The perturbation of azimuthal alpha-alpha correlations by many-body Co
ulomb interactions with other emitted particles is investigated. Indiv
idual emissions are simulated by modeling instantaneous emission from
the surface of a hot rotating gas. Upon emission, the particle traject
ories are calculated by means of classical calculations which incorpor
ate the many-body Coulomb interaction between the emitted particles an
d the emitting source. For high-multiplicity events, the initial azimu
thal correlation between emitted cu particles can be attenuated by fin
al-state Coulomb interactions. The effect is most pronounced for cu pa
rticles emitted close to the barrier, but it appears of ruiner importa
nce for ct particles emitted at large relative angles and at energies
well above the Coulomb barrier.