Abstract
In this paper, we establish a link between a “curvature inheritance symmetry" of a semi-Riemannian
manifold and a class of almost Ricci solitons(ARS). In support of this link we present three
mathematical models of conformally flat ARS-manifolds. As an application to relativity, by
investigating the kinematic and dynamic properties of ARS-spacetimes we present a physical
model of three classes (namely, shrinking, steady and expanding) of perfect fluid solutions
for ARS-spacetimes and prove the existence of a family of totally umbilical ARS Einstein
hypersurfaces of a GRW-spacetime. Finally, we propose two open problems for further study.