Find surface of maximum flux given the vector field's potential

I am not sure what you mean with the limits of integration.I also do not follow your calculation. You seem to be integrating a polynomial in ##r## but the result is not a polynomial (also you seem to have dropped the 8π which is not important for the location of the maximum but important for the actual value of the integral).
  • #1
Addez123
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Homework Statement
A vector field has the potential
$$\Phi = x^2 + y^2 + z^2 - (x^2 + y^2 + z^2)^2$$
Find the surface where the flux is at maximum.
Relevant Equations
Gauss theorem
The vectorfield is
$$A = grad \Phi$$ $$A = x^2 + y^2 + z^2 - (x^4 + y^4 + z^4 + 2x^2y^2 + 2x^2z^2 + 2y^2z^2)$$
The surface with maximum flux is the same as the volume of maximum divergence, thus:
$$div A = 6 - 20(x^2 + y^2 + z^2)$$

This would suggest at the point 0,0,0 the flux is at maximum.

But the book says its the surface where
$$div grad \Phi > 0$$
aka:
$$x^2 + y^2 + z^2 < 3/10$$
 
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  • #2
Addez123 said:
Homework Statement:: A vectorfield has the potential
$$\Phi = x^2 + y^2 + z^2 - (x^2 + y^2 + z^2)^2$$
Find the surface where the flux is at maximum
Relevant Equations:: Gauss theorem

The vectorfield is
$$A = grad \Phi$$ $$A = x^2 + y^2 + z^2 - (x^4 + y^4 + z^4 + 2x^2y^2 + 2x^2z^2 + 2y^2z^2)$$

[itex]A = \nabla \Phi[/itex] is a vector. What are its components? Your expression appears to be a scalar.

The surface with maximum flux is the same as the volume of maximum divergence, thus:
$$div A = 6 - 20(x^2 + y^2 + z^2)$$

This would suggest at the point 0,0,0 the flux is at maximum.

But the book says its the surface where
$$div grad \Phi > 0$$
aka:
$$x^2 + y^2 + z^2 < 3/10$$

You're not choosing a point such that [itex]\nabla \cdot A[/itex] is maximal; you are choosing a volume [itex]V[/itex] such that [itex]\int_V \nabla \cdot A\,dV = \int_{\partial V} A \cdot dS[/itex] is maximal.

In this case, [itex]\nabla \cdot A[/itex] is positive for [itex]r < \frac{3}{10}[/itex]. Therefore you can increase the flux across a surface within this volume by increasing the volume within the surface. The largest you can make the volume is by having it consist of everything inside [itex]r < \frac{3}{10}[/itex].

Outside of this sphere [itex]\nabla \cdot A < 0[/itex], so including any portion of this region will reduce the flux.
 
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  • #3
Also note that you really don't need the divergence theorem for this. In spherical coordinates the scalar field is ##\Phi = r^2(1-r^2)## so that it is clear that everything has spherical symmetry and therefore so will the sought surface. Because of the radial symmetry ##\vec A = d\Phi/dr \vec e_r = (2r-4r^3) \vec e_r## and so the flux ##F## out of the sphere of radius ##r = R## is
$$
F = \oint_{r = R} (2R - 4R^3) R^2 d\Omega = 8\pi (R^3 - 2 R^5).
$$
This leads to
$$
\frac{dF}{dR} = 8\pi (3R^2 - 10 R^4) = 0
$$
for the extreme value and therefore ##R^2 = 3/10##. We obtain the maximal flux from this by insertion.

pasmith said:
The largest you can make the volume is by having it consist of everything inside [itex]r < \frac{3}{10}[/itex].
Nitpicking, but ##r^2 < 3/10##.
 
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  • #4
Very nice explained @Orodruin I just have one small problem.

$$F = \int A * n dS = \int r^2(1 - r^2) * ? dS$$
dS = r^2 (jacobian) dr dv du

But what's my normal vector?
 
  • #5
Addez123 said:
Very nice explained @Orodruin I just have one small problem.

$$F = \int A * n dS = \int r^2(1 - r^2) * ? dS$$
dS = r^2 (jacobian) dr dv du

But what's my normal vector?
There is no normal left at that (the last) step. The normal of a sphere is ##\vec e_r## and this has been dotted with the ##\vec e_r## from ##\vec A## for a result of 1.
 
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  • #6
Orodruin said:
F=∮r=R(2R−4R^3)R^2dΩ=8π(R^3−2R^5).
What is your limit of integrations on this?

Also I don't see how your integral is correct:
$$\int (2r-4r^3)*r^2 = \int 2r^3 - 4r^5 = | r^4/2 - 2/3*r^6$$
not ##R^3−2R^5##
 
  • #7
Addez123 said:
What is your limit of integrations on this?

Also I don't see how your integral is correct:
$$\int (2r-4r^3)*r^2 = \int 2r^3 - 4r^5 = | r^4/2 - 2/3*r^6$$
not ##R^3−2R^5##
The integral is over the unit sphere. In other words ##R## is constant.
 

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