Proton decay

Proton decay is the key process to test the stability of matter and baryon number conservation and has long been a subject of both theoretical and experimental interests. Violation of baryon number conservation is one of the three key ingredients to explain the asymmetry of matter and antimatter in the Universe, as first formulated by Andrei Sakharov in 1967. Despite significant experimental effort, proton decay has never been observed. The current experimental lower bound on the proton lifetime ( τ p {\displaystyle \tau _{p}} ) is 2.4×1034 years (in the decay channel into a positron and a neutral pion: p → e+ + π0). According to the Standard Model, the proton, a type of baryon, is stable because baryon number is conserved. Since protons are the lightest baryons in the model, they cannot decay into other particles on their own and are therefore stable. However, baryon number conservation is an accidental global symmetry of the Standard Model, not associated with any fundamental gauge symmetry, slightly violated by non-perturbative SU(2)L sphaleron effects, negligible at low temperatures but relevant in the early Universe. Positron emission and electron capture—forms of radioactive decay in which a proton becomes a neutron—are not proton decay, because in these processes the proton interacts with other particles within the atom. Grand Unified Theories (GUTs) explicitly break the baryon number symmetry, allowing protons to decay via the Higgs particle, magnetic monopoles, or new X bosons with a half-life in the range 1031 to 1036 years. For comparison, the universe is roughly 1.4×1010 (14 billion) years old, which is at least twenty orders of magnitude lower. Although at first glance it may seem nearly impossible to explore such long lifetimes, it is sufficient to monitor 1034 protons per year (with efficiency = 1) to be sensitive to average lifetimes of...