  Solar neutrinos induce elastic neutrino-electron scattering in dark matter
direct detection experiments, resulting in detectable event rates at current
facilities. We analyze recent data from the XENONnT, LUX-ZEPLIN, and PandaX-4T
experiments and we derive stringent constraints on several $U(1)'$ extensions
of the Standard Model, accommodating new neutrino-electron interactions. We
provide bounds on the relevant coupling and mass of light vector mediators for
a variety of models, including the anomaly-free $B-L$ model, lepton
flavor-dependent interactions like $L_\alpha - L_{\beta}$, $B-2L_e - L_{\mu,
\tau}$, $B-3L_\alpha$, and $B+2L_\mu +2 L_{\tau}$ models. We compare our
results with other limits obtained in the literature from both terrestrial and
astrophysical experiments. Finally, we present forecasts for improving current
bounds with a future experiment like DARWIN.
