Clarity through the neutrino fog: constraining new forces in dark matter detectors

dc.contributor.authorBlanco-Mas, Pabloen
dc.contributor.authorColoma, Pilaren
dc.contributor.authorHerrera, Gonzaloen
dc.contributor.authorHuber, Patricken
dc.contributor.authorKopp, Joachimen
dc.contributor.authorShoemaker, Ian M.en
dc.contributor.authorTabrizi, Zahraen
dc.date.accessioned2025-08-11T13:31:33Zen
dc.date.available2025-08-11T13:31:33Zen
dc.date.issued2025-08-06en
dc.date.updated2025-08-10T03:17:45Zen
dc.description.abstractThe PandaX-4T and XENONnT experiments present indications of Coherent Elastic Neutrino Nucleus Scattering (CEνNS) from 8B solar neutrinos at 2.6σ and 2.7σ, 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.en
dc.description.versionPublished versionen
dc.format.mimetypeapplication/pdfen
dc.identifier.citationJournal of High Energy Physics. 2025 Aug 06;2025(8):43en
dc.identifier.doihttps://doi.org/10.1007/JHEP08(2025)043en
dc.identifier.urihttps://hdl.handle.net/10919/137281en
dc.language.isoenen
dc.rightsCreative Commons Attribution 4.0 Internationalen
dc.rights.holderThe Author(s)en
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en
dc.titleClarity through the neutrino fog: constraining new forces in dark matter detectorsen
dc.title.serialJournal of High Energy Physicsen
dc.typeArticle - Refereeden
dc.type.dcmitypeTexten

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