Although cosmic rays were discovered 100 years ago, their origin remains¹ one of the most enduring mysteries in physics. Now, the IceCube Neutrino Observatory², a massive detector³ in Antarctica, is homing in on how the highest energy cosmic rays are produced. "Although we have not discovered where cosmic rays come from, we have taken a major step towards ruling out one of the leading predictions," said IceCube principal investigator⁴ and University of Wisconsin-Madison physics professor Francis Halzen.

Cosmic rays are electrically charged particles, such as protons, that strike Earth from all directions, with energies up to one hundred million times higher than those created in human-made accelerators. The intense conditions needed to generate such energetic particles have focused physicists⁵' interest on two potential sources: the massive black holes at the centers of active galaxies⁶, and the exploding fireballs observed by astronomers⁷ as gamma ray bursts (GRBs).

IceCube is using neutrinos, which are believed to accompany cosmic ray production, to explore these theories. In a paper published in the April 19 issue of the journal Nature, the IceCube collaboration⁸ describes a search for neutrinos emitted from 300 gamma ray bursts observed, most recently in coincidence with the SWIFT and Fermi satellites, between May 2008 and April 2010. Surprisingly, they found none -- a result that contradicts 15 years of predictions and challenges one of the two leading theories for the origin of the highest energy cosmic rays.

"The result of this neutrino search is significant because for the first time we have an instrument with sufficient sensitivity to open a new window on cosmic ray production and the interior processes of GRBs," said IceCube spokesperson and University of Maryland physics professor Greg Sullivan. "The unexpected absence of neutrinos from GRBs has forced a re-evaluation of the theory for production of cosmic rays and neutrinos in a GRB fireball and possibly the theory that high energy cosmic rays are generated in fireballs."

IceCube is a high energy neutrino telescope at the geographical⁹ South Pole in Antarctica, operated by a collaboration of 250 physicists and engineers from the USA, Germany, Sweden, Belgium, Switzerland, Japan, Canada, New Zealand, Australia and Barbados.

The IceCube Neutrino Observatory was built under a National Science Foundation (NSF) Major Research Equipment and Facilities Construction grant, with assistance from partner funding agencies around the world. The NSF Office of Polar Programs continues to support the project with a Maintenance and Operations grant. Construction was finished in December 2010.