A fluid in which the viscous stresses taken place from its flow at all the point are linearly proportional to the rate of change in its deformation over time is called Newtonian fluid. Newtonian fluid explains the relationship between the shear rate and the shear stress is linear with the proportionality constant, which is to be referred as the coefficient of viscosity. Non-Newtonian fluid is a fluid where the properties of fluid flow are not similar with Newtonian fluid. In Newtonian fluids, the viscosity of fluid is dependent on the shear rate history. In the non-Newtonian fluid, the relationship between the shear stress and the shear rate is different and can even be time dependent. A coefficient of viscosity cannot be constant in all cases.
…show more content…
Energy equation
Equation of energy for an electrically conducting, viscous incompressible fluid is ρC_P [∂T/∂t+(q ̅.∇)T]=K∇^2 T+μ(1+1/γ) (1.3) where =2[(∂u/∂x)^2+(∂v/∂y)^2+(∂w/∂z)^2 ]+(∂v/∂x+∂u/∂y)^2+(∂w/∂y+∂v/∂z)^2+(∂u/∂z+∂w/∂x)^2 is the dissipation function which represents the time rate at which energy is being dissipated per unit volume through the action of viscosity. Here, u,v and w are the velocity components of the fluid along thex,y and z directions respectively.C_P is the specific heat at constant pressure, T is the temperature, K is the thermal conductivity and γ is the Casson fluid parameter.
Species Concentration equation
The species concentration equation is given by
∂C/∂t+(q ̅.∇)C=D∇^2 C (1.4)
Here, C is the concentration of the species, D is the molecular diffusivity.
Maxwell’s …show more content…
Let n ̂ denote the unit normal drawn to the interface of two media 1 and 2 and [ ] denote the jump in the enclosed quantity in crossing interface from 1 to 2. The boundary conditions on the velocity vector for inviscid fluid flow are simple because here, the normal component of the velocity alone need to be continuous where as for viscous fluid flow both the normal and tangential components of the velocity must be continuous and hence the boundary conditions are given by n ̂ .[q ̅ ]=0 (1.13) n ̂×[q ̅ ]=0 (1.14) If J ̅,ρ_e denote surface current and surface charge density respectively, then the magnetic boundary conditions are n ̂ .[B ̅ ]=0 (1.15) n ̂×[H ̅ ]=J ̅ (1.16) n ̂ .[D ̅ ]=ρ_e (1.17) n ̂×[E ̅ ]=0 (1.18) Physically the above conditions mean that the normal component of the magnetic induction is continuous at the interface, the tangential component is discontinuous on account of sheer current if one or both the medium become infinitely conducting, the normal component of the electric field is discontinuous on account of surface charge density and the tangential component of the electric field is continuous always across the
Energy equation
Equation of energy for an electrically conducting, viscous incompressible fluid is ρC_P [∂T/∂t+(q ̅.∇)T]=K∇^2 T+μ(1+1/γ) (1.3) where =2[(∂u/∂x)^2+(∂v/∂y)^2+(∂w/∂z)^2 ]+(∂v/∂x+∂u/∂y)^2+(∂w/∂y+∂v/∂z)^2+(∂u/∂z+∂w/∂x)^2 is the dissipation function which represents the time rate at which energy is being dissipated per unit volume through the action of viscosity. Here, u,v and w are the velocity components of the fluid along thex,y and z directions respectively.C_P is the specific heat at constant pressure, T is the temperature, K is the thermal conductivity and γ is the Casson fluid parameter.
Species Concentration equation
The species concentration equation is given by
∂C/∂t+(q ̅.∇)C=D∇^2 C (1.4)
Here, C is the concentration of the species, D is the molecular diffusivity.
Maxwell’s …show more content…
Let n ̂ denote the unit normal drawn to the interface of two media 1 and 2 and [ ] denote the jump in the enclosed quantity in crossing interface from 1 to 2. The boundary conditions on the velocity vector for inviscid fluid flow are simple because here, the normal component of the velocity alone need to be continuous where as for viscous fluid flow both the normal and tangential components of the velocity must be continuous and hence the boundary conditions are given by n ̂ .[q ̅ ]=0 (1.13) n ̂×[q ̅ ]=0 (1.14) If J ̅,ρ_e denote surface current and surface charge density respectively, then the magnetic boundary conditions are n ̂ .[B ̅ ]=0 (1.15) n ̂×[H ̅ ]=J ̅ (1.16) n ̂ .[D ̅ ]=ρ_e (1.17) n ̂×[E ̅ ]=0 (1.18) Physically the above conditions mean that the normal component of the magnetic induction is continuous at the interface, the tangential component is discontinuous on account of sheer current if one or both the medium become infinitely conducting, the normal component of the electric field is discontinuous on account of surface charge density and the tangential component of the electric field is continuous always across the