Poisson's equation and Green's functions

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The discussion revolves around verifying the integral solution to Poisson's equation and addressing a contradiction encountered when applying the Laplacian. The integral for the solution is correctly stated, but the confusion arises when evaluating the Laplacian of the term 1/|x-x'|, which is mistakenly assessed as zero instead of yielding the delta function. References like Jackson's "Classical Electrodynamics" clarify that the Laplacian of this term equals -4πδ(x-x'), and the discussion includes attempts to derive this result from first principles. Ultimately, the participants work through the necessary steps to confirm the correct evaluation of the integral and the properties of the Laplacian.
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Trying to verify the general integral solution to Poisson's equation I reach the following contradiction, what am I missing/doing wrong?

A solution u(\mathbf{x}) to Poisson's equation satisfies:

\nabla^2 u(\mathbf{x}) = - \frac{\rho(\mathbf{x})}{\epsilon_0}

we can find such a solution in a given domain by evaluating:

u(\mathbf{x}) = \int_{V} \frac{\rho(\mathbf{x'})}{4 \pi \epsilon_0 |\mathbf{x}-\mathbf{x'}|} d\mathbf{x'}

or equivalently (if we are only interested in the electric field):

\mathbf{E} = -\nabla u = - \int_{V} \frac{\rho(\mathbf{x'})}{4 \pi \epsilon_0} \frac{\mathbf{x}-\mathbf{x'}}{|\mathbf{x}-\mathbf{x'}|^3} d\mathbf{x'}

We can think of these solutions as either the Green's function solution or, physically, as the convolution of the point source solution with the source density \rho(\mathbf{x}).

However if I take the Laplacian (or the divergence in the case of the electric field solution) of either of the above I get zero instead of -\frac{\rho}{\epsilon_0}. What am I missing??

To evaluate the Laplacian/divergence of the above I make use of the fact that \mathbf{x'} is a 'dummy variable', which allows me to switch the order of integration and differentiation when applying \nabla^2 to the integral on the RHS and also means the components of \mathbf{x'} all have derivative zero. With these assumptions the operation is fairly straightforward to carry out, but I have anyway verified my answer with Mathematica.
 
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Not so. You should take the Laplacian with respect to x (after all you are calculating \nabla^2{u(x)}). Since
\nabla^2 \frac{1}{|x-x'|}=\delta(x-x')
you get the right result from the integration.
This expression is derived in many places:
Jackson, Classical Electrodynamics, 2nd ed., Eq. (1.31)
Arfken, Math Methods for Physicists, 2nd ed., sect. 1.15
to give two examples.
 
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Thanks marcusl.

Yes I was taking the derivative wrt x (hence the derivatives of all components of x' being zero). But I was erroneously evaluating the Laplacian of \frac{1}{|x-x'|} as zero.

I've since found references to the result you quote, but they all start by searching for the Green's function G that satisfies \nabla^2 G = \delta(x-x') and then deducing it to be the above... out of interest do you know of any way to show it starting from the other end --- i.e. directly differentiating \frac{1}{|x-x'|} and showing its Laplacian to be the delta function? Or do the references you quote do it that way?

I'll look them up when I get the chance. Thanks again.
 
Yes, Jackson shows it explicitly. And, now that I'm looking at his formula instead of relying on memory, I see I forgot the constant
\nabla^2 \frac{1}{|x-x'|}=-4\pi \delta(x-x')
 
marcusl said:
Yes, Jackson shows it explicitly. And, now that I'm looking at his formula instead of relying on memory, I see I forgot the constant
\nabla^2 \frac{1}{|x-x'|}=-4\pi \delta(x-x')

In my 2nd edition, Jackson says on p.40 :" since \nabla^{2}(1/r) = 0 for r \neq 0 and its volume integral is -4\pi, we can write the formal equation, \nabla^{2}(1/r) = -4\pi \delta^{3}(x)..."

In exam, if you reproduce "Jackson's proof", I give you 2 marks out of 10! You would gain the remaining 8 marks, if you prove the underlined sentence in Jackson's statement. I can tell you, it is a tricky one, and Jackson doesn't do it!

regards

sam
 
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OK samalkhaiat I'll have a shot at your "remaining 8 marks", let me know if I'm missing something!

From the divergence theorem we have,

I = \int_{V} \nabla^2 (1/r) dV = \int_{S} \nabla (1/r) \cdot \mathbf{dS}

Since the RHS is a surface integral we don't need to worry about evaluating \nabla (1/r) at the origin and so, choosing V as a sphere centred on the origin, we can straightforwardly write the surface integral as:

I = \int_{0}^{2\pi} \int_{0}^{\pi} \frac{\partial}{\partial r} \left(\frac{1}{r}\right) r^2 \sin{\theta} \; d\theta \; d\phi = -4\pi

(since \frac{\partial}{\partial r} \left(\frac{1}{r}\right) = -\frac{1}{r^2}) as required.
 
Jackson has similar expressions on p. 39 (he calls the integral C instead of I).
 
jmb said:
OK samalkhaiat I'll have a shot at your "remaining 8 marks", let me know if I'm missing something!

From the divergence theorem we have,

I = \int_{V} \nabla^2 (1/r) dV = \int_{S} \nabla (1/r) \cdot \mathbf{dS}

Since the RHS is a surface integral we don't need to worry about evaluating \nabla (1/r) at the origin and so, choosing V as a sphere centred on the origin, we can straightforwardly write the surface integral as:

I = \int_{0}^{2\pi} \int_{0}^{\pi} \frac{\partial}{\partial r} \left(\frac{1}{r}\right) r^2 \sin{\theta} \; d\theta \; d\phi = -4\pi

(since \frac{\partial}{\partial r} \left(\frac{1}{r}\right) = -\frac{1}{r^2}) as required.

For this, I give you 3 marks out of the 8! Your next step is to show that the result -4\pi holds true for ANY surfase S bounding V (not just spherical). Then and only then you can earn the remaining marks! Have a go at it and let me know.


regards

sam
 
samalkhaiat said:
jmb said:
For this, I give you 3 marks out of the 8! Your next step is to show that the result -4\pi holds true for ANY surfase S bounding V (not just spherical). Then and only then you can earn the remaining marks! Have a go at it and let me know.


regards

sam

Doesn't it just follow on from the properties of \nabla^2(1/r)?

We already know that \nabla^2(1/r) is zero everywhere except r=0, thus any volume V (enclosed by some surface S) which encloses r=0 will produce the same value for the integral, regardless of its shape, since the integrand gives no contribution to the integral at any other location. Equally any volume not enclosing r=0 will give zero when integrated. Maybe I'm missing a subtlety?
 
  • #10
jmb said:
samalkhaiat said:
We already know that \nabla^2(1/r) is zero everywhere except r=0, thus any volume V (enclosed by some surface S) which encloses r=0 will produce the same value for the integral, regardless of its shape, since the integrand gives no contribution to the integral at any other location. Equally any volume not enclosing r=0 will give zero when integrated. Maybe I'm missing a subtlety?

By stating this, you gain the remaining marks. The trick is to surround the point x = 0 by small enough sphere and do the integration in the bounded region x \neq 0:

Let \Sigma be a surface bounding a region V containing the orign, and let \sigma be a small spherical surface enclosing the point x = 0. Therefore, we have x \neq 0 everywhere in the region U bounded by \Sigma + \sigma, i.e.,

\int_{U} \nabla^{2}|\frac{1}{x}| \ d^{3}x = 0 = \int_{\Sigma + \sigma} \vec{\nabla}|\frac{1}{x}| \ . \ d\vec{S}

From this it follows that the integral over the whole region V is

\int_{V} \nabla^{2}|\frac{1}{x}| \ d^{3}x = \int_{\Sigma} \vec{\nabla}|\frac{1}{x}| \ . \ d\vec{S} = - \int_{\sigma} \vec{\nabla}|\frac{1}{x}| \ . \ d\vec{S}

Or,

\int_{V} \nabla^{2}|\frac{1}{x}| \ d^{3}x = \int_{\sigma} \frac{1}{|x|^{2}} \left( \hat{x}. \hat{n}_{\sigma} \right) dS

where \hat{x} is the unit vector along x and \hat{n}_{\sigma} is the unit OUTWARD normal at dS of \sigma;

\hat{x} . \hat{n}_{\sigma} = -1

Thus

\int_{V} \nabla^{2}|1/x| \ d^{3}x = - \frac{1}{R^{2}} \int_{\sigma} dS = -4\pi


regards

sam
 
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  • #11
Cool. Many thanks again to both marcusl and samalkhaiat for your help!
 

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