Particle Acceleration on Megaparsec Scales in a Merging Galaxy Cluster

Details Particle Acceleration on Megaparsec Scales in a Merging Galaxy Cluster Particle Acceleration on Megaparsec Scales in a Merging Galaxy Cluster

2010-10-20

arxiv.org/abs/1010.4306v1

Science, Volume 330, Issue 6002, pp. 347- (2010)

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

Published in Science Express on 23 September 2010, 6 figures, Supporting Online Material included. This is the author's versio

Scientific paper

10.1126/science.1194293

Galaxy clusters form through a sequence of mergers of smaller galaxy clusters and groups. Models of diffusive shock acceleration (DSA) suggest that in shocks that occur during cluster mergers, particles are accelerated to relativistic energies, similar to supernova remnants. Together with magnetic fields these particles emit synchrotron radiation and may form so-called radio relics. Here we report the detection of a radio relic for which we find highly aligned magnetic fields, a strong spectral index gradient, and a narrow relic width, giving a measure of the magnetic field in an unexplored site of the universe. Our observations prove that DSA also operates on scales much larger than in supernova remnants and that shocks in galaxy clusters are capable of producing extremely energetic cosmic rays.

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