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

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SUMMARY

This discussion focuses on the application of Stokes' theorem to relate angular velocity and vorticity in fluid dynamics. It establishes that the component of angular velocity, Ω, in the direction of the unit vector n is equal to half the vorticity ω, expressed mathematically as Ω = 0.5ω. The derivation utilizes the limit of a circular disc's boundary as its radius approaches zero, confirming the relationship through the equation ∇ × u for vorticity. The discussion also highlights the importance of understanding the translational and rotational components of fluid motion.

PREREQUISITES
  • Understanding of Stokes' theorem in vector calculus
  • Familiarity with the concept of vorticity in fluid dynamics
  • Basic knowledge of angular velocity and its components
  • Proficiency in parametric equations and limits in calculus
NEXT STEPS
  • Study the derivation of Stokes' theorem and its applications in fluid dynamics
  • Learn about the physical significance of vorticity and its calculation
  • Explore the relationship between angular momentum and vorticity in rotating fluids
  • Investigate the implications of Stokes' theorem in other areas of physics, such as electromagnetism
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Students and professionals in fluid dynamics, physicists studying rotational motion, and engineers involved in fluid mechanics applications will benefit from this discussion.

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Homework Statement


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


Homework Equations


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


The Attempt at a Solution


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

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


Start with this

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

then use Stokes theorem and get in the limit R \rightarrow 0

<br /> \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<br />
 

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