Stripped-envelope supernovae enable QCD axion detection to masses around 10^{-4} eV via gamma-ray signals from conversion in progenitor magnetic fields.
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Turbulent magnetic fields enhance axion-photon conversion signals from supernovae, improving limits on axion-proton and axion-photon couplings by up to two orders of magnitude.
The study calculates sensitivity of space- and Moon-based radio telescopes to resonant light dark matter conversion in solar system targets, finding encouraging prospects for dark photon searches with the Sun and axion-like particle conversion in Jupiter's magnetosphere.
citing papers explorer
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Stripped-Envelope Supernovae for QCD Axion Detection
Stripped-envelope supernovae enable QCD axion detection to masses around 10^{-4} eV via gamma-ray signals from conversion in progenitor magnetic fields.
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Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion
Turbulent magnetic fields enhance axion-photon conversion signals from supernovae, improving limits on axion-proton and axion-photon couplings by up to two orders of magnitude.
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Low-frequency radio telescopes sensitivity to light dark matter
The study calculates sensitivity of space- and Moon-based radio telescopes to resonant light dark matter conversion in solar system targets, finding encouraging prospects for dark photon searches with the Sun and axion-like particle conversion in Jupiter's magnetosphere.