  Axino arises in supersymmetric versions of axion models and is a natural
candidate for cold or warm dark matter. Here we revisit axino dark matter
produced thermally and non-thermally in light of recent developments. First we
discuss the definition of axino relative to low energy axion one for several
KSVZ and DFSZ models of the axion. Then we review and refine the computation of
the dominant QCD production in order to avoid unphysical cross-sections and,
depending on the model, to include production via SU(2) and U(1) interactions
and Yukawa couplings.
