Divergence in spherical coordinates

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The discussion focuses on calculating the divergence of the vector function F(r) and its implications in spherical coordinates. The divergence is derived as a function of r and ε, with specific attention to how ε affects the outcome. Participants seek clarification on calculating the flux of F through a sphere and verifying its relation to the divergence within that sphere. The conversation highlights the need for understanding flux and its independence from the radius R in the limit as ε approaches zero. Overall, the thread emphasizes the mathematical approach to divergence and flux in the context of vector fields.
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Problem:

For the vector function \vec{F}(\vec{r})=\frac{r\hat{r}}{(r^2+{\epsilon}^2)^{3/2}}

a. Calculate the divergence of ##\vec{F}(\vec{r})##, and sketch a plot of the divergence as a function ##r##, for ##\epsilon##<<1, ##\epsilon##≈1 , and ##\epsilon##>>1.

b. Calculate the flux of ##\vec{F}## outward through a sphere of radius R centered at the origin, and verify that it is equal to the integral of the divergence inside the sphere.

c. Show that the flux is ##4 \pi## (independent of R) in the limit ##\epsilon \rightarrow 0##.

Solution:

a. Calculating the divergence is simply a matter of plugging the function correctly into the spherical coordinates divergence formula. I get F_r=\frac{r}{(r^2+{\epsilon}^2)^{3/2}} \Rightarrow \frac{\partial F}{\partial r}=3r^2(r^2+{\epsilon}^2)^{-3/2}-3r^4(r^2+{\epsilon}^2)^{-5/2}

Therefore,

\nabla \cdot \vec{F}= 3(r^2+{\epsilon}^2)^{-3/2}-3r^2(r^2+{\epsilon}^2)^{-5/2}

So for the different values of ##\epsilon## do I just substitute?
 
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Also can someone point me in the right direction for parts b. and c.? Thanks.
 
Anyone?
 
Check your ∂F/∂r.

Anyway, the end result is correct.

As for b), what is flux?

ehild
 
Last edited:

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