Numerical modeling of relativistic particle shock acceleration

Details Numerical modeling of relativistic particle shock acceleration Numerical modeling of relativistic particle shock acceleration

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011astra...7..287m&link_type=abstract

Astrophysics and Space Sciences Transactions, Volume 7, Issue 3, 2011, pp.287-294

Astronomy and Astrophysics

Astrophysics

Scientific paper

The shock acceleration mechanism is invoked to explain non-thermal cosmic rays in Supernova Remnants, Active Galactic Nuclei and Gamma Ray Bursts jets. Especially, the importance of relativistic shock acceleration in extragalactic sources is a recurring theme raising a significant interest in the research community. We will briefly overview the shock acceleration mechanism and we will address the properties of non-relativistic and relativistic shocks, particularly focusing on relativistic simulation studies.

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