Problem with taking the divergence

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Homework Help Overview

The discussion revolves around taking the divergence of the vector field \(\frac{\hat{r}}{r^2}\) in the context of vector calculus, specifically within spherical coordinates. The original poster seeks clarification on the relationship between the divergence of this expression and the Dirac delta function.

Discussion Character

  • Exploratory, Conceptual clarification, Assumption checking

Approaches and Questions Raised

  • Participants discuss the use of spherical coordinates and the implications of the divergence theorem. Questions arise regarding the behavior of the divergence at the origin and the interpretation of the results in relation to the Dirac delta function.

Discussion Status

The conversation is ongoing, with participants exploring different interpretations of the divergence and its implications. Some guidance has been provided regarding the divergence theorem and its application in different scenarios related to the origin.

Contextual Notes

There is a mention of the undefined nature of \(\frac{1}{r^2}\) at \(r=0\) and the need to consider volumes that either enclose or do not enclose the origin when applying the divergence theorem.

lavster
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hi, can someone tell me how \nabla\dot(\frac{\widehat{r}}{r^2})=4\pi\delta^3(r)

thanks
 
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lavster said:
hi, can someone tell me how \nabla\dot(\frac{\widehat{r}}{r^2})=4\pi\delta^3(r)

thanks

How would you normally proceed with taking the divergence? What coordinate system is this in?
 
i would use spherical coord system. using the corresponding form of div. but this gives 0 as the r^2 in the formula is canceled but the r^2 in the div eqn
 
lavster said:
i would use spherical coord system. using the corresponding form of div. but this gives 0 as the r^2 in the formula is canceled but the r^2 in the div eqn

Sure, it gives zero everywhere, except at r=0. Remember, \frac{1}{r^2} is undefined at r=0:wink:

What does the divergence theorem tell you about the volume integral

\int_{\mathcal{V}}\left(\mathbf{\nabla}\cdot\frac{\hat{\mathbf{r}}}{r^2}\right)dV

in two cases:

(1) When \mathcal{V} is any volume enclosing the origin?
(2) When \mathcal{V} is any volume not enclosing the origin?

Compare these results, along with the fact that \mathbf{\nabla}\cdot\frac{\hat{\mathbf{r}}}{r^2}[/itex] is zero everywhere except at r=0, where it is undefined, to the properties defining the 3D Dirac Delta function.
 

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