Spherical coordinates vector question

AI Thread Summary
The discussion centers on understanding the divergence of a radial vector field in spherical coordinates, specifically the equation ∇ · r = 3. The initial confusion arises from attempting to compute the divergence using a different approach, leading to an incorrect result. The correct method involves using the formula ∇ · F = (1/r²) ∂/∂r (r² F), where F represents the magnitude of the vector function. The clarification emphasizes that for a purely radial function, F equals r, which simplifies the calculation. This highlights the importance of using the appropriate divergence formula in spherical coordinates.
renlok
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I've no idea where to put this question but here it is I am trying to work through the examples our lecture has given in class and I wasn't getting them at all
the first thing that confused me was \nabla . \underline{r} = 3 I tried this myself with \nabla . \underline{r} = \frac{1}{r^2}\frac{\delta{r^2}}{\delta{r}} = \frac{2}{r} (working in spherical coords)
but if you use \textbf{e_r} = \frac{\textbf{r}}{r} it works but I have no idea where this comes from could someone at least point me in the right direction that would be really helpful thanks

 
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You should try to use the template. But oh well.

You've had a go at using spherical coordinates - yep that's one way to do it. But I think you've done it wrong. When the function is purely radial (as it is in your case), the divergence is equal to:

\frac{1}{r^2} \frac{\partial}{\partial r} (r^2 F)
(where F is the magnitude of the vector function in question). For your problem, F=r.
 
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