Ultralight axion dark matter search with DANCE
ORAL · Invited
Abstract
Axion and axion-like particles are leading candidates for ultralight dark matter, and there have been enormous efforts to search for their signatures through a variety of experiments and astrophysical observations. Axion may cause a polarization rotation of light through the parity-violating interaction with photons. Recently, we have proposed to search for axion dark matter by enhancing the polarization rotation effect using a bow-tie optical ring cavity [PRL 121, 161301 (2018)]. We have shown that this Dark matter Axion search with riNg Cavity Experiment (DANCE) can improve the sensitivity to axion-photon coupling for axion mass m_a<10^{-10} eV by up to several orders of magnitude, compared with the current best limits. Currently, a prototype experiment DANCE Act-1 is underway at Tokyo to demonstrate the feasibility of the method. In this talk, I will present the principle of DANCE and the status of DANCE Act-1, including our first results from May 2021 run [arXiv:2303.035947].
*This work is supported by JSPS KAKENHI Grant Nos. JP18K13537, JP19H01894, JP19K14702, JP20H04726, JP20H05850, JP20H05854, JP20H05859, JP20J21866, JP22J21087 and JP22J21530, by the Sumitomo Foundation, and by JST PRESTO Grant No. JPMJPR200B.
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Publication: https://doi.org/10.1103/physrevlett.121.161301
https://doi.org/10.1088/1742-6596/1468/1/012032
https://doi.org/10.1088/1742-6596/2156/1/012042
https://doi.org/10.1088/1742-6596/2156/1/012182
https://arxiv.org/abs/2303.03594
Presenters
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Yuta Michimura