Agegraphic dark energy cosmology and Quantum loop-correction

In this paper, we extend the agegraphic dark energy model through quantum loop-correction on Einstein–Hilbert action. We investigate the evolution of the equation of state and energy density of proposed agegraphic dark energy for non-interaction and interaction scenarios. Also, the deceleration parameter and square of sound speed of both scenarios are studied and we have shown model is stable classically only for the interaction case. Moreover, considering the interaction scenario shows for the very early universe, this new agegraphic dark energy may treat such as inflation field. © 2022 Elsevier B.V.