Erratum: Cosmic-ray nuclei, antiprotons and gamma-rays in the galaxy: a new diffusion model

By Carmelo Evoli, D. Gaggero, D. Grasso, L. Maccione. Journal of Cosmology and Astroparticle Physics, 2008

221 citations recorded by the source corpus.

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Subfields: Atmospheric Science, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/189e451eef771d3a7f47e7f1c7db53c98c61b497

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In Nuclear and High Energy Physics

1. Olivier Mattelaer
2. Fabio Maltoni
3. Mihailo Backovic
4. U. Firenze
5. E. Amato
6. Gopolang Mohlabeng
7. Gran Sasso Science Institute
8. P. S. A. A. D. Arcetri

Citations in the corpus

• Cosmic ray transport in the Galaxy: A review (2017, background): “In fact Evoli et al. (2015); Giesen et al. (2015) find that present data are still marginally compatible with the standard model once the uncertainties in the cross section for p̄ production and in CR transport are taken into account.”
• MadDM v.3.0: A comprehensive tool for dark matter studies (2018, methodology): “3 If MadDM is set on the ‘precise’ running mode both positrons and anti-protons fluxes are computed via the CR propagation code DRAGON [26].”