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  2. Neutrino - Wikipedia

    en.wikipedia.org/wiki/Neutrino

    A neutrino (/ nj uː ˈ t r iː n oʊ / new-TREE-noh; denoted by the Greek letter ν) is an elementary particle that interacts via the weak interaction and gravity. [2] [3] The neutrino is so named because it is electrically neutral and because its rest mass is so small that it was long thought to be zero.

  3. Neutrino astronomy - Wikipedia

    en.wikipedia.org/wiki/Neutrino_astronomy

    Neutrinos interact incredibly rarely with matter, so the vast majority of neutrinos will pass through a detector without interacting. If a neutrino does interact, it will only do so once. Therefore, to perform neutrino astronomy, large detectors must be used to obtain enough statistics. [23] The IceCube Neutrino Detector at the South Pole.

  4. Neutrino theory of light - Wikipedia

    en.wikipedia.org/wiki/Neutrino_theory_of_light

    To form a photon, which satisfies parity and charge conjugation, two sets of two-component neutrinos (i.e., right-handed and left-handed neutrinos) are needed. Perkins (see Sec. VI of Ref. [ 17 ] ) attempted to solve this problem by noting that the needed two sets of two-component neutrinos would exist if the positive muon is identified as the ...

  5. Weak interaction - Wikipedia

    en.wikipedia.org/wiki/Weak_interaction

    as electric charge does in electromagnetism, and color charge in the strong interaction; a different number with a similar name, weak charge, discussed below, is used for interactions with the Z 0. All left-handed fermions have a weak isospin value of either ⁠+ + 1 / 2 ⁠ or ⁠− + 1 / 2 ⁠; all right-handed fermions have 0 isospin.

  6. Neutrino detector - Wikipedia

    en.wikipedia.org/wiki/Neutrino_detector

    The inside of the MiniBooNE neutrino detector. A neutrino detector is a physics apparatus which is designed to study neutrinos.Because neutrinos only weakly interact with other particles of matter, neutrino detectors must be very large to detect a significant number of neutrinos.

  7. Supernova neutrinos - Wikipedia

    en.wikipedia.org/wiki/Supernova_Neutrinos

    The flavor evolution of neutrinos, propagating through the dense and turbulent interior of the supernova, is dominated by the collective behavior associated with neutrino-neutrino interactions. Therefore, supernova neutrinos offer an opportunity to examine neutrino flavor mixing under high-density conditions. [9]

  8. Lepton - Wikipedia

    en.wikipedia.org/wiki/Lepton

    In particle physics, a lepton is an elementary particle of half-integer spin (spin ⁠ 1 / 2 ⁠) that does not undergo strong interactions. [1] Two main classes of leptons exist: charged leptons (also known as the electron-like leptons or muons), including the electron, muon, and tauon, and neutral leptons, better known as neutrinos.

  9. Standard Model - Wikipedia

    en.wikipedia.org/wiki/Standard_Model

    Neutrinos of all generations also do not decay, and pervade the universe, but rarely interact with baryonic matter. There are six quarks: up , down , charm , strange , top , and bottom . [ 34 ] [ 37 ] Quarks carry color charge , and hence interact via the strong interaction .