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.
Mart´ ınez-Mirav´ e and I
2 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 2representative citing papers
The helium flash produces a neutrino burst with a 1.7 MeV line detectable up to almost 3 pc in future facilities, but asteroseismology remains the practical probe for now.
citing papers explorer
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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.
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Detection horizon for the neutrino burst from the stellar helium flash
The helium flash produces a neutrino burst with a 1.7 MeV line detectable up to almost 3 pc in future facilities, but asteroseismology remains the practical probe for now.