Abstract
The orbital velocity profile around the Kerr black holes has a non-monotonic radial behavior in the Locally Nonrotating Frames (LNRF). Using Mathisson- Papapetrou- Dixon equation for a massive spinning particle, again this maximum-minimum feature has been shown by considering the linear spin approximation. Also the spin of black holes and absolute value of particle's spin have an important rule in Aschenbach effect.
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