A quantum-enhanced search for dark matter axions

In dark matter axion searches, quantum uncertainty manifests as a fundamental noise source, limiting the measurement of the quadrature observables used for detection. We use vacuum squeezing to circumvent the quantum limit in a search for a new particle. By preparing a microwave-frequency electromag...

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Veröffentlicht in:arXiv.org 2020-08
Hauptverfasser: Backes, K M, Palken, D A, S Al Kenany, Brubaker, B M, Cahn, S B, Droster, A, Hilton, Gene C, Ghosh, Sumita, Jackson, H, Lamoreaux, S K, Leder, A F, Lehnert, K W, Lewis, S M, Malnou, M, Maruyama, R H, Rapidis, N M, Simanovskaia, M, Singh, Sukhman, Speller, D H, Urdinaran, I, Vale, Leila R, van Assendelft, E C, K van Bibber, Wang, H
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Sprache:eng
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Zusammenfassung:In dark matter axion searches, quantum uncertainty manifests as a fundamental noise source, limiting the measurement of the quadrature observables used for detection. We use vacuum squeezing to circumvent the quantum limit in a search for a new particle. By preparing a microwave-frequency electromagnetic field in a squeezed state and near-noiselessly reading out only the squeezed quadrature, we double the search rate for axions over a mass range favored by recent theoretical projections. We observe no signature of dark matter axions in the combined \(16.96-17.12\) and \(17.14-17.28\space\mu\text{eV}/c^2\) mass window for axion-photon couplings above \(g_{\gamma} = 1.38\times g_{\gamma}^\text{KSVZ}\), reporting exclusion at the 90% level.
ISSN:2331-8422
DOI:10.48550/arxiv.2008.01853