High-energy Neutrino Emission from a Radiatively Inefficient Accretion Flow with a Three-dimensional General Relativistic Magnetohydrodynamic Simulation
The high-energy particle production in the accretion flow onto black holes can be key physics to explain the high-energy neutrino background. While the single-zone approximation has been commonly adopted in studies of the high-energy neutrino emission around black holes, the effects of the global pl...
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| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
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| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/adee96 |
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