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We present a pseudo-Newtonian potential for accretion disk modeling aroundthe rotating black holes. This potential can describe the general relativisticeffects on accretion disk. As the inclusion of rotation in a proper way is veryimportant at an inner edge of disk the potential is derived from the Kerrmetric. This potential can reproduce all the essential properties of generalrelativity within 10% error even for rapidly rotating black holes.Comment: 5 Latex pages including 1 figure. Version to appear in Astrophysical  Journal, V-581, N-1, December 10, 200

Description of Pseudo‐Newtonian Potential for the Relativistic Accretion Disks around Kerr Black Holes