First Sub-MeV Dark Matter Search with the QROCODILE Experiment Using Superconducting Nanowire Single-Photon Detectors

We present the first results from the (QROCODILE). The QROCODILE experiment uses a microwire-based superconducting nanowire single-photon detector (SNSPD) as a target and sensor for dark matter scattering and absorption, and is sensitive to energy deposits as low as 0.11 eV. We introduce the experimental configuration and report new world-leading constraints on the interactions of sub-MeV dark matter particles with masses as low as 30 keV. The thin-layer geometry of the system provides anisotropy in the interaction rate, enabling directional sensitivity. In addition, we leverage the coupling between phonons and quasiparticles in the detector to simultaneously constrain interactions with both electrons and nucleons. We discuss the potential for improvements to both the energy threshold and effective volume of the experiment in the coming years.

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Publication Details

Journal
Universität Zürich, ZORA
Published
2025-08-20
DOI
https://doi.org/10.5167/uzh-283325
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
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article

First Sub-MeV Dark Matter Search with the QROCODILE Experiment Using Superconducting Nanowire Single-Photon Detectors

C. Capelli, A. Schilling, C. Koos, Artem Kuzmin et al.
Universität Zürich, ZORA
Dark Matter and Cosmic Phenomena
article

First Sub-MeV Dark Matter Search with the QROCODILE Experiment Using Superconducting Nanowire Single-Photon Detectors

C. Capelli, A. Schilling, C. Koos, Artem Kuzmin, Alexander H. Bismark, A. Kavner, D. Ramírez García, Ilya Charaev, J. Garcia, Severin Nägeli, Titus Neupert, Noah Brugger, Yonit Hochberg, Benjamin V Lehmann, Guy Daniel Hadas, Bjoern Penning, Laura Baudis, Judith K. Hohmann
article en

Abstract

We present the first results from the (QROCODILE). The QROCODILE experiment uses a microwire-based superconducting nanowire single-photon detector (SNSPD) as a target and sensor for dark matter scattering and absorption, and is sensitive to energy deposits as low as 0.11 eV. We introduce the experimental configuration and report new world-leading constraints on the interactions of sub-MeV dark matter particles with masses as low as 30 keV. The thin-layer geometry of the system provides anisotropy in the interaction rate, enabling directional sensitivity. In addition, we leverage the coupling between phonons and quasiparticles in the detector to simultaneously constrain interactions with both electrons and nucleons. We discuss the potential for improvements to both the energy threshold and effective volume of the experiment in the coming years.

Universität Zürich, ZORA
Affordable and clean energy
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Dark Matter and Cosmic Phenomena
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