Stellar atmospheres produce a sub-dominant Galactic diffuse gamma-ray and neutrino background that is negligible at 1 TeV and below IceCube limits but becomes an irreducible local component above 10 TeV.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Galactic Diffuse Gamma-Ray and Neutrino Emission from Cosmic-Ray Interactions in Stellar Atmospheres
Stellar atmospheres produce a sub-dominant Galactic diffuse gamma-ray and neutrino background that is negligible at 1 TeV and below IceCube limits but becomes an irreducible local component above 10 TeV.