Thermodynamical Properties and Quasi-localized Energy of the Stringy Dyonic Black Hole Solution

Abstract

In this article, we calculate the heat flux passing through the horizon $.\mathbf{TS}{|}_{r_h}$ and the difference of energy between the Einstein and Møller prescription within the region $\mathcal{M}$, in which is the region between outer horizon ${\mathcal{H}}_{+}$ and inner horizon ${\mathcal{H}}_{-}$, for the modified GHS solution, KLOPP solution and CLH solution. The formula . E_{\rm Einstein}|_{\cal M} = . E_{\rm Møller}|_{\cal M} - \sum_{\partial {\cal M}} {\bf TS}$ is obeyed for the mGHS solution and the KLOPP solution, but not for the CLH solution. Also, we suggest a RN-like stringy dyonic black hole solution, which comes from the KLOPP solution under a dual transformation, and its thermodynamical properties are the same as the KLOPP solution.