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.
For each sampled star in the population, an evolution- ary survival criterion is first applied
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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.