Abstract
The Dark photon as an ultralight dark matter candidate can interact with the standard model particles via kinetic mixing. We propose to search for the ultralight dark photon dark matter using radio telescopes with solar observations. The dark photon dark matter can efficiently convert into photons in the outermost region of the solar atmosphere, the solar corona, where the plasma mass of photons is close to the dark photon rest mass. Because of the strong resonant conversion and benefiting from the short distance between the Sun and the Earth, the radio telescopes can lead the dark photon search sensitivity in the mass range of , corresponding to the frequency 10–1000 MHz. As a promising example, the low-frequency array telescope can reach the kinetic mixing () within 1 (100) h of solar observations. The future experiment square kilometer array phase 1 can reach with 1 h of solar observations.
- Received 9 November 2020
- Revised 1 March 2021
- Accepted 7 April 2021
DOI:https://doi.org/10.1103/PhysRevLett.126.181102
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
Published by the American Physical Society