  It has been shown that a functional dependence of the configurational entropy
(CE) density exhibits a cosmological comoving behavior related to the scale
parameter, $a$, of the FRW flat universe. Such a circumstantial comoving
behavior shows that the CE evolves with $a^{-3}$ for fermionic and bosonic
radiation and with $a^{-3/2}$ for non-relativistic fermionic matter. The
results are discussed in the domain of matter and radiation, as well as in a
simplified context of the $\Lambda$CDM cosmology. Our results suggest that the
CE can work as a theoretical driver for particle and nuclear interactions in
the context of large scale cosmic events.
