Spectral Shape of Galactic Cosmic Rays: Modeling and Implications on Diffusive Gamma-Ray Emission
L.E. Espinosa Castro*,
L.E. Espinosa Castro,
F.L. Villante,
V. Vecchiotti,
C. Evoli and
G. Pagliaroli*: corresponding author
Pre-published on:
September 23, 2025
Published on:
—
Abstract
We model the hadronic gamma-ray production in the Galaxy using an updated phenomenological description of the cosmic ray spectra and different Galactic gas templates. We find a persistent discrepancy in both normalization and spectral shape between the predicted gamma-ray flux and observations by LHAASO. We conclude that the local cosmic-ray proton flux measured by LHAASO overshoots the Galactic gamma-ray emission observed in the TeV-PeV sky, calling for a revision of current cosmic ray models.
DOI: https://doi.org/10.22323/1.501.0640
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