Divergence in spherical coordinates

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Homework Help Overview

The discussion revolves around calculating the divergence of a vector function in spherical coordinates and exploring related concepts such as flux through a sphere. The vector function is defined as \(\vec{F}(\vec{r})=\frac{r\hat{r}}{(r^2+{\epsilon}^2)^{3/2}}\), with specific tasks related to divergence and flux for varying values of \(\epsilon\).

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • The original poster attempts to calculate the divergence of the vector function using the spherical coordinates divergence formula and questions whether substituting different values of \(\epsilon\) is the correct approach. Other participants inquire about the definition of flux and check the differentiation performed by the original poster.

Discussion Status

The discussion is ongoing, with participants seeking clarification on the calculations and definitions involved. Some guidance has been offered regarding the need to verify the differentiation step, while others are exploring the concept of flux in relation to the problem.

Contextual Notes

Participants are navigating the complexities of the problem, including the implications of varying \(\epsilon\) and the definitions of divergence and flux. There is an emphasis on ensuring the correct application of mathematical principles in spherical coordinates.

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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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