  The present work investigates the dissipation of configurational entropy in
some of the most widely studied Chaplygin gas models, such as the generalized
Chaplygin gas and the modified Chaplygin gas, and communicate the existence of
a wide range of parameter space which gives rise to a viable dissipation of
configurational entropy, and therefore certifying its time derivative to hit a
minimum at a scale factor which complies with the current observational
constraints on the redshift of transition from a dust to an accelerated
Universe.
