Spectral evolution of PKS 2155-304 observed with BeppoSAX during an activegamma-ray phase

We present the results of BeppoSAX observations of PKS 2155 - 304 during an intense gamma-ray flare. The source was in a high X-ray state. A temporal analysis of the data reveals a tendency of the amplitude of variations to i ncrease with energy and the presence of a soft lag with a timescale of the order 10(3) s. A curved continuum spectrum, with no evidence of spectral fe atures, extends up to similar to 50 keV, while there is indication of a fla tter component emerging at higher energies, consistent with the interpretat ion of the broadband spectral energy distribution (SED) due to synchrotron self-Compton emission from a single region. Notably, the fitting of the SED with such a model is consistent with an interpretation of the detected sof t lag due to radiative cooling, supporting the idea that radiation losses p lay an important role in variability. The observed shifts of the SED peaks between the lowest and highest flux levels can be accounted for by an incre ase of the "break" energy in the relativistic particle spectrum. The model predicts emission at TeV energies in good agreement with the recently repor ted detection.