Non-thermal acceleration mechanisms in supernova remnant shells
Anne Decourchelle (SAp/AIM, CEA Saclay)

TL;DR
This paper reviews non-thermal particle acceleration mechanisms in supernova remnants, discusses recent X-ray and gamma-ray observations, and highlights open questions in the field for future research.
Contribution
It provides a comprehensive overview of acceleration processes and observational evidence, emphasizing future X-ray missions like Simbol-X.
Findings
Summary of nonthermal acceleration mechanisms
Review of supernova remnant observations in X-rays and gamma rays
Discussion of open issues in particle acceleration
Abstract
A review of the main issues in the field of particle acceleration in Supernova Remnants is provided in the context of future X-ray observations with Simbol-X. After a summary of the nonthermal acceleration mechanisms at work, I briefly review the observations of supernova remnants in hard X-rays and in gamma rays. Open issues are discussed in this framework.
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Taxonomy
TopicsGeophysics and Gravity Measurements · Astrophysics and Cosmic Phenomena · Geomagnetism and Paleomagnetism Studies
