Modelling the current accelerated expansion of the Universe with Holographic Dark Energy

In this work we explore a Holographic Dark Energy Model in a flat Friedmann-Lemaitre-Robertson-Walker Universe, which contains baryons, radiation, cold dark matter and dark energy within the framework of General Relativity. Furthermore, we consider three types of phenomenological interactions in the dark sector. With the proposed model we obtained the algebraic expressions for the cosmological parameters of our interest: the deceleration and coincidence parameters. Likewise, we graphically compare the proposed model with the $\Lambda$CDM model.