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  2. Neutrino - Wikipedia

    en.wikipedia.org/wiki/Neutrino

    More formally, neutrino flavor eigenstates (creation and annihilation combinations) are not the same as the neutrino mass eigenstates (simply labeled "1", "2", and "3"). As of 2024, it is not known which of these three is the heaviest. The neutrino mass hierarchy consists of two possible configurations. In analogy with the mass hierarchy of the ...

  3. Atomic mass - Wikipedia

    en.wikipedia.org/wiki/Atomic_mass

    The atomic mass (relative isotopic mass) is defined as the mass of a single atom, which can only be one isotope (nuclide) at a time, and is not an abundance-weighted average, as in the case of relative atomic mass/atomic weight. The atomic mass or relative isotopic mass of each isotope and nuclide of a chemical element is, therefore, a number ...

  4. Lepton - Wikipedia

    en.wikipedia.org/wiki/Lepton

    The masses of those particles are small compared to nucleons—the mass of an electron (0.511 MeV/c 2) [18] and the mass of a muon (with a value of 105.7 MeV/c 2) [19] are fractions of the mass of the "heavy" proton (938.3 MeV/c 2), and the mass of a neutrino is nearly zero. [20]

  5. Generation (particle physics) - Wikipedia

    en.wikipedia.org/wiki/Generation_(particle_physics)

    The lower bound for a fourth generation neutrino (ν' τ) mass as of 2010 was at about 60 GeV (millions of times larger than the upper bound for the other 3 neutrino masses). [10] As of 2024, no evidence of a fourth-generation neutrino has ever been observed in neutrino oscillation studies either.

  6. Degenerate matter - Wikipedia

    en.wikipedia.org/wiki/Degenerate_matter

    Degenerate gas can be compressed to very high densities, typical values being in the range of 10,000 kilograms per cubic centimeter. There is an upper limit to the mass of an electron-degenerate object, the Chandrasekhar limit, beyond which electron degeneracy pressure cannot support the object against

  7. Supernova neutrinos - Wikipedia

    en.wikipedia.org/wiki/Supernova_Neutrinos

    The luminosity of different neutrino and antineutrino species are roughly the same. [3] They carry away about 99% of the gravitational energy of the dying star as a burst lasting tens of seconds. [ 4 ] [ 5 ] The typical supernova neutrino energies are 10 to 20 MeV . [ 6 ]

  8. Electron capture - Wikipedia

    en.wikipedia.org/wiki/Electron_capture

    Electron capture happens most often in the heavier neutron-deficient elements where the mass change is smallest and positron emission is not always possible. When the loss of mass in a nuclear reaction is greater than zero but less than 2m e c 2 the process cannot occur by positron emission, but occurs spontaneously for electron capture.

  9. Neutronium - Wikipedia

    en.wikipedia.org/wiki/Neutronium

    Neutronium (or neutrium, [1] neutrite, [2] or element zero) is a hypothetical substance made purely of neutrons.The word was coined by scientist Andreas von Antropoff in 1926 (before the 1932 discovery of the neutron) for the hypothetical "element of atomic number zero" (with no protons in its nucleus) that he placed at the head of the periodic table (denoted by -).