  We review recent developments in the use of renormalization group (RG)
methods in low-energy nuclear physics. These advances include enhanced RG
technology, particularly for three-nucleon forces, which greatly extends the
reach and accuracy of microscopic calculations. We discuss new results for the
nucleonic equation of state with applications to astrophysical systems such as
neutron stars, new calculations of the structure and reactions of finite
nuclei, and new explorations of correlations in nuclear systems.
