Published November 13, 2025 | Version v1
Journal article

Flux-Tunable Cavity for Dark Matter Detection

  • 1. Fermi National Accelerator Laboratory
  • 2. University of Chicago
  • 3. New York University

Description

Developing a dark matter detector with wide mass tunability is an immensely desirable property, yet, it is challenging due to maintaining strong sensitivity. Resonant cavities for dark matter detection have traditionally employed mechanical tuning, moving parts around to change electromagnetic boundary conditions. However, these cavities have proven challenging to operate in sub-Kelvin cryogenic environments due to differential thermal contraction, low heat capacities, and low thermal conductivities. Instead, we develop an electronically tunable cavity architecture by coupling a superconducting 3D microwave cavity with a dc flux tunable superconducting quantum interference device. With a flux delivery system engineered to maintain high coherence in the cavity, we perform a hidden-photon dark matter search below the quantum-limited threshold. A microwave photon counting technique is employed through repeated quantum nondemolition measurements using a transmon qubit. With this device, we perform a hidden-photon search and constrain the kinetic mixing angle to 𝜖 <8.2 ×10−15 in a tunable band from 5.672 to 5.694 GHz. By coupling multimode tunable cavities to the transmon, wider hidden-photon searching ranges are possible.

Data availability

The data that support the findings of this article are openly available [47], embargo periods may apply.

Additional details

Identifiers

DOI
10.1103/clp9-xc2n
Other
oai:uchicago.tind.io:16645

Funding

Office of High Energy Physics
United States Department of Energy
DE-AC02-07CH11359

UChicago Information

Division(s)
Institutes & Centers, Physical Sciences Division, Pritzker School of Molecular Engineering
Department(s)
Physics
Center(s) or Institute(s)
James Franck Institute, Kavli Institute for Cosmological Physics