Abstract
Thermal evolution of hadronic resonance matter in ultrarelativistic nucleus-nucleus col lisions is studied in the framework of cascade models. We investigate the role of higher baryonic resonances during the time evolution in (p, T) diagram of hot and dense hadronic matter at AGS energies. Although final hadronic spectra do not strongly depend on the number of higher resonances included in the calculation, it is shown that they prevent the temperature from going beyond 200 MeV.
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