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astro-ph.HE2022
Diffuse -ray emission in Cygnus X: Comments to Yan & Pavaskar
Ottavio Fornieri, Heshou Zhang
It has been pointed out in arXiv:2211.17057 that our recent (published) paper might be revised, due to an incorrect evaluation of the diffusion coefficients, , employed in th…
astro-ph.HE2022★ 1 cited
MHD decomposition explains diffuse -ray emission in Cygnus X
Ottavio Fornieri, Heshou Zhang
Cosmic-ray (CR) diffusion is the result of the interaction of such charged particles against magnetic fluctuations. These fluctuations originate from large-scale turbulence cascadi…