First results from the HAYSTAC axion search
Benjamin M. Brubaker

TL;DR
The paper reports the first results from HAYSTAC, a new cryogenic haloscope detector that searches for axion dark matter above 20 μeV, achieving high sensitivity and near-quantum-limited noise performance.
Contribution
It introduces the HAYSTAC detector, details its design and commissioning, and presents the first data analysis setting new limits on axion-photon coupling in a higher mass range.
Findings
Excluded axion models with coupling g_{aγγ} ≥ 2×10^{-14} GeV^{-1} in the 23.55-24.0 μeV range.
Demonstrated total noise approaching the standard quantum limit in a haloscope.
Achieved sensitivity to cosmologically relevant axion masses above previous limits.
Abstract
The axion is a well-motivated cold dark matter (CDM) candidate first postulated to explain the absence of violation in the strong interactions. CDM axions may be detected via their resonant conversion into photons in a "haloscope" detector: a tunable high- microwave cavity maintained at cryogenic temperature, immersed a strong magnetic field, and coupled to a low-noise receiver. This dissertation reports on the design, commissioning, and first operation of the Haloscope at Yale Sensitive to Axion CDM (HAYSTAC), a new detector designed to search for CDM axions with masses above . I also describe the analysis procedure developed to derive limits on axion CDM from the first HAYSTAC data run, which excluded axion models with two-photon coupling , a factor of 2.3 above the benchmark KSVZ model, over…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies · Cosmology and Gravitation Theories
