Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

A prototype hybrid mode cavity for heterodyne axion detection

Journal Article · · Nucl.Instrum.Meth.A
In the heterodyne approach to axion detection, axion dark matter induces transitions between two modes of a microwave cavity, resulting in a parametrically enhanced signal power. We describe the fabrication and characterization of a prototype normal conducting cavity specifically optimized for heterodyne detection. Corrugations on the cavity walls support linearly polarized hybrid modes which maximize the signal power while strongly suppressing noise. We demonstrate tuning mechanisms which allow one mode frequency to be scanned across a 4 MHz range, while suppressing cross-coupling noise by at least 80 dB. A future superconducting cavity with identical geometry to our prototype would have the potential to probe orders of magnitude beyond astrophysical bounds.
Research Organization:
Arizona State U.; CERN; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Geneva U., CAP; Geneva U., Dept. Theor. Phys.; IPhT, Saclay; LPENS, Paris; Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); UC, Berkeley
Sponsoring Organization:
US Department of Energy
Grant/Contract Number:
89243024CSC000002
OSTI ID:
2572657
Report Number(s):
FERMILAB-PUB-25-0465-PPD; oai:inspirehep.net:2944561; arXiv:2507.07173
Journal Information:
Nucl.Instrum.Meth.A, Journal Name: Nucl.Instrum.Meth.A Vol. 1088
Country of Publication:
United States
Language:
English

Similar Records

Cavity Microwave Searches for Cosmological Axions
Book · Sun Jan 21 23:00:00 EST 2007 · OSTI ID:940485

Axion searches with two superconducting radio-frequency cavities
Journal Article · Thu Jul 08 20:00:00 EDT 2021 · Journal of High Energy Physics (Online) · OSTI ID:1764071

QSHS: an axion dark matter resonant search apparatus
Journal Article · Sun Oct 05 20:00:00 EDT 2025 · New Journal of Physics · OSTI ID:3019697

Related Subjects