Abstract
We report here several technical improvements to the HAYSTAC (Haloscope at Yale Sensitive To Axion Cold dark matter) that have improved operational efficiency, sensitivity, and stability.
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Acknowledgements
This work was supported by the National Science Foundation, under grants PHY-1362305 and PHY-1607417, by the Heising-Simons Foundation under grants 2014-181, 2014-182, and 2014-183, and by Yale University. HAYSTAC is a collaboration between U.C. Berkeley, Colorado University/JILA, and Yale.
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Zhong, L., Brubaker, B.M., Cahn, S.B., Lamoreaux, S.K. (2018). Recent Technical Improvements to the HAYSTAC Experiment. In: Carosi, G., Rybka, G., van Bibber, K. (eds) Microwave Cavities and Detectors for Axion Research. Springer Proceedings in Physics, vol 211. Springer, Cham. https://doi.org/10.1007/978-3-319-92726-8_12
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DOI: https://doi.org/10.1007/978-3-319-92726-8_12
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