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Axion Dark Matter eXperiment: Run 1B Analysis Details

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arxiv 2010.06183 v1 pith:YO5WIVIC submitted 2020-10-13 astro-ph.CO astro-ph.IM

classification astro-ph.COastro-ph.IM
keywords admxanalysisaxiondarkmatterrangedetailsexperiment
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Searching for axion dark matter, the ADMX collaboration acquired data from January to October 2018, over the mass range 2.81--3.31 $\mu$eV, corresponding to the frequency range 680--790 MHz. Using an axion haloscope consisting of a microwave cavity in a strong magnetic field, the ADMX experiment excluded Dine-Fischler-Srednicki-Zhitnisky (DFSZ) axions at 100% dark matter density over this entire frequency range, except for a few gaps due to mode crossings. This paper explains the full ADMX analysis for Run 1B, motivating analysis choices informed by details specific to this run.

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  1. High-Frequency Gravitational Wave Detection with Superconducting Qubits

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    An idealized model shows that Dicke-entangled transmon qubits at the TE212 cavity mode could reach a strain sensitivity of about 5.6e-26 at 5 GHz, scaling as n_q^{-3/4}.

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