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Hunting Axion Dark Matter with Protoplanetary Disk Polarimetry
Tomohiro Fujita1,2, Ryo Tazaki3, Kenji Toma3,4
1Department of Physics, Kyoto University, Kyoto, 606-8502, Japan.
Abstract:
We find that the polarimetric observations of protoplanetary disks are useful to search for ultralight axion dark matter. Axion dark matter predicts the rotation of the linear polarization plane of propagating light, and protoplanetary disks are ideal targets to observe it. We show that a recent observation puts the tightest constraint on the axion-photon coupling constant for an axion mass m≲10^{-21} eV.
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