  The Cornell potential can be derived from a recently proposed non-local
extension of Abelian electrodynamics. Non-locality can be alternatively
described by an extended charge distributions in Maxwell electrodynamics. We
state that in these models the energy momentum tensor necessarily requires the
presence of the interaction term between the field and the charge itself. We
show that this extended form of energy momentum tensor leads to an exact
solution of the Einstein equations describing a charged AdS black hole. We
refer to it as the "Cornell black hole"(CBH). Identifying the effective
cosmological constant with the pressure of Van der Waals fluid, we study the
gas-liquid phase transition and determine the critical parameters.
