CORDIS Project
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This project investigates the acceleration of high-energy particles at collisionless shocks in astrophysical plasmas, focusing on gamma-ray bursts and supernova remnants. It aims to understand how these processes convert flow energy into relativistic particles, contributing to our knowledge of cosmic rays and their emi…
The acceleration of high-energy particles at collisionless shocks in astrophysical plasmas is a common phenomenon in the Universe and takes place in a variety of systems, from the heliosphere up to the most distant cosmic sources.
The best known example for such non-thermal particle populations are cosmic rays, but additional evidence for the existence of high energy particles comes from observations of non-thermal synchrotron and inverse Compton emission from several sources, as pulsar wind neb…
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