Cosmological comoving behavior of the configurational entropy
arXiv:1908.04095 · doi:10.1016/j.physletb.2019.07.028
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, , of the FRW flat universe. Such a circumstantial comoving behavior shows that the CE evolves with for fermionic and bosonic radiation and with 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 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.
arXiv comment06 pages, 03 figs
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