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2016

Detecting ultralight axion dark matter wind with laser interferometers

Aoki, Arata, Soda, Jiro

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The ultralight axion with mass around $10^{-22}$ eV is known as a candidate of dark matter.

A peculiar feature of the ultralight axion is oscillating pressure in time, which produces oscillation of gravitational potentials.
Since the solar system moves through the dark matter halo at the velocity of about $v \sim 300 \, \text{km} / \text{s} = 10^{-3}$, there exists axion wind, which looks like scalar gravitational waves for us.
Hence, there is a chance to detect ultralight axion dark matter with a wide mass range by using laser interferometer detectors.

Detecting ultralight axion dark matter wind with laser interferometers · Around

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