First Search for Light Dark Matter in the Neutrino Fog with XENONnT

Abstract

We search for dark matter (DM) with a mass [3,12] $\mathrm{GeV}/c^2$ using an exposure of 3.51 $\mathrm{t}\times \mathrm{y}$ with the XENONnT experiment.We consider spin-independent DM-nucleon interactions mediated by a heavy or light mediator, spin-dependent DM-neutron interactions, momentum-dependent DM scattering, and mirror DM. Using a lowered energy threshold compared to the previous WIMP search, a blind analysis of [0.5, 5.0] $\mathrm{keV}$ nuclear recoil events reveals no significant signal excess over the background. XENONnT excludes spin-independent DM-nucleon cross sections $>2.5\times 10^{-45}{\mathrm{cm}}^2$ at $90\%$ confidence level for 6 $\mathrm{GeV}/c^2$ DM. In the considered mass range, the DM sensitivity approaches the 'neutrino fog', the limitation where neutrinos produce a signal that is indistinguishable from that of light DM-xenon nucleus scattering.

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