Solar radio emissions and ultralight dark matter

Abstract

Ultralight axions and dark photons are well-motivated dark matter candidates. Inside the plasma, once the mass of ultralight dark matter candidates equals the plasma frequency, they can resonantly convert into electromagnetic waves, due to the coupling between the ultralight dark matter particles and the standard model photons. The converted electromagnetic waves are monochromatic. In this article, we review the development of using radio detectors to search for ultralight dark matter conversions in the solar corona and solar wind plasma.

arXiv comment13 pages, 3 figures. An invited review for the special issue "Solar Radio Emissions" in the journal Universe

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Cited by in corpus (5)

• Searching for Ultralight Dark Matter Conversion in Solar Corona using Low Frequency Array Data
• Fermion Proca Stars: Vector Dark Matter Admixed Neutron Stars
• In Situ Measurements of Dark Photon Dark Matter Using Parker Solar Probe: Going beyond the Radio Window
• Polarization Signals from Axion-Photon Resonant Conversion in Neutron Star Magnetosphere
• Low-frequency radio telescopes sensitivity to light dark matter