First test of a photonic band gap structure for ADMX-HF
Samantha Lewis
Graduate student University of California - Berkeley
Workshop on Microwave Cavities and Detectors for Axion Research Livermore National Laboratory January 13, 2017
First test of a photonic band gap structure for ADMX-HF Workshop on - - PowerPoint PPT Presentation
First test of a photonic band gap structure for ADMX-HF Workshop on Microwave Cavities and Detectors for Axion Research Livermore National Laboratory January 13, 2017 Samantha Lewis Graduate student University of California - Berkeley
Graduate student University of California - Berkeley
Workshop on Microwave Cavities and Detectors for Axion Research Livermore National Laboratory January 13, 2017
Background and motivation
Background and motivation
– Mode crossings reduce scan rate and make some tuning regions effectively unusable
– Lots of design parameters and flexibility
Background and motivation
Background and motivation
Adapted from: Smirnova, et al., J. Appl. Phys., 2002
Disallowed regions Disallowed region
Prototype design
for structural stability
removing multiple periods
roughly 10 GHz
Prototype design
Note: tuning curve for a slightly different lattice
Prototype design
Prototype design
TM010-like mode No TE modes, two TEM modes found with field probes but not S21
Prototype design
Size of “equivalent” cavity
Prototype design
Cavity TM010-like mode
Fixed frequency results
Fixed frequency results
Fixed frequency results
– Likely somewhat due to haphazard setup: poor connection with antennas – Simulation does not include the holes in the endcaps for access ports and the tuning rod axle – Simulation includes absorber outside the structure which we plan to use – Worst case: poor electrical contact within the structure
Discussion and future work
– Take more thorough measurements – Incorporate all features of the design into the simulation
– Verify all three modes are what we expect – Check the flatness of the profile
Discussion and future work
– Requires disassembly and reassembly, allowing for a full cleaning of the structure
– Look for unexpected modes – Study the potential TEM mode crossing – Validate full simulations of the tuning curve – Make a complete mode map
Discussion and future work
Steve Lamoreaux, Ling Zhong, Ben Brubaker, Sid Cahn, Kelly Backes
Karl van Bibber, Maria Simanovskaia, Samantha Lewis, Jaben Root, Saad Al Kenany, Nicholas Rapidis, Isabella Urdinaran
Konrad W. Lehnert, Daniel Palken, William F. Kindel, Maxime Malnou
Gianpaolo Carosi, Tim Shokair