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Membrane-less phonon trapping and resolution enhancement in optical microwave kinetic inductance detectors

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arxiv 2204.13669 v1 pith:GAZQGPSL submitted 2022-04-28 astro-ph.IM physics.ins-det

classification astro-ph.IMphysics.ins-det
keywords phonondetectorsenergyinductancekineticmicrowavemkidsphoton
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abstract

Microwave Kinetic Inductance Detectors (MKIDs) sensitive to light in the ultraviolet to near-infrared wavelengths are superconducting micro-resonators that are capable of measuring photon arrival times to microsecond precision and estimating each photon's energy. The resolving power of non-membrane MKIDs has remained stubbornly around 10 at 1 $\mu$m despite significant improvements in the system noise. Here we show that the resolving power can be roughly doubled with a simple bilayer design without needing to place the device on a membrane, avoiding a significant increase in fabrication complexity. Based on modeling of the phonon propagation, we find that the majority of the improvement comes from the inability of high energy phonons to enter the additional layer due to the lack of available phonon states.

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  1. Dark Matter-Electron Detectors for Dark Matter-Nucleon Interactions

    hep-ph 2024-12 conditional novelty 7.0 of 10

    Electron-sensitive superconducting detectors are simultaneously sensitive to dark matter-nucleon interactions, yielding new bounds on MeV-scale hadrophilic dark matter.

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