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Searches for New Particles, Dark Matter, and Gravitational Waves with SRF Cavities

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arxiv 2203.12714 v1 pith:YMGUDMQ2 submitted 2022-03-23 hep-ph hep-ex

Searches for New Particles, Dark Matter, and Gravitational Waves with SRF Cavities

classification hep-ph hep-ex
keywords cavitiesphysicssearchesacceleratordarkgravitationalhighincluding
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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This is a Snowmass white paper on the utility of existing and future superconducting cavities to probe fundamental physics. Superconducting radio frequency (SRF) cavity technology has seen tremendous progress in the past decades, as a tool for accelerator science. With advances spear-headed by the SQMS center at Fermilab, they are now being brought to the quantum regime becoming a tool in quantum science thanks to the high degree of coherence. The same high quality factor can be leveraged in the search for new physics, including searches for new particles, dark matter, including the QCD axion, and gravitational waves. We survey some of the physics opportunities and the required directions of R&D. Given the already demonstrated integration of SRF cavities in large accelerator systems, this R&D may enable larger scale searches by dedicated experiments.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Qubit Noise Sensing via Induced Photon Loss in a Superconducting Cavity

    quant-ph 2026-03 unverdicted novelty 7.0

    A cavity-based method converts qubit frequency noise into measurable photon loss, validated with injected noise and yielding an upper bound of 5e3 Hz²/Hz at 508 MHz.

  2. Quantum sensing of high-frequency gravitational waves with ion crystals

    gr-qc 2025-12 unverdicted novelty 6.0

    Ion crystals detect high-frequency gravitational waves via resonant drumhead mode excitation and spin entanglement for beyond-SQL readout, with sensitivity scaling with crystal size.

  3. The SKAO Pulsar Timing Array

    astro-ph.IM 2026-07 accept novelty 3.5

    An SKAO PTA with ~174 millisecond pulsars can dominate nanohertz GW sensitivity within four years and enable continuous-wave detections plus anisotropy maps of the gravitational-wave background.