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This is a non-exhaustive list of neutrino experiments, neutrino detectors, and neutrino telescopes. Accelerator neutrino (AC), Active galactic nuclei neutrino (AGN), Atmospheric neutrino (ATM), Cosmic ray neutrino (CR), Low-energy solar neutrino (LS), Low-energy supernova neutrino (LSN), Pulsar neutrino (PUL), Reactor neutrino (R), Solar neutrino (S), Supernova neutrino (SN), Terrestrial neutrino (T). Double beta decay (BB), Charged current (CC), Elastic scattering (ES), Neutral current (NC).

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  • Neutrinoobservatorium (de)
  • List of neutrino experiments (en)
  • Eksperymenty neutrinowe (pl)
  • Список экспериментов в физике нейтрино (ru)
rdfs:comment
  • This is a non-exhaustive list of neutrino experiments, neutrino detectors, and neutrino telescopes. Accelerator neutrino (AC), Active galactic nuclei neutrino (AGN), Atmospheric neutrino (ATM), Cosmic ray neutrino (CR), Low-energy solar neutrino (LS), Low-energy supernova neutrino (LSN), Pulsar neutrino (PUL), Reactor neutrino (R), Solar neutrino (S), Supernova neutrino (SN), Terrestrial neutrino (T). Double beta decay (BB), Charged current (CC), Elastic scattering (ES), Neutral current (NC). (en)
  • Eksperymenty neutrinowe (jak również detektory neutrin, obserwatoria neutrin i teleskopy neutrin) służą badaniu zagadnień związnych z fizyką neutrin, takich jak: * właściwości neutrin (np. obserwacje kolejnych zapachów neutrin, pomiary masy neutrin, testy czy są cząstkami Majorany), * procesy produkcji neutrin (badanie neutrin z różnych źródeł w tym pozaziemskich), * oddziaływania neutrin, * oscylacje neutrin. Poniższa tabela zawiera niepełną listę eksperymentów neutrinowych, detektorów neutrin i obserwatoriów neutrin. (pl)
  • Список экспериментов, исследующих физику нейтрино, и нейтринных телескопов. (ru)
  • Neutrinoobservatorien (auch als Neutrinoteleskope, Neutrinodetektoren oder – etwas zu allgemein – Neutrino-Experimente bezeichnet) sind Teilchendetektoren speziell für den Nachweis und die Messung von Neutrinos aus weit entfernten Quellen. Als weit entfernt werden hier 100 Meter oder mehr angesehen. Weil Neutrinoreaktionen sehr kleine Wirkungsquerschnitte haben, reagieren Neutrinos mit normaler Materie nur sehr selten. Neutrinodetektoren müssen deshalb sehr groß sein und meist jahrelang Daten sammeln, um statistisch signifikante Messergebnisse zu erreichen. (de)
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