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  2. Neutrino astronomy - Wikipedia

    en.wikipedia.org/wiki/Neutrino_astronomy

    Neutrino telescopes consist of hundreds to thousands of optical modules distributed over a large volume. Neutrino astronomy is the branch of astronomy that gathers information about astronomical objects by observing and studying neutrinos emitted by them with the help of neutrino detectors in special Earth observatories. [1]

  3. KM3NeT - Wikipedia

    en.wikipedia.org/wiki/KM3NeT

    The Cubic Kilometre Neutrino Telescope, or KM3NeT, is a European research infrastructure located at the bottom of the Mediterranean Sea.It hosts water Cherenkov neutrino telescopes designed to detect and study neutrinos from distant astrophysical sources as well as from our own atmosphere, contributing significantly to both astrophysics and particle physics knowledge.

  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. Irvine–Michigan–Brookhaven (detector) - Wikipedia

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

    The project was delayed by funding problems and leaks in the water tank, but by the end of summer 1982 the detector was operating at full capacity. The first results were published in 1982. [ 4 ] In 1987, it gained fame for detecting 8 of the roughly 10 58 neutrinos emitted by Supernova 1987A .

  6. Kate Scholberg - Wikipedia

    en.wikipedia.org/wiki/Kate_Scholberg

    Kate Scholberg is a Canadian and American neutrino physicist whose research has included experimental studies of neutrino oscillation and the detection of supernovae. She is currently the Arts & Sciences Distinguished Professor of Physics and Bass Fellow at Duke University .

  7. Radio Neutrino Observatory Greenland - Wikipedia

    en.wikipedia.org/wiki/Radio_Neutrino_Observatory...

    Simulation of a Neutrino Event. An event view from simulations for RNO-G. The neutrino induced particle cascade creates radio emission via the Askaryan effect. This is strongest at the Cherenkov angle at 56°, here shown as a red cone. The radio signal will propagate to the detector according to the ice density (direct and reflected).

  8. Jiangmen Underground Neutrino Observatory - Wikipedia

    en.wikipedia.org/wiki/Jiangmen_Underground...

    The Jiangmen Underground Neutrino Observatory (JUNO) is a medium baseline [2] [3] reactor neutrino experiment under construction at Kaiping, Jiangmen in Guangdong province in Southern China. It aims to determine the neutrino mass hierarchy and perform precision measurements of the Pontecorvo–Maki–Nakagawa–Sakata matrix elements.

  9. ANTARES (telescope) - Wikipedia

    en.wikipedia.org/wiki/ANTARES_(telescope)

    An artist illustration of the Antares neutrino detector and the Nautile For the star, see Antares . ANTARES ( A stronomy with a N eutrino T elescope and A byss environmental RES earch project) is a neutrino detector residing 2.5 km under the Mediterranean Sea off the coast of Toulon , France .