Title: Dark matter in dwarf galaxies,
Abstract: Although the cusp-core controversy for dwarf galaxies is seen as a problem, I
argue that the cored central profiles can be explained by flattened cusps
because they suffer from conflicting measurements and poor statistics and
because there is a large number of conventional processes that could have
flattened them since their creation, none of which requires new physics. Other
problems, such as "too big to fail", are not discussed.