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Concept information

high-energy astrophysics > particle astrophysics > cosmic ray > Greisen-Zatsepin-Kuzmin cut off
... > theoretical physics aspects > field theory > classical field theory > electromagnetism > electromagnetic radiation > ionizing radiation > cosmic ray > Greisen-Zatsepin-Kuzmin cut off

Terme préférentiel

Greisen-Zatsepin-Kuzmin cut off  

Définition

  • The Greisen–Zatsepin–Kuzmin limit (GZK limit) is a theoretical upper limit on the energy of cosmic ray protons traveling from other galaxies through the intergalactic medium to our galaxy. The limit is 5×10¹⁹eV (50 EeV), or about 8 joules (the energy of a proton travelling at ≈ 99.99999999999999999998% the speed of light). The limit is set by the slowing effect of interactions of the protons with the microwave background radiation over long distances (≈ 160 million light-years). The limit is at the same order of magnitude as the upper limit for energy at which cosmic rays have experimentally been detected, although indeed some detections appear to have exceeded the limit, as noted below. For example, one extreme-energy cosmic ray, the Oh-My-God Particle, which has been found to possess a record-breaking 3.12×10²⁰eV (50 joules) of energy (about the same as the kinetic energy of a 95 km/h baseball). (Wikipedia, The Free Encyclopedia, https://en.wikipedia.org/wiki/Greisen%E2%80%93Zatsepin%E2%80%93Kuzmin_limit)

Concept générique

Synonyme(s)

  • Greisen-Zatsepin-Kuzmin cutoff
  • Greisen-Zatsepin-Kuzmin limit
  • GZK cut off
  • GZK cutoff
  • GZK limit

Traductions

URI

http://data.loterre.fr/ark:/67375/MDL-CRK7HNXF-1

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