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Reynolds Transport Theorem




Reynolds transport theorem is a fundamental theorem used in formulating the basic laws of Fluid Dynamics . The basic laws are the continuity equation, the momentum equations and the energy equation. In physics and engineering, these laws are also known, respectively, as the Law Of Conservation Of Mass , Newton's Second Law , and the Laws Of Thermodynamics .

Imagine a system with a Control Volume and a Control Surface . Reynolds' transport theorem states that the Rate Of Change of an Extensive Property N within the system is equal to the rate of change of N within the control volume and the net rate of change of N through the control surface. For an example, the law of conservation of mass states that rate of change of the property, mass, is equal to the sum of the rate of accumulation of mass within a control volume and the net rate of flow of mass across the control surface.

The differential forms of these equations with additional assumptions are commonly known as the Navier-Stokes Equations . The additional assumptions are the Newton's Viscosity Law and the Fourier's Conduction Law .


GENERAL FORM

The Reynolds transport theorem refers to any extensive property, N, of the fluid in a particular Control Volume . It is expressed in terms of a Substantive Derivative on the left-hand side.

rac{DN_{sys}}{Dt} = \int_{c.v.}^{} rac{\partial}{\partial t} ( ho \eta) dV + \int_{c.s.}^{} ho \eta \overrightarrow{\upsilon_b}\cdot \widehat{n} dA+\int_{c.s.}^{} ho \eta \overrightarrow{\upsilon_r}\cdot \widehat{n} dA,

where η is N per unit mass, t is time, c.v. refers to the control volume, c.s. refers to the control surface, ρ is the fluid density, V is the volume, \upsilon_b is the velocity of the boundary of the control volume (the control surface), \upsilon_r is the velocity of the fluid with respect to the control surface, n is the outward pointing normal vector on the control surface, and A is the area.


MASS FORMULATION

Also called the continuity equation, the control volume form of the conservation of mass is found by substituting mass in for N. This means that η is equal to 1.

rac{DM_{sys}}{Dt}=\int_{c.v.}^{} rac{\partial ho}{\partial t}\;dV + \int_{c.s.}^{} ho ec{v}_b \cdot \widehat{n}\;dA + \int_{c.s.}^{} ho ec{v}_r \cdot \widehat{n}\;dA

All variables are defined as in the general formulation. M is equal to the mass of the control volume. In a steady flow system, the left hand side of the equation will be equal to 0, i.e. the mass of the control volume does not change, implying that the mass flow rate into the control volume is equal to the mass flow rate out of the control volume.


MOMENTUM FORMULATION

The momentum equation is found by substituting momentum in for N. From this, η is found to be velocity. The time rate of change of momentum (now the left hand side of the equation) is, from Newton's Second Law , equal to the net force. Note that this is a vector equation.

\sum_{} \overrightarrow{F}=\int_{c.v.}^{} rac{\partial}{\partial t}( ho \overrightarrow{\upsilon}) dV + \int_{c.s.}^{} ho \overrightarrow{\upsilon}(\overrightarrow{\upsilon_b} \cdot \widehat{n})dA + \int_{c.s.}^{} ho \overrightarrow{\upsilon}(\overrightarrow{\upsilon_r} \cdot \widehat{n})dA,

where F is force, \upsilon is the velocity of fluid in a coordinate system attached to the control surface, and all other variables are defined as in the general formulation.


ENERGY FORMULATION

The energy equation is found by substituting energy in for N. From this, η is found to be energy per unit mass.

\dot{Q}-\sum{} \dot{W}=\int_{c.v.}^{} rac{\partial}{\partial t} \left [ ho \left ( rac{\upsilon^2}{2}+gz+ ilde{u} ight ) ight ] dV + \int_{c.s.}^{} \left [ rac{\upsilon^2}{2}+gz+ ilde{u}+ rac{p}{ ho}\ ight] ho \overrightarrow{\upsilon_b}\cdot\widehat{n}dA + \int_{c.s.}^{} \left [ rac{\upsilon^2}{2}+gz+ ilde{u}+ rac{p}{ ho}\ ight] ho \overrightarrow{\upsilon_r}\cdot\widehat{n}dA

where Q is the Heat Transfer into the control volume, W is the Work done by the system, g is the acceleration due to gravity, z is the vertical distance from an arbitrary datum, ilde{u} is the Specific Internal Energy of the fluid, p is the pressure and all other variables are defined as in the general formulation.

Note that these equations make no consideration for chemical reactions or potential energy associated with Electromagnetic Field s.


REFERENCES

  • M.C. Potter, J.F. Foss, ''Fluid Mechanics'', Great Lakes Press, 1982


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