  The pasta phase in core-collapse supernova matter (finite temperatures and
fixed proton fractions) is studied within relativistic mean field models. Two
different calculations are used for comparison, the Thomas-Fermi (TF) and the
Coexisting Phases (CP) approximations. The effects of including light clusters
in nuclear matter and the densities at which the transitions between pasta
configurations and to uniform matter occur are also investigated. Finally, a
comparison with a finite temperature Skyrme-Hartree-Fock calculation is drawn.
