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In the present paper, the pasta phase is studied at finite temperatureswithin a Thomas-Fermi (TF) approach. Relativistic mean field models, both withconstant and density-dependent couplings, are used to describe this frustratedsystem. We compare the present results with previous ones obtained within aphase-coexistence description and conclude that the TF approximation gives riseto a richer inner pasta phase structure and the homogeneous matter appears athigher densities. Finally, the transition density calculated within TF iscompared with the results for this quantity obtained with other methods.

Warm pasta phase in the Thomas-Fermi approximation