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New Results from HAYSTAC's Phase II Operation with a Squeezed State Receiver

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arxiv 2301.09721 v2 pith:PULWXHLM submitted 2023-01-23 hep-ex physics.ins-det

classification hep-exphysics.ins-det
keywords searchaxionsexperimenthaystacmassesoperationreceiversqueezed
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

A search for dark matter axions with masses $>10 \mu eV/c^{2}$ has been performed using the HAYSTAC experiment's squeezed state receiver to achieve sub-quantum limited noise. This report includes details of the design and operation of the experiment previously used to search for axions in the mass ranges $16.96-17.12$ and $17.14-17.28 \mu eV/c^{2}$($4.100-4.140$GHz) and $4.145-4.178$GHz) as well as upgrades to facilitate an extended search at higher masses. These upgrades include improvements to the data acquisition routine which have reduced the effective dead time by a factor of 5, allowing for the new region to be scanned $\sim$1.6 times faster with comparable sensitivity. No statistically significant evidence of an axion signal is found in the range $18.44-18.71\mu eV/c^{2}$($4.459-4.523$GHz), leading to an aggregate upper limit exclusion at the $90\%$ level on the axion-photon coupling of $2.06\times g_{\gamma}^{KSVZ}$.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Catalogues of Cosmologically Self-Consistent Hadronic QCD Axion Models

    hep-ph 2024-12 conditional novelty 7.0 of 10

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  3. Exploration of new experimental strategies for the detection of ultralight dark matter : laboratory searches on ground and in space

    hep-ph 2024-11 conditional novelty 6.0 of 10

    The thesis derives detailed theoretical sensitivities for several ultralight dark matter detection schemes, including a corrected dish-antenna model showing that focused power is much lower than previously assumed.

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