  The atomic recombination process leads to a softening of the matter equation
of state as reflected by a reduced generalized adiabatic index, with
accompanying heat release. We study the effects of this recombination softening
and reheating of the cosmic plasma on the ionization history, visibility
function, Cold Dark Matter (CDM) transfer function, and the Cosmic Microwave
Background (CMB) spectra. The resulting modifications of the CMB spectrm is
1/10 of WMAP's current error and is comparable to PLANCK's error. Therefore,
this effect should be considered when data with higher accuracy are analysed.
