Bulletin of the American Physical Society
APS April Meeting 2019
Volume 64, Number 3
Saturday–Tuesday, April 13–16, 2019; Denver, Colorado
Session Y09: Axion II
1:30 PM–3:06 PM,
Tuesday, April 16, 2019
Sheraton
Room: Governor's Square 11
Sponsoring
Unit:
DPF
Chair: LIndley Winslow, Massachusetts Institute of Technology
Abstract: Y09.00003 : A tunable higher-frequency resonant cavity for HAYSTAC*
1:54 PM–2:06 PM
Presenter:
Maria Simanovskaia
(University of California, Berkeley)
Authors:
Maria Simanovskaia
(University of California, Berkeley)
Alex Droster
(University of California, Berkeley)
Karl Albert Van Bibber
(University of California, Berkeley)
Collaboration:
HAYSTAC
HAYSTAC is a dark matter detector that looks for an axion-induced power excess spectrally coincident with the resonance of a microwave cavity immersed in a strong magnetic field. The current HAYSTAC cavity achieves frequency-tunability over the 3.6-5.8 GHz window via its single, off-center tuning rod. Probing higher frequencies, however, introduces unique challenges. In particular, smaller volumes, lower quality factors, and higher densities of intruder modes decrease sensitivity and increase operational complexity. Here, we present the design and initial testing results of a cavity using seven tuning rods for the frequency range 5.5-7.4 GHz. Our seven-rod design will allow HAYSTAC to probe higher axion masses while maintaining axion sensitivity significantly greater than that of the standard design.
*This work was supported under the auspices of the National Science Foundation under grant PHY-1607242 and the Heising-Simons Foundation under grant 2016-044. MS is supported by the Berkeley Fellowship and the National Science Foundation Graduate Research Fellowship Program under Grant No. DGE-1745016.
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