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  2. 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.

  3. Homestake experiment - Wikipedia

    en.wikipedia.org/wiki/Homestake_experiment

    After Bahcall calculated the rate at which the detector should capture neutrinos, Davis's experiment turned up only one third of this figure. The experiment was the first to successfully detect and count solar neutrinos, and the discrepancy in results created the solar neutrino problem. The experiment operated continuously from 1970 until 1994.

  4. List of neutrino experiments - Wikipedia

    en.wikipedia.org/wiki/List_of_neutrino_experiments

    Neutrino experiments are scientific studies investigating the properties of neutrinos, which are subatomic particles that are very difficult to detect due to their weak interactions with matter. Neutrino experiments are essential for understanding the fundamental properties of matter and the universe's behaviour at the subatomic level.

  5. High-energy cosmic neutrino detected under Mediterranean Sea

    www.aol.com/news/high-energy-cosmic-neutrino...

    Using an observatory under construction deep beneath the Mediterranean Sea near Sicily, scientists have detected a ghostly subatomic particle called a neutrino boasting record-breaking energy in ...

  6. Neutrino astronomy - Wikipedia

    en.wikipedia.org/wiki/Neutrino_astronomy

    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. The PMTs are under more than a kilometer of ice, and will detect the photons from neutrino interactions within a cubic kilometer of ice

  7. 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 ...

  8. Inverse beta decay - Wikipedia

    en.wikipedia.org/wiki/Inverse_beta_decay

    The timing and spatial coincidence between the prompt positron annihilation and delayed neutron capture provides a clear IBD signature in neutrino detectors, allowing for discrimination from background. [4] The IBD cross section is dependent on antineutrino energy and capturing element, although is generally on the order of 10 −44 cm 2 ...

  9. CONUS-Experiment - Wikipedia

    en.wikipedia.org/wiki/CONUS-Experiment

    Due to this fact, neutrino detectors are generally very large and filled with several (kilo)tons of target material. There are basically two possibilities to detect neutrinos: First, they can interact with the electrons in the atomic shell of a target atom, and second they can interact with the protons and neutrons of an atomic nucleus ...

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