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Belley, Antoine

University of British Columbia

Exotic weak decays offer a unique way to probe physics beyond the Standard Model in a low-energy regime using the atomic nucleus as a window to complement the high-energy searches done at particle accelerator facilities. However, in order to extract the relevant physics parameters from experimental observations, inputs from nuclear theory are required. The hypothetical neutrinoless double-beta decay has gathered a lot of interest, as its observation would answer many outstanding questions in particle physics. First, it would unveil fundamental properties of the most abundant, yet most elusive, massive particle: the neutrino. A simple observation of this decay would imply the neutrino to be Majorana, meaning that it is its own antiparticle, as well as give insight into its absolute mass. Furthermore, the existence of this decay would explain the matter/antimatter asymmetry of the universe. In order to extract the neutrino mass and potential couplings to more exotic mechanisms, as well as compare sensitivities of experiments using different isotopes, the nuclear matrix element must be obtained from nuclear theory. Unfortunately, the different models that have historically been used to compute this quantity have shown a large spread, with no means of quantifying their respective uncertainties, greatly hindering the experimental precision. In this thesis, we use recent advances in ab initio methods, which profit from the rapid increase in computational power, to calculate nuclear observables directly from the interaction between the nucleons. In particular, we use the ab initio valence-space in-medium similarity renormalization group method to compute the matrix element of all relevant candidate isotopes for experimental searches. We further develop a new machine learning emulator that greatly increases the speed of calculations. Using this emulator, we probe the full input parameter space of the calculation to give the first statistical uncertainty on the matrix element. Our results show smaller values than previous models and are consistent with other ab initio methods. This provides a much tighter constraint than the spread coming from previous models, greatly clarifying the picture for both current and future experimental searches of the decay.

Text

2024-08-22

Attribution-NonCommercial-NoDerivatives 4.0 International

http://hdl.handle.net/2429/88996

Physics

University of British Columbia

UBCV

http://creativecommons.org/licenses/by-nc-nd/4.0/