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Clarity through the Neutrino Fog: Constraining New Forces in Dark Matter Detectors

Clarity through the Neutrino Fog: Constraining New Forces in Dark Matter Detectors

来源:Arxiv_logoArxiv
英文摘要

The PANDAX-4T and XENONnT experiments present indications of Coherent Elastic Neutrino Nucleus Scattering (CE$ν$NS) from ${}^{8}$B solar neutrinos at 2.6$σ$ and 2.7$σ$, respectively. This constitutes the first observation of the neutrino "floor" or "fog", an irreducible background that future dark matter searches in terrestrial detectors will have to contend with. Here, we first discuss the contributions from neutrino-electron scattering and from the Migdal effect in the region of interest of these experiments, and we argue that they are non-negligible. Second, we make use of the recent PANDAX-4T and XENONnT data to derive novel constraints on light scalar and vector mediators coupling to neutrinos and quarks. We demonstrate that these experiments already provide world-leading laboratory constraints on new light mediators in some regions of parameter space.

Pilar Coloma、Gonzalo Herrera、Patrick Huber、Joachim Kopp、Ian M. Shoemaker、Zahra Tabrizi、Pablo Blanco-Mas

物理学

Pilar Coloma,Gonzalo Herrera,Patrick Huber,Joachim Kopp,Ian M. Shoemaker,Zahra Tabrizi,Pablo Blanco-Mas.Clarity through the Neutrino Fog: Constraining New Forces in Dark Matter Detectors[EB/OL].(2025-08-01)[2025-08-18].https://arxiv.org/abs/2411.14206.点此复制

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