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\section{Models}  You In this paper we will consider the "Running FLRW" model introduced in \cite{Grande_2011}.  In this model the value of the Cosmological Constant (CC) is seen as an effective quantity whose value  can get started evolve with the expansion of the universe.  This model also enforces the conservation of matter  by \textbf{double clicking} allowing a cosmological evolution for the gravitational coupling.  In  this text block model we retain the standard model's interpretation of the CC as vacuum energy while considering the reasonable possibility that its energy density might be related to other time-varying cosmological quantities.  This idea has solid roots in fundamental physics but in this paper we will limit our discussion to the introduction the main equations  and begin editing. You can also click notation necessary for our analysis. We refer  the \textbf{Insert} button below reader  to add new block elements. Or you can \textbf{drag the aforementioned literature for a thorough description of the underlying Quantum Field Theory background necessary to justify some choices used in literature  and drop an image} right onto also in  this text. Happy writing! paper.