Interacting holographic Ricci dark energy as running vacuum

Earlier studies have shown that in a two component model of the universe with dark matter and the running vacuum energy, which is phenomenologically a combination of H-2 and H, either eternal deceleration or acceleration is produced in the absence of a hare constant in the density of the running vacuum. In this paper, we have shown that in the interaction scenario, where the interaction between matter and vacuum is introduced through a phenomenological term, the two component model is capable of causing a transition from a prior decelerated to a later accelerated epoch without a bare constant in the running vacuum density. On contrasting the model with the cosmological data, we have found that the interaction coupling constant is small enough for a slow decay of the running vacuum. The model is subjected to dynamical system analysis, which revealed that the end de Sitter phase of the model is a stable one. We did an analysis on the thermal behavior of the system, which shows that the entropy is bounded at the end stage so that the system behaves like an ordinary macroscopic system. Apart from these, we have also performed the state finder diagnostic analysis which implies the quintessence nature of running vacuum and confirms that the model will approach the standard ACDM in the future.