Extragalactic cosmic ray

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The energy spectrum for cosmic rays
The energy spectrum for cosmic rays

Extragalactic cosmic rays are very-high-energy particles that flow into our solar system from beyond our galaxy. The energies these particles possess are in excess of 1015 eV.

[edit] Origin

Unlike Solar cosmic rays or galactic cosmic rays, little is known about the origins of extragalactic cosmic rays. Partially, this can be attributed to a lack of statistics: the amount of cosmic rays reaching the Earth's surface originating from extragalactic sources, is about 1 particle per square meter per year; see figure.

Image of an active galactic nucleus of the active galaxy M87.
Image of an active galactic nucleus of the active galaxy M87.

There are many ideas about which processes may be responsible for cosmic rays with such high energies. In the 'bottom-up' approach, cosmic rays gain more and more energy through electromagnetic processes. Bouncing randomly back and forth in the shock waves of some violent object allows some of the particles to gain energy. Eventually they may build up enough speed that the object can no longer contain them, and they escape. Proposed sites for this type of acceleration include gamma ray bursts and active galactic nuclei.[1] Indeed, recent analysis of cosmic ray measurements with the Pierre Auger Observatory suggests a correlation between the arrival directions of cosmic rays of the highest energies of more than 5×1019 eV and the positions of nearby active galaxies.[2]

There are many more possible sources scientists are considering. These include colliding galaxy systems, accretion flow shocks to clusters of galaxies, and more exotic processes from the very early universe, such as the decay of superheavy particles trapped in the galactic halo, or topological defects.[3]

[edit] Composition

Due to the very low flux of extragalactic cosmic particles received on Earth, little is known about their composition. Most estimates, based on theoretical and numerical models, predict light atomic nuclei such as protons as the dominant particle type.[4]

[edit] References

  1. ^  Fonseca, M.V., Very High Energy Cosmic Rays, Nuclear Physics B (Proc. Suppl.) 114 (2003), pp. 233-246
  2. ^  The Pierre Auger Collaboration,Correlation of the Highest-Energy Cosmic Rays with Nearby Extragalactic Objects, Science 318 (2007), pp. 938-943
  3. ^  Nagano, M. and Watson, A.A., Observations and implications of the ultrahigh-energy cosmic rays, Reviews of Modern Physics 72 (2000) pp. 689-732
  4. ^  Rachen, J., Stanev, T. and Biermann, P., Extragalactic ultra-high energy cosmic rays — II. Comparison with experimental data, Astronomy & Astrophysics 273 (1993) pp. 377-382