Cosmic Rays around Supernova Remnants

A special issue of Galaxies (ISSN 2075-4434).

Deadline for manuscript submissions: closed (30 November 2020) | Viewed by 6296

Special Issue Editor


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Guest Editor
Max-Planck-Institut fuer extraterrestrische Physik, 85748 Garching bei München, Germany
Interests: high-energy astrophysics; cosmic rays; gamma rays

Special Issue Information

Dear Colleagues,

Supernova remnants (SNR) are probably a main source of high-energy particles in the galaxy, although this remains to be proved. Observations of related electromagnetic radiation (gamma rays, X-ray, synchrotron) provide clues to the details of the mechanisms involved in the acceleration and propagation of these cosmic rays (CR). Interaction with nearby gas clouds, amplification of the magnetic field, and secondary particle production in the remnants are of special importance. While many SNR have been observed from radio to gamma rays, the emission process may be hadronic or leptonic, or a combination of these, with an observational distinction often difficult to assess. Synchrotron X-rays probe very high-energy electrons and acceleration on short time scales. SNR affect CR observed at the earth, for example secondary positrons and antiprotons, as well as secondary nuclei. Evidence for a nearby recent supernova via radioactive 60Fe is also changing our view of the subject. This Special Issue aims to cover current research on cosmic rays in and around SNR, both theoretical and observational. Other related sources like pulsar wind nebulae, pulsars and superbubbles, may also be addressed.

Dr. Andrew W. Strong
Guest Editor

 Reference

  1. Sano, H.; Rowell, G.; Reynoso, E. M.; Jung-Richardt, I.; Yamane, Y.; Nagaya, T.; Yoshiike, S.; Hayashi, K.; Torii, K.; Maxted, N.; et al. Possible Evidence for Cosmic-Ray Acceleration in the Type Ia Supernova Remnant RCW 86: Spatial Correlation between TeV Gamma rays and Interstellar Atomic Protons. Astrophys. J. 2018. (Draft version)
  2. D'Angelo, M.; Blasi, P.; Amato, E. Grammage of cosmic rays around Galactic supernova remnants. Phys. Rev. D 2016, 94, 083003.
  3. Gabici, S.; Krause, J.; Morlino, G.; Nava, L. Acceleration of cosmic rays and gamma-ray emission from supernova remnant/molecular cloud associations. In Proceeding of EPJ Web of Conferences, Geneva, Switzerland, December 2015.
  4. Berezhko, E. G. Origin of Galactic Cosmic Rays from Supernova Remnants. Nucl. Phys. B 2014, 256, 23–35.
  5. Grenier, I.A.; Black, J.H.; Strong, A.W. The Nine Lives of Cosmic Rays in Galaxies. Annu. Rev. Astron. Astrophys. 2015, 53, 199–246.

 

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Keywords

  • cosmic rays
  • supernova remnants
  • interstellar medium

Published Papers (2 papers)

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Review

13 pages, 308 KiB  
Review
The Self-Control of Cosmic Rays
by Pasquale Blasi
Galaxies 2019, 7(2), 64; https://doi.org/10.3390/galaxies7020064 - 04 Jun 2019
Cited by 13 | Viewed by 3084
Abstract
Several independent pieces of information have recently hinted at a prominent role of cosmic rays in controlling their own transport, within and around the sources as well as throughout their propagation on Galactic scales and even possibly during their escape from the Galaxy. [...] Read more.
Several independent pieces of information have recently hinted at a prominent role of cosmic rays in controlling their own transport, within and around the sources as well as throughout their propagation on Galactic scales and even possibly during their escape from the Galaxy. I will discuss this topic with special attention to the theoretical implications and possible additional observational evidence that we may seek with upcoming experiments. Full article
(This article belongs to the Special Issue Cosmic Rays around Supernova Remnants)
16 pages, 839 KiB  
Review
The Important Role of Cosmic-Ray Re-Acceleration
by Martina Cardillo
Galaxies 2019, 7(2), 49; https://doi.org/10.3390/galaxies7020049 - 24 Apr 2019
Cited by 6 | Viewed by 2916
Abstract
In the last decades, the improvement of high energy instruments has enabled a deeper understanding of the Cosmic Ray origin issue. In particular, the γ -ray satellites AGILE (Astrorivelatore Gamma ad Immagini LEggero) and Fermi-LAT (Fermi-Large Area Telescope) have strongly contributed to the [...] Read more.
In the last decades, the improvement of high energy instruments has enabled a deeper understanding of the Cosmic Ray origin issue. In particular, the γ -ray satellites AGILE (Astrorivelatore Gamma ad Immagini LEggero) and Fermi-LAT (Fermi-Large Area Telescope) have strongly contributed to the confirmation of direct involvement of Supernova Remnants in Cosmic Ray energization. Despite several attempts to fit experimental data assuming the presence of freshly accelerated particles, the scientific community is now aware that the role of pre-existing Cosmic Ray re-acceleration cannot be neglected. In this work, we highlight the importance of pre-existing Cosmic Ray re-acceleration in the Galaxy showing its fundamental contribution in middle aged Supernova Remnant shocks and in the forward shock of stellar winds. Full article
(This article belongs to the Special Issue Cosmic Rays around Supernova Remnants)
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