The Universe contains much better particle accelerators than anything we humans can contrive. While the Large Hadron Collider (LHC) is capable of sending individual protons to energies of 7 trillion electron volts (7 TeV, or 7×1012 eV), cosmic ray protons can exceed 1018 eV—a million times more energetic. Achieving this acceleration requires a highly energetic source. The leading candidates are gamma ray bursts (GRBs), which are exceedingly bright astronomical events, often associated with supernovae. According to a commonly accepted model of GRB explosions, the proton acceleration should be accompanied by a flood of neutrinos—low-mass neutral particles.
That model is apparently in trouble. An analysis of high-energy neutrinos observed by the IceCube experiment at the South Pole has found too few neutrinos relative to what GRB models say we should see. By comparing the incidences of GRBs from satellite observations to the flux of neutrinos at the IceCube neutrino observatory, researchers were able to set an upper limit on the total number of neutrinos at the energies associated with GRBs. They determined that no current GRB model is able to match the observed flux, meaning either that GRBs are not the primary source of high-energy cosmic rays, or that the model for GRB neutrino production is incorrect.
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