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- W4293492988 abstract "New evidence that cosmic rays (hadronic component) are accelerated by supernova remnant shocks all the way from low energies to high energies, has come from recent works combining gamma-ray observations in the sub-GeV to TeV domain on the one hand, and in the submm-mm domain on the other hand. These observations concern the specific cases of supernova remnants interacting with molecular cloud complexes, that have long been suspected to be ideal laboratories to study in situ cosmic ray acceleration and diffusion. Indeed, enhanced gamma-ray emission from neutral pion decay, as well as enhanced ionization (both by at least one order of magnitude with respect to average galactic values) have been observed in several regions of massive star formation housing supernova remnants interacting with molecular cloud complexes. This paper summarizes the main physical and chemical processes at work, as well as recent observations, that further support the paradigm of cosmic ray acceleration by supernova remnants all the way from the MeV domain up to several tens of TeV, although much work remains to be done to understand cosmic ray penetration and diffusion inside and around molecular clouds, and reveal the actual spectrum of the accelerated cosmic rays." @default.
- W4293492988 created "2022-08-29" @default.
- W4293492988 creator A5015187914 @default.
- W4293492988 creator A5038847773 @default.
- W4293492988 date "2015-10-07" @default.
- W4293492988 modified "2023-09-27" @default.
- W4293492988 title "Observations of supernova remnants and molecular clouds from the mm to the gamma-ray domain: bridging low and high energy cosmic rays" @default.
- W4293492988 doi "https://doi.org/10.48550/arxiv.1510.02102" @default.
- W4293492988 hasPublicationYear "2015" @default.
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