Abstract
An analysis of evaporated particles originating from the interaction of 32-GeV positrons with photoemulsion nuclei was performed. The yields of protons, deuterons, tritons, and alpha particles were measured, and the results were compared with evaporation-theory predictions. The energy spectra of protons, deuterons, and tritons agree with a Maxwellian distribution. The excitation energy of photoemulsion nuclei complies with the theoretical estimate for the emission of these particles from the equilibrium state.
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