How to Determine Scalar Potential Inside and Outside a Charged Sphere?

Join the discussion
Registration is free. Ask a follow-up in this thread, or start your own.
7 replies · 4K views
dsta
Messages
8
Reaction score
0

Homework Statement


Use Poisson's equation and Laplace's equation to determine the scalar potential inside and outside a sphere of constant charge density po. Use Coulomb's law to give the limit at very large r, and an argument from symmetry to give the value of E at r=0.


Homework Equations


del2V = - p/epsilono
del2V = 0

The Attempt at a Solution


Not sure how to start this just using Poisson's/Laplace's equation.
 
Physics news on Phys.org
Hmm okay. I'm not sure what symmetries you would need to consider to simplify [itex]\nabla^2V[/itex] in spherical coordinates. Because the charge density is constant, V does not depend on r inside the sphere...I'm not sure about anything else.
 
What makes you think [itex]V[/itex] doesn't depend on [itex]r[/itex]?:confused:

Surely you can say that it doesn't depend on either the azimuthal or polar angles though right?...After all, a test charged placed at any given value of [itex]r[/itex], will "see" the same charge distribution at say [itex]\theta=\phi=\pi/4[/itex] as it would at say [itex]\theta=3\pi[/itex], [itex]\phi=\pi/7[/itex] or any other angle wouldn't it? (Draw a picture to convince yourself of this!)...This type of symmetry is called spherical symmetry.
 
Oops sorry, I meant to say that. Okay so using the simplified form of the equation for [itex]\nabla^2V[/itex] in spherical coordinates, and Poisson's equation, I was able to get the equation for V inside the sphere. For outside the sphere, the charge density is 0 obviously, so you have to use Laplace's equation. I tried to do this but I can't anywhere near the form of the equation I'm meant to be getting :frown:
 
Inside the sphere:
[tex]\nabla^2V = \frac{1}{r}[/tex][tex]\frac{d}{dr}(r^2\frac{dV}{dr}) = \frac{\rho_{o}}{\epsilon_{o}}[/tex]
[tex]\Rightarrow V = - \frac{\rho_{o} r^2}{6\epsilon_{o}}[/tex]

Outside the sphere:
[tex]\nabla^2V = \frac{1}{r}[/tex][tex]\frac{d}{dr}(r^2\frac{dV}{dr}) = 0[/tex]
[tex]\Rightarrow r^2\frac{dV}{dr} = constant = a[/tex]
[tex]\Rightarrow V = \frac{-a}{r} + c[/tex]
I'm assuming that you now have to use some sort of boundary conditions...
 
Last edited:
dsta said:
Inside the sphere:
[tex]\nabla^2V = \frac{1}{r}[/tex][tex]\frac{d}{dr}(r^2\frac{dV}{dr}) = \frac{\rho_{o}}{\epsilon_{o}}[/tex]
[tex]\Rightarrow V = - \frac{\rho_{o} r^2}{6\epsilon_{o}}[/tex]

You're missing a minus sign in your first equation (although it looks like that's just a typo, since your answer has the correct sign)...More importantly, shouldn't you have two constants of integration for the solution to this 2nd order ODE?:wink: