Diffuse gamma-ray emission from self-confined cosmic rays around Galactic sources. Issue 2 (3rd November 2017)

• Record Type: Journal Article
• Authors: D'Angelo, M.; Morlino, G.; Amato, E.; Blasi, P.
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 474:Issue 2(2018)
• Page Start: 1944
• Page End: 1954
• Publication Date: 2017-11-03
• Subjects: radiation mechanisms: non-thermal -- cosmic rays -- ISM: supernova remnants -- gamma-rays: diffuse background; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stx2828
• Languages: English
• ISSNs: 0035-8711

Abstract

Abstract: The propagation of particles accelerated at supernova remnant shocks and escaping the parent remnants is likely to proceed in a strongly non-linear regime, due to the efficient self-generation of Alfvén waves excited through streaming instability near the sources. Depending on the amount of neutral hydrogen present in the regions around the sites of supernova explosions, cosmic rays may accumulate an appreciable grammage in the same regions and get self-confined for non-negligible times, which in turn results in an enhanced rate of production of secondaries. Here we calculate the contribution to the diffuse gamma-ray background due to the overlap along lines of sight of several of these extended haloes as due to pion production induced by self-confined cosmic rays. We find that if the density of neutrals is low, the haloes can account for a substantial fraction of the diffuse emission observed by Fermi -Large Area Telescope (LAT), depending on the orientation of the line of sight with respect to the direction of the Galactic Centre.