We present global limits for Majorana neutrino masses by combining the latest results from neutrinoless double-beta ($0\nu \beta \beta$) decay searches and ab initio nuclear theory. Limits are derived in a Bayesian framework utilizing likelihood functions from a suite of $0\nu \beta \beta$-decay experiments in conjunction with nuclear matrix elements calculated from nuclear and electroweak forces derived from chiral effective field theory and implemented in the in-medium similarity renormalization group many-body approach. In contrast to nuclear models, ab initio results indicate that the current generation of $0\nu \beta \beta$-decay experiments have likely not yet reached sensitivities required to probe the mass regime allowed by neutrino-oscillation data, where the combined bounds are notably stronger than those given by individual experiments. Finally, from predicted sensitivities of next-generation searches, we show that, while no one individual experiment fully covers the inverted mass ordering, this can be achieved from combined contributions from the four key isotopes: ${}^{76}\mathrm{Ge}$, ${}^{100}\mathrm{Mo}$, ${}^{130}\mathrm{Te}$, and ${}^{136}\mathrm{Xe}$.

Close

PrevNext

View figure in article

• Beta decay
• Neutrinoless double beta decay
• Nuclear decay
• Nucleus-neutrino interactions
• Particle decays