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Encyclopedia > GZK cutoff

The Greisen-Zatsepin-Kuzmin limit (GZK limit) is a theoretical upper limit on the energy of cosmic rays from distant sources. Cosmic rays can loosely be defined as energetic particles originating outside of the Earth. ...


This limit was computed in 1966 by Kenneth Greisen, Vadem Kuzmin and Georgi Zatsepin, based on interactions predicted by special relativity between the cosmic ray and the photons of the cosmic microwave background radiation. They predicted that cosmic rays with energies over the threshold energy of 5×1019 eV would interact with CMB photons until their energy fell below the threshold. Therefore, extragalactic cosmic rays with energies greater than this threshold energy should never be observed on Earth.-1... Special relativity (SR) or the special theory of relativity is the physical theory published in 1905 by Albert Einstein. ... WMAP image of the CMB anisotropy,Cosmic microwave background radiation(June 2003) The cosmic microwave background radiation (CMB) is a form of electromagnetic radiation that fills the whole of the universe. ... An electronvolt (symbol: eV) is the amount of energy gained by a single unbound electron when it falls through an electrostatic potential difference of one volt. ...

Unsolved problems in physics: Why is it that some cosmic rays appear to possess energies that are theoretically too high, given that there are no possible near Earth sources, and that rays from distant sources should have been absorbed by the cosmic microwave background radiation?

A number of observations have been made by the AGASA experiment that appear to show cosmic rays from distant sources with energies above this limit (whimsically dubbed Oh-My-God particles). The observed existence of these particles is the so-called GZK paradox or cosmic ray paradox. General science-related image. ... The following are some of the unsolved problems in physics. ... WMAP image of the CMB anisotropy,Cosmic microwave background radiation(June 2003) The cosmic microwave background radiation (CMB) is a form of electromagnetic radiation that fills the whole of the universe. ... On the evening of October 15, 1991, an ultra-high energy cosmic particle was observed over Salt Lake City, Utah. ...


These observations appear to contradict the predictions of the theory of special relativity. However, there are a number of possible explanations for these observations that are consistent with special relativity. Firstly, the observations could be due to an instrument error or an incorrect interpretation of the experiment. Secondly, the cosmic rays could have local sources (although it is unclear what these sources could be). Another suggestion involves ultra-high energy weakly interacting particles (for instance neutrinos) which might be created at great distances and later react locally to give rise to the particles observed. The neutrino is an elementary particle. ...


A number of exotic theories have been advanced to explain these observations, of which the most notable is the theory of doubly-special relativity. Doubly-Special Relativity is a new theory of special relativity first postulated in a paper by Giovanni Amelino-Camelia. ...


As of 2003, a number of cosmic ray experiments such as GLAST and the Pierre Auger Observatory are now planned which are intended to confirm or deny the correctness of the earlier observations. 2003 is a common year starting on Wednesday of the Gregorian calendar, and also: The International Year of Freshwater The European Disability Year Events January events January 1 Luíz Inácio Lula Da Silva becomes the 37th President of Brazil. ... The Gamma-ray Large Area Space Telescope, or GLAST, is future space-based gamma-ray telescope, designed to explore the high-energy Universe. ...


External links

  • http://www.physics.rutgers.edu/hex/HIRES.html
  • http://physicsweb.org/article/world/15/9/3
  • http://www.p-ng.si/public/pao/history.php

  Results from FactBites:
 
Re: Why do we expect GZK cutoff at the energies 6x10^19 eV ? (244 words)
The GZK cutoff is not due to proton pair production.
You don't calculate the GZK cutoff exactly at the threshhold, but rather at the delta (1232 MeV) resonance where the cross section is largest.
The GZK cutoff is not sharp, since the cross-sections vary with energy and the CMB photons have a wide distribution.
More About PAO (1253 words)
There is a general agreement on the fact that the conventional acceleration mechanisms have difficulties in explaining the observations made of UHE cosmic rays up to the end of the spectrum.
The corresponding attenuation lengths are less than a few tens of Mpc: this is the origin of the GZK cutoff.
Above the GZK cutoff the rate is roughly 10 events per century and per square kilometer for a standard ground detector.
  More results at FactBites »


 

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