Neutrino science in multipurpose dark matter detectors

Direct dark matter detection experiments will soon be sensitive to neutrinos from astrophysical sources, including the Sun, the atmosphere, and supernova. This sets an important benchmark for these experiments, and opens up a new window in neutrino physics and astrophysics. I will discuss the physics and astrophysics that can be extracted from the detection of these neutrinos, and highlight how this signal is complementary to accelerator and reactor-based experiments which study neutrinos over the same energy range.