A short note on Magnetized Black-hole in Non-linear Electrodynamics

We have analyzed the thermodynamic properties of magnetized black-hole in the background of non-linear electrodynamics with two parameters $\beta$ and $\gamma$. We have studied the Bekenstein-Hawking entropy, Hawking temperature, specific heats in two-dimesional surface plots as a function of event horizon ($r_{+}$) and $\gamma$. We showed the variation profiles of the above thermodynamic parameters for $\gamma$ [$0 \rightarrow 1$]. We identified regions of parameters for the possible phase-transitions and the stability of the black-holes.