and convective angular momentum fluxes respectively that define as follow: $$J_{vis}=-r^{3}\nu
\Sigma\frac{d\Omega}{dr}$$ and $$J_{con}=-\nu_{con} 
\Sigma r^{3\frac{(1+g)}{2}}\frac{d}{dr}(\Omega  r^{3\frac{(1-g)}{2}})$$

where $\nu$ is the kinematic viscosity coefficient and formalized by Shakura & Sunyaev (1973) as: $$\nu=\alpha c_{s}H$$ where $\alpha$ is a constant less than unity that has called the viscous parameter. Also we have formalized all of the turbulence in our system like convective diffusion and resistivity similar to viscosity turbulence. So, $$\nu_{con}=\alpha_{c} c_{s}H$$ where $\alpha_{c}$ is the dimensionless convective parameter and we get it according the mixing length theory and $g$ is an index for determining the condition for angular momentum transportations. There are several possibilities for transporting of angular momentum by convection (Narayan et al. 2000) which is depends on the magnitude of $g$ parameter. Generally, convection transports angular momentum inward or outward for $g < 0 $ or $g > 0$, respectively while $g = 0$ corresponds to zero angular momentum transportation (Narayan et al. 2000). When $g=1$ the convection behaves like turbulence viscosity but if $g=-\frac{1}{3}$ the convection transport angular momentum inward. In this paper we consider the convective angular momentum flux as: $$J_{con}=-r\nu_{con}
\Sigma\frac{d}{dr}(r^{2}\Omega)$$ where is correspond to $g=-\frac{1}{3}$ and represents that the convective angular momentum flux is 