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The experiment is part of a global effort to study CEνNS,[4][5]a process important for understanding neutrino properties, testing the Standard Model, and supporting research in related fields such as dark matter detection.[6]
Background and scientific aims
CEνNS is a process predicted by the Standard Model, in which a neutrino scatters coherently off an entire atomic nucleus, producing a small nuclear recoil.[6] First predicted in 1974[7], CEνNS was observed for the first time in 2017, when the COHERENT experiment reported the first detection at a spallation neutron source.[8]
Detecting CEνNS using reactor neutrinos[9] is more challenging due to their low energies[10], which produce recoil signals on the order of tens to hundreds of electronvolts[11] due to the low energy of reactor antineutrinos. Achieving sensitivity to these small signals requires detectors with extremely low energy thresholds and careful suppression of backgrounds from cosmic rays and environmental radiation.[2]
NUCLEUS is designed to address this challenge by deploying ultra-sensitive cryogenic calorimeters just 72 meters[1] from a 4.25 GWth commercial reactor core at the Chooz nuclear power plant.[1] This proximity to the core provides a high flux of low-energy antineutrinos.
The experiment seeks to confirm CEνNS at reactor energies and open paths toward new physics searches, including neutrino magnetic moments, sterile neutrinos, and non-standard interactions.
The scientific objectives of NUCLEUS include:
Measuring the CEνNS cross-section at reactor neutrino energies, which are lower than those accessible at spallation sources;
Advancing cryogenic detector technologies capable of operating at sub-keV thresholds for rare-event searches, including CEνNS and low-mass dark matter.[12]
The detectors are designed to measure low-energy nuclear recoils and the aim is for thresholds below 100 electronvolts.[15] To reduce backgrounds from cosmic rays and environmental radiation, the experiment is located in a dedicated underground experimental hall[16] near the reactor core and employs extensive passive shielding and an active muon veto system.[17]A dilution refrigerator and pulse-tube cryocooler system maintains a stable operating temperature near 10 mK.[18]
The setup is housed in a dedicated cryostat[1] at the Chooz nuclear power plant and is designed to be scalable.
Timeline and Development
NUCLEUS builds on R&D from the CRESST and EDELWEISS collaborations. The experiment began conceptual development in 2016–2017[6] and has since advanced through detector prototyping and infrastructure preparation. Installation at the Chooz nuclear power plant was completed in 2023.[19]
In 2023, the collaboration reported a major milestone with the observation of a nuclear recoil peak at the 100 eV scale induced by neutron capture in the detector material.[20] This result demonstrates the detector's ability to operate at the energy threshold needed for CEνNS.[21][22]
The experiment is currently in commissioning[19], with data taking expected to begin in full operation phases in 2025.[19]
It shares detector R&D efforts with projects such as CRESST, EDELWEISS, and the BULLKID R&D program, which explores kinetic inductance detectors (KIDs) as a future path to ultralow-threshold CEvNS and dark matter detection.
^Kaznacheeva, Margarita; Schäffner, Karoline (2024). "Scintillating low-temperature calorimeters for direct dark matter search". Journal of Advanced Instrumentation in Science. arXiv:2406.12887. doi:10.31526/jais.2024.514.
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