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  2. Proton decay - Wikipedia

    en.wikipedia.org/wiki/Proton_decay

    In particle physics, proton decay is a hypothetical form of particle decay in which the proton decays into lighter subatomic particles, such as a neutral pion and a positron. [1] The proton decay hypothesis was first formulated by Andrei Sakharov in 1967. Despite significant experimental effort, proton decay has never been observed.

  3. List of unsolved problems in physics - Wikipedia

    en.wikipedia.org/wiki/List_of_unsolved_problems...

    b →J/ψK − p channel, which represents the decay of the bottom lambda baryon (Λ 0 b) into a J/ψ meson (J/ψ), a kaon (K −) and a proton (p). The results showed that sometimes, instead of decaying directly into mesons and baryons, the Λ 0 b decayed via intermediate pentaquark states. The two states, named P + c (4380) and P +

  4. Kamioka Observatory - Wikipedia

    en.wikipedia.org/wiki/Kamioka_Observatory

    The first of the Kamioka experiments was named KamiokaNDE for Kamioka Nucleon Decay Experiment. It was a large water Čerenkov detector designed to search for proton decay. To observe the decay of a particle with a lifetime as long as a proton an experiment must run for a long time and observe an enormous number of protons. This can be done ...

  5. Irvine–Michigan–Brookhaven (detector) - Wikipedia

    en.wikipedia.org/wiki/Irvine–Michigan...

    IMB detected fast-moving particles such as those produced by proton decay or neutrino interactions by picking up the Cherenkov radiation generated when such a particle moves faster than light's speed in water. Since directional information was available from the phototubes, IMB was able to estimate the initial direction of neutrinos.

  6. Soudan 2 - Wikipedia

    en.wikipedia.org/wiki/Soudan_2

    Soudan 2 was the successor to the Soudan 1, a similar 30 ton detector also intended to search for proton decay. [2] The excavation for Soudan 2 was done in 1984–1985. Installation was started in 1986 and was completed in 1993. The experiment was run from April 1989 to June 2001, beginning with a partial detector of 275 tons. [3]

  7. Proton emission - Wikipedia

    en.wikipedia.org/wiki/Proton_emission

    Proton emission (also known as proton radioactivity) is a rare type of radioactive decay in which a proton is ejected from a nucleus.Proton emission can occur from high-lying excited states in a nucleus following a beta decay, in which case the process is known as beta-delayed proton emission, or can occur from the ground state (or a low-lying isomer) of very proton-rich nuclei, in which case ...

  8. Baryon asymmetry - Wikipedia

    en.wikipedia.org/wiki/Baryon_asymmetry

    However, the Standard Model is known to violate the conservation of baryon number only non-perturbatively: a global U(1) anomaly. To account for baryon violation in baryogenesis, such events (including proton decay) can occur in Grand Unification Theories (GUTs) and supersymmetric (SUSY) models via hypothetical massive bosons such as the X boson.

  9. Future of an expanding universe - Wikipedia

    en.wikipedia.org/wiki/Future_of_an_expanding...

    See § Future without proton decay below. Shorter or longer proton half-lives will accelerate or decelerate the process. This means that after 10 40 years (the maximum proton half-life used by Adams & Laughlin (1997)), one-half of all baryonic matter will have been converted into gamma ray photons and leptons through proton decay.