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.
Conse- quently, uniform sampling across numerical time steps yields severe data redundancy during quiescent phases and drastically undersamples structurally rapid transi- tions
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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.