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2022

Detecting axion dark matter beyond the magnetoquasistatic approximation

Benabou, Joshua N., Foster, Joshua W., Kahn, Yonatan et al.

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A number of proposals have been put forward for detecting axion dark matter (DM) with grand unification scale decay constants that rely on the conversion of coherent DM axions to oscillating magnetic fields in the presence of static, laboratory magnetic fields.

Crucially, such experiments $\unicode{x2013}$ including ABRACADABRA $\unicode{x2013}$ have to-date worked in the limit that the axion Compton wavelength is larger than the size of the experiment, which allows one to take a magnetoquasistatic (MQS) approach to modeling the axion signal.
We use finite element methods to solve the coupled axion-electromagnetism equations of motion without assuming the MQS approximation.
We show that the MQS approximation becomes a poor approximation at frequencies two orders of magnitude lower than the naive MQS limit.

Detecting axion dark matter beyond the magnetoquasistatic approximation · Around

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