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  2. Proton decay - Wikipedia

    en.wikipedia.org/wiki/Proton_decay

    Free neutrons—those not inside an atomic nucleus—are already known to decay into protons (and an electron and an antineutrino) in a process called beta decay. Free neutrons have a half-life of 10 minutes (610.2 ± 0.8 s) [17] due to the weak interaction. Neutrons bound inside a nucleus have an immensely longer half-life – apparently as ...

  3. Help:Download as PDF - Wikipedia

    en.wikipedia.org/wiki/Help:Download_as_PDF

    In the Print/export section select Download as PDF. The rendering engine starts and a dialog appears to show the rendering progress. When rendering is complete, the dialog shows "The document file has been generated. Download the file to your computer." Click the download link to open the PDF in your selected PDF viewer.

  4. Free neutron decay - Wikipedia

    en.wikipedia.org/wiki/Free_neutron_decay

    In this type of free neutron decay, in essence all of the neutron decay energy is carried off by the antineutrino (the other "body"). The reverse process of recombination of a proton and an electron into a neutron and a neutrino by electron capture occurs in neutron stars, under the conditions of neutron degeneracy.

  5. 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 ...

  6. Particle decay - Wikipedia

    en.wikipedia.org/wiki/Particle_decay

    In particle physics, particle decay is the spontaneous process of one unstable subatomic particle transforming into multiple other particles. The particles created in this process (the final state ) must each be less massive than the original, although the total mass of the system must be conserved.

  7. 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.

  8. Internal conversion - Wikipedia

    en.wikipedia.org/wiki/Internal_conversion

    Internal conversion is an atomic decay process where an excited nucleus interacts electromagnetically with one of the orbital electrons of an atom. This causes the electron to be emitted (ejected) from the atom. [1] [2] Thus, in internal conversion (often abbreviated IC), a high-energy electron is emitted from the excited atom, but not from the ...

  9. SO(10) - Wikipedia

    en.wikipedia.org/wiki/SO(10)

    The shortened name SO(10) is conventional [1] among physicists, and derives from the Lie algebra or less precisely the Lie group of SO(10), which is a special orthogonal group that is double covered by Spin(10). SO(10) subsumes the Georgi–Glashow and Pati–Salam models, and unifies all fermions in a generation into a single field.

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