A holographic model for closed strings and Kolmogorov-Volkoff black holes

Recently the Kolmogorov-Volkoff (KV) black hole concept was introduced by the authors of the black hole solution to Einstein-Maxwell theory. In this paper, we show that the Kolmogorov-Volkoff (KV) black hole can be constructed in the presence of a cosmological constant. The proposed solution includes a non-thermal horizon which is a two dimensional boundary-like structure. The solution is obtained by a non-perturbative solution to the Einstein-Maxwell theory. Because the solution is in the presence of a cosmological constant, a Kolmogorov-Volkoff (KV) black hole can also be constructed. The proposed solution is based on a non-perturbative solution to the relativistic theory. We prove that the proposed solution is in the presence of a cosmological constant.