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  2. Neutrino oscillation - Wikipedia

    en.wikipedia.org/wiki/Neutrino_oscillation

    Neutrino oscillation is a quantum mechanical phenomenon in which a neutrino ... Right-handed neutrinos would help to explain the origin of matter through a mechanism ...

  3. Mikheyev–Smirnov–Wolfenstein effect - Wikipedia

    en.wikipedia.org/wiki/Mikheyev–Smirnov...

    The Mikheyev–Smirnov–Wolfenstein effect (often referred to as the matter effect) is a particle physics process which modifies neutrino oscillations in matter of varying density. The MSW effect is broadly analogous to the differential retardation of sound waves in density-variable media, however it also involves the propagation dynamics of ...

  4. Neutrino - Wikipedia

    en.wikipedia.org/wiki/Neutrino

    The neutrino [a] was postulated first by Wolfgang Pauli in 1930 to explain how beta decay could conserve energy, momentum, and angular momentum ().In contrast to Niels Bohr, who proposed a statistical version of the conservation laws to explain the observed continuous energy spectra in beta decay, Pauli hypothesized an undetected particle that he called a "neutron", using the same -on ending ...

  5. Physics beyond the Standard Model - Wikipedia

    en.wikipedia.org/wiki/Physics_beyond_the...

    Physics beyond the Standard Model (BSM) refers to the theoretical developments needed to explain the deficiencies of the Standard Model, such as the inability to explain the fundamental parameters of the standard model, the strong CP problem, neutrino oscillations, matter–antimatter asymmetry, and the nature of dark matter and dark energy. [1]

  6. Hyper-Kamiokande - Wikipedia

    en.wikipedia.org/wiki/Hyper-Kamiokande

    Neutrino oscillations are a quantum mechanical phenomenon in which neutrinos change their flavour (neutrino flavours states: ν e, ν μ, ν τ) while moving, caused by the fact that the neutrino flavour states are a mixture of the neutrino mass states (ν 1, ν 2, ν 3 mass states with masses m 1, m 2, m 3, respectively). The oscillation ...

  7. Supernova neutrinos - Wikipedia

    en.wikipedia.org/wiki/Supernova_Neutrinos

    Neutrino oscillations in dense matter is an active field of research. [31] Schematic of neutrino bulb model. Neutrinos undergo flavor conversions after they thermally decouple from the proto-neutron star. Within the neutrino-bulb model, neutrinos of all flavors decouple at a single sharp surface near the surface of the star. [32]

  8. Super-Kamiokande - Wikipedia

    en.wikipedia.org/wiki/Super-Kamiokande

    The K2K experiment was a neutrino experiment from June 1999 to November 2004. This experiment was designed to verify oscillations observed by Super-Kamiokande through muon neutrinos. It gives first positive measurement of neutrino oscillations in conditions that both source and detector are under control. The Super-Kamiokande detector plays an ...

  9. Pontecorvo–Maki–Nakagawa–Sakata matrix - Wikipedia

    en.wikipedia.org/wiki/Pontecorvo–Maki...

    In particle physics, the Pontecorvo–Maki–Nakagawa–Sakata matrix (PMNS matrix), Maki–Nakagawa–Sakata matrix (MNS matrix), lepton mixing matrix, or neutrino mixing matrix is a unitary [a] mixing matrix that contains information on the mismatch of quantum states of neutrinos when they propagate freely and when they take part in weak interactions.