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  2. Muometric navigation - Wikipedia

    en.wikipedia.org/wiki/Muometric_navigation

    The sender and receiver use the same muons to create truly random cryptographic keys from the timestamp. Based on the precise time delay between the sender and the receiver calculated from the distance between the detectors within 10 meters each other, [ 23 ] the receiver knows the private key without having to directly exchange it between the ...

  3. Muon - Wikipedia

    en.wikipedia.org/wiki/Muon

    Muons have a mass of 105.66 MeV/c 2, which is approximately 206.768 2827 (46) ‍ [6] times that of the electron, m e. There is also a third lepton, the tau, approximately 17 times heavier than the muon. Due to their greater mass, muons accelerate more slowly than electrons in electromagnetic fields, and emit less bremsstrahlung (deceleration ...

  4. IceCube Neutrino Observatory - Wikipedia

    en.wikipedia.org/wiki/IceCube_Neutrino_Observatory

    There is a large background of muons created not by neutrinos from astrophysical sources but by cosmic rays impacting the atmosphere above the detector. There are about 10 6 times more cosmic ray muons than neutrino-induced muons observed in IceCube. [citation needed] Most of these can be rejected using the fact that they are traveling ...

  5. 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.

  6. Neutrino oscillation - Wikipedia

    en.wikipedia.org/wiki/Neutrino_oscillation

    Neutrino oscillation is a quantum mechanical phenomenon in which a neutrino created with a specific lepton family number ("lepton flavor": electron, muon, or tau) can later be measured to have a different lepton family number.

  7. Cosmic ray - Wikipedia

    en.wikipedia.org/wiki/Cosmic_ray

    An active search from Earth orbit for anti-alpha particles as of 2019 [12] had found no unequivocal evidence. Upon striking the atmosphere, cosmic rays violently burst atoms into other bits of matter, producing large amounts of pions and muons (produced from the decay of charged pions, which have a short half-life) as well as neutrinos. [13]

  8. ISIS Neutron and Muon Source - Wikipedia

    en.wikipedia.org/wiki/ISIS_Neutron_and_Muon_Source

    ISIS Neutron and Muon Source; Location: Rutherford Appleton Laboratory, United Kingdom: Scientific Purpose: Supports national and international community of around 3000 scientists who use neutrons and muons for research in physics, chemistry, materials science, engineering, biology and more.

  9. Experimental testing of time dilation - Wikipedia

    en.wikipedia.org/wiki/Experimental_testing_of...

    The emergence of the muons is caused by the collision of cosmic rays with the upper atmosphere, after which the muons reach Earth. The probability that muons can reach the Earth depends on their half-life, which itself is modified by the relativistic corrections of two quantities: a) the mean lifetime of muons and b) the length between the upper and lower atmosphere (at Earth's surface).