Leonard E Parker

Center for Gravitation, Cosmology & Astrophysics

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Leonard E Parker Center for Gravitation, Cosmology and Astrophysics

Closing in on the origin of cosmic rays

Posted by Luis Anchordoqui on 12 November 2007

UWM Professor Luis Anchordoqui and the rest of the Pierre Auger Collaboration may have just solved one of the greatest mysteries of modern astrophysics: what is the origin of cosmic rays?
Cosmic rays are particles of astounding energy that bombard the Earth from all direction in space.

Each second, about 200 cosmic ray particles with energies of a few million electron volts strike every square meter of the Earth. While these low-energy cosmic rays are plentiful, those with higher energies are far rarer. Events have been observed with an energy 100 million times higher than those produced by the most powerful particle accelerator on Earth, but at a rate of only a few per square kilometer per millenium! Instruments with extremely large collecting areas are deployed to sample the shower of secondary particles produced when the primary cosmic ray collides with the Earth atmosphere.

For decades, physicists have wondered what the source of these particles, with energies that can exceed 100 exa-EV (that's a 1 followed by 20 zeroes of electron volts), could be. The Pierre Auger Observatory, a collection of particle detectors covering 3000 square kilometers in Western Argentina, may have just provided the answer.

Scientists of the Pierre Auger Collaboration announced that active galactic nuclei are the most likely candidate for the source of the highest-energy cosmic rays that hit Earth. The team of scientists from 17 countries found that the sources of the highest-energy particles are not distributed uniformly across the sky. Instead, their results link the origins of these mysterious particles to the locations of nearby galaxies that have active nuclei in their centers.

The celestial sphere in galactic coordinates showing the arrival directions of the 27 highest energy cosmic rays detected by Auger. These are shown as circles of radius 3.1°. The positions of 472 AGN within 75 megaparsecs are shown as red *'s. The blue region defines the field of view of Auger; deeper blue indicates larger exposure. The closest AGN, Centaurus A, is marked as a white *. The supergalactic plane is indicated by a dashed curve. Published in Science 318, 938 (2007).

Active Galactic Nuclei (AGN) are thought to be powered by supermassive black holes that are devouring large amounts of matter. They have long been considered sites where high-energy particle production might take place. They swallow gas, dust and other matter from their host galaxies and spew out particles and energy. While most galaxies have black holes at their center, only a fraction of all galaxies have an AGN. The exact mechanism of how AGNs can accelerate particles to energies 100 million times higher than the most powerful particle accelerator on Earth is still a mystery.

The results were published at the Nov. 9 2007 issue of the journal Science.

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