Abstract
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 ΛCDM 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.
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