How Does Stokes' Theorem Relate to Vorticity in Fluid Dynamics?

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Homework Statement


Consider an imaginary circular disc, of radius R, whose arbitrary orientation is described by the unit vector, [tex]\vec {n}[/tex], perpendicular to the plane of the disc. Define the component, in the direction [tex]\vec {n}[/tex], of the angular velocity, [tex]\vec {\Omega}[/tex], at a point in the fluid by [tex]\vec {\Omega}. \vec {n} = \lim_{R \rightarrow 0}[\frac {1}{2 \pi R^2} \oint_C \vec {u}.dl][/tex], where C denotes the the boundary (rim) of the disc. Use Stokes' theorem, and the arbitrariness of [tex]\vec {n}[/tex], to show that [tex]\vec {\Omega}= \frac {1}{2} \vec {\omega}[/tex], where [tex]\vec {\omega} = \nabla * \vec {u}[/tex] is the vorticity of the fluid at R=0. [This definition is based on a description applicable to the rotation of solid bodies. Confirm this by considering [tex]\vec {u} = \vec {U} + \vec {\Omega}* \vec{r}[/tex], where [tex]\vec {U}[/tex] is the translational velocity of the body, [tex]\vec {\Omega}[/tex] is its angular velocity and [tex]\vec {r}[/tex] is the position vector of a point relative to a point on the axis of rotation.]


Homework Equations


Stokes' theorem : [tex]\oint_c u.dl = \iint_S (\nabla * u) .n ds[/tex]


The Attempt at a Solution


Either 1.:
C is boundary of [tex]x^2 + y^2 = R^2[/tex]. Parametrically x= Rcost, y = Rsint
dx = -Rsintdt, dy = Rcostdt
L.H.S. of Stokes becomes [tex]\oint_c udx + vdy + wdz[/tex]
= [tex]\oint_C -uRSintdt + vRCostdt[/tex]
=[tex]\int_{0}^{2 \pi} -uRSint dt + vRCost dt[/tex]
=[tex]uRCost + vRSint \right]_{0}^{2 \pi}[/tex]
= -uR - uR
=-2uR
multiply term outside integral
=[tex]-\frac{u}{\pi R}[/tex]

Or 2:
[tex]\frac {1}{2} (\nabla * \vec {u}). \vec {n} = \lim_{R \rightarrow 0}[\frac {1}{2 \pi R^2} \iint_S (\nabla * u) .n ds ][/tex], ...
 
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[ Nevermind :) .. I was wrong. ]
 


Start with this

[tex] \vec {\Omega}. \vec {n} = \lim_{R \rightarrow 0}[\frac {1}{2 \pi R^2} \oint_C \vec {u}.dl] [/tex]

then use Stokes theorem and get in the limit [tex]R \rightarrow 0[/tex]

[tex] \vec {\Omega}. \vec {n} = \lim_{R \rightarrow 0}[\frac {1}{2 \pi R^2} \iint_S (\nabla * u) .n ds ] = \lim_{R \rightarrow 0}[\frac {1}{2 \pi R^2} (\nabla * u) \pi R^2 ] = 0.5 \nabla * u[/tex]