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Supernova Remnant-Cosmic Ray connection: a modern view

Published online by Cambridge University Press:  17 October 2017

Giovanni Morlino Open the ORCID record for Giovanni Morlino [Opens in a new window]
Giovanni Morlino*
Affiliation:
Gran Sasso Science Institute, viale F. Crispi 7, 67100 L’Aquila, Italy. email: giovanni.morlino@infn.gssi.it
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Abstract

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The Cosmic Ray (CR) physics has entered a new era driven by high precision measurements coming from direct detection (especially AMS-02 and PAMELA) and also from gamma-ray observations (Fermi-LAT). In this review we focus our attention on how such data impact the understanding of the supernova remnant paradigm for the origin of CRs. In particular we discuss advancement in the field concerning the three main stages of the CR life: the acceleration process, the escape from the sources and the propagation throughout the Galaxy. We show how the new data reveal a phenomenology richest than previously thought that could even challenge the current understanding of CR origin.

Keywords

acceleration of particlesradiation mechanisms: nonthermal(ISM:) cosmic rayssupernova remnantsgamma rays: observations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S331: Supernova 1987A:30 years later - Cosmic Rays and Nuclei from Supernovae and their aftermaths , February 2017 , pp. 230 - 241
Copyright
Copyright © International Astronomical Union 2017 

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