  In this paper we study the relativistic bulk tensor, shear tensor and the
shear stress viscosity of the relativistic accretion disks around the rotating
black holes. we calculate all non-zero components of the bulk tensor, shear
tensor and shear stress viscosity in the equatorial plan in the BLF. We obtain
the relations of the relativistic bulk tensor, shear tensor and shear stress
viscosity in the terms of components of four velocity and derivatives,
Christoffel symbols and metric components. To see the behaviorr of the
components of relativistic bulk tensor, shear tensor and shear stress
viscosity, we introduce a radial form for the radial component of the four
velocity in the LNRF then all components of the bulk tensor, shear tensor and
shear stress viscosity are derived in BLF. Figures of non-zero components of
the bulk tensor, shear tensor and shear stress viscosity are shown for some
states. The importance and influence of the relativistic bulk viscosity in the
accretion disks around the rotating black holes are studied in this paper.
