Proving Divergence Theorem using Gauss' Theorem

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Homework Help Overview

The discussion revolves around proving the Divergence Theorem using Gauss' Theorem, specifically focusing on the integral involving the divergence of a vector field and an exponential decay factor. Participants are exploring the mathematical relationships and identities that apply to this context.

Discussion Character

  • Mathematical reasoning, Problem interpretation, Assumption checking

Approaches and Questions Raised

  • Participants discuss setting functions for the application of vector identities, question the choice of variables, and explore the implications of integrating over a spherical surface. There are inquiries about the behavior of the integrand at infinity and the appropriateness of coordinate systems used for differentiation.

Discussion Status

The conversation is active, with participants sharing insights and hints. Some have suggested approaches to simplify integrals and have raised questions about the limits of integration and the behavior of functions at infinity. There is no explicit consensus yet, but several productive lines of reasoning are being explored.

Contextual Notes

Participants are working under the assumption that the original integral is over all space, and there are discussions about the implications of this assumption on the surface integrals involved. The use of different coordinate systems for differentiation is also a point of consideration.

latentcorpse
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I need to show that, using Gauss' Theorem (Divergence Theorem), i.e. integration by parts, that:

\int_V dV e^{-r} \nabla \cdot (\frac{\vec{\hat{r}}}{r^2}) = \int_V dV \frac{e^{-r}}{r^2}

any ideas on where to start?
 
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Hint:The following vector identity should be useful:

\vec{\nabla}\cdot{f\vec{A}}=f(\vec{\nabla}\cdot\vec{A})+\vec{A}\cdot(\vec{\nabla}f)
 
thanks.
1, do i set f=\frac{1}{r^2}?
2, how did you know to do that so quickly?
 
1. No, set f=e^{-r}

2. It's a common theme in many EM derivations.
 
ok so it then equals
\int_V dV \nabla \cdot (\frac{e^{-r} \vec{\hat{r}}}{r^2}) - \int_V dV (\frac{\vec{\hat{r}}}{r^2}) \cdot (\nabla e^{-r}) = \int_S (\frac{e^{-r} \vec{\hat{r}}}{r^2}) \cdot \vec{n} dS - \int_V dV (\frac{\vec{\hat{r}}}{r^2}) \cdot (\nabla e^{-r})
My instinct is to do the integral over the surface S using S = sphere of radius a as then \vec{n}=\vec{\hat{r}} and i can get rid of that dot product. but then dS=4 \pi a^2 which messes stuff up and also what do I do on the right?
 
I'm assuming that the original integral was over all of space, correct?

If so, then your surface integral is over the boundary of all space which is at r\to\infty...what is the value of the integrand there?:wink:

For the second term; Take the gradient of e^{-r} using spherical coords...
 
ok. might be getting somewhere now. on the right i took the grad of the exponential term and got \nabla e^{-r} = -e^{-r} \vec{\hat{r}} is that right?
seems to be so because that causes the integral on the right to simplify substantially to -\int_V dV (\frac{\vec{\hat{r}}}{r^2}) \cdot (\nabla e^{-r}) = + \int_V dV \frac{e^{-r}}{r^2} which is what we're looking for - therefore it appears to just be a matter of showing the integral on the left vanishes?
 
indeed it is over all space. i would then imagine it would zero because e^{-r} \rightarrow 0 as r \rightarrow \infty. If this is the case, how owuld you recommend I write that in order to be an acceptable answer? Also, I took the grad of the exponential using Cartesians - does that matter?
 
latentcorpse said:
indeed it is over all space. i would then imagine it would zero because e^{-r} \rightarrow 0 as r \rightarrow \infty. If this is the case, how owuld you recommend I write that in order to be an acceptable answer? Also, I took the grad of the exponential using Cartesians - does that matter?

Formally, you could start by assuming that your volume is a sphere of radius a and then take the limit as a approaches infinity.

And it doesn't matter that you used Cartesian coords to take the gradient; although it would probably have been quicker to use spherical coords.
 
  • #10
ok
but then
\int_S (\frac{e^{-r} \vec{\hat{r}}}{r^2}) \cdot \vec{n} dS = \int_S (\frac{e^{-r} \vec{\hat{r}} \cdot \vec{\hat{r}}}{r^2}) dS= \frac{e^{-r}}{r^2} 4 \pi a^2
if i take the limit as a \rightarrow \infty i get \infty
 
  • #11
unless i take dS=4 \pi r^2 and then the intergal becomes 4 \pi e^{-r} and then the limit as r \rightarrow \infty would be 0. Any advice? Cheers.
 
  • #12
latentcorpse said:
ok
but then
\int_S (\frac{e^{-r} \vec{\hat{r}}}{r^2}) \cdot \vec{n} dS = \int_S (\frac{e^{-r} \vec{\hat{r}} \cdot \vec{\hat{r}}}{r^2}) dS= \frac{e^{-r}}{r^2} 4 \pi a^2
if i take the limit as a \rightarrow \infty i get \infty

Along the surface, r=a.
 
  • #13
i don't understand what you mean there sorry
 
  • #14
actually surely if i integrate over a sphere of radius a, dS=a^2 \sin{\theta} d\theta d\phi?

in which case this integral becomes \int_S \frac{e^{-r} a^2}{r^2} \sin{\theta} d\theta d\phi = 4 \pi \frac{a^2}{r^2} e^{-r}

would i then let a or r go to infinity, or is this all complete bollocks? HELP I am really confused now! arghhhh!
 
  • #15
r is the distance from the origin to the infinitesimal area element dS. Since the entire surface is a distance a from the origin, that means that r=a everywhere on the surface.

\implies \int_S \frac{e^{-r}}{r^2}dS=\int_S \frac{e^{-a}}{a^2} dS =\int_S \frac{e^{-a} a^2}{a^2} \sin{\theta} d\theta d\phi = 4 \pi e^{-a}
 
  • #16
cheers buddy!
 

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