\begin{document}$ N = L^{D-2}/G,\; \mu = GTI_D/L^{D-2} $\end{document}, where G is the variable Newton constant, \begin{document}$ I_D $\end{document} is the Euclidean action, and L is a constant length scale. In the cases without a cosmological constant, i.e., the Myers-Perry black holes, the physical mass and the intensive variables can be expressed as explicit macro state functions in the extensive variables in a simple and compact form, which allows for an analytical calculation of the heat capacity. The results indicate that the Myers-Perry black holes with zero, one, and k equal rotation parameters are all thermodynamically unstable."> Thermodynamics for higher dimensional rotating black holes with variable Newton constant -
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