Direct dark matter detection experiments will soon be able to observe solar neutrinos. Although this might limit their capability to search for dark matter particles, it offers a unique opportunity to probe new physics in the neutrino sector. In this talk I will show that, due to their sensitivity to neutrino-electron and neutrino-nucleus scattering, they will be particularly useful to explore the parameter space of general non-standard neutrino interactions (NSI), as well as some scenarios with sterile neutrinos. This offers a complementary view to that of spallation sources and neutrino oscillation experiments. This talk is based on arXiv:2302.12846 and arXiv:2307.05176.
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Meeting ID: 954 4985 9404