-t-y) in the 4 keV region of interest (ROI) around the 2039 keV Q-value for 76Ge Neutrinoless double-beta decay. In this paper, we discuss the physics of neutrinoless double beta decay and then focus on the Majorana Demonstrator, including its design and approach to achieve ultra-low backgrounds and the status of the experiment.
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