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· 2021 · arXiv 2011.05211

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2026 1

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Solar Axions from Nuclear Transitions

hep-ph · 2026-05-22 · unverdicted · novelty 3.0

Solar axion fluxes from 57Fe and 83Kr nuclear transitions differ by three orders of magnitude, yielding stronger constraints on |g_aN^eff × g_aγγ| and g_aγγ vs. m_a from Chandrayaan-2 XSM data for iron.

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  • Solar Axions from Nuclear Transitions hep-ph · 2026-05-22 · unverdicted · none · ref 62

    Solar axion fluxes from 57Fe and 83Kr nuclear transitions differ by three orders of magnitude, yielding stronger constraints on |g_aN^eff × g_aγγ| and g_aγγ vs. m_a from Chandrayaan-2 XSM data for iron.