hole in the extremal vanishing horizon (EVH) limit. Knowing the fact that geodesics
equations on Myers–Perry black hole are integrable in ellipsoidal coordinates, we take the
near horizon limit in this coordinate system and obtain the near horizon EVH geometry and
its Killing tensors. We explicitly show that geodesics equations are integrable on the near
horizon EVH geometry ofMyers–Perry and compute the constants of motion. The resultant …