Calculating Electric Field of a Polarized Sphere

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SUMMARY

The discussion focuses on calculating the electric field of a polarized sphere with a polarization defined as P = k * r, where k is a constant and r is the vector from the center. The bound surface charge density σ_b is calculated using σ_b = P · n̂, resulting in σ_b = kR cos(θ), while the bound volume charge density ρ_b is found to be ρ_b = -3k. The electric field inside the sphere is given by E = -kr/ε₀ n̂, and outside the sphere, the electric field is zero. The discussion emphasizes the correct application of Gauss's law and the potential integral method for accurate results.

PREREQUISITES
  • Understanding of electric polarization and bound charges
  • Familiarity with Gauss's law in electrostatics
  • Knowledge of vector calculus, specifically divergence and gradient operations
  • Proficiency in using integral calculus for potential calculations
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  • Study Griffiths' "Introduction to Electrodynamics" for detailed explanations on polarization
  • Learn about the application of Gauss's law in non-symmetric charge distributions
  • Explore the method of calculating electric fields using potential integrals
  • Investigate the implications of bound charges in dielectric materials
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abode_x
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From Griffiths, Problem 4.1
A sphere of radius R carries a polarization
<br /> \textbf{P}=k\textbf{r}<br />

where k is constant and r is the vector from the center.
a. Calculate \sigma_b and \rho_b.
b. Find the field inside and outside the sphere.

part a is handled simply by \sigma_b=\textbf{P}\cdot\hat{n} and \rho_b=-\nabla\cdot\textbf{P}.

part b is handled most easily by using the bound charges found and gauss's law, giving: \textbf{E}=\frac{-kr}{\epsilon_0}\hat{r} and 0 outside.

part b can also be handled by first getting the potential through:\frac{1}{4\pi \epsilon_0}\int_v \frac{\hat{r}\cdot\textbf{P}}{r^2}d\tau. Then just get the negative gradient of V to yield E. This gives the same result as method 1 for both inside and outside (P=0 when dealing with outside case).

Now, i tried to get the field, again by computing for V but this time with:
V(r)=\frac{1}{4\pi \epsilon_0}\oint_s\frac{\sigma_b}{r}da + \frac{1}{4\pi \epsilon_0}\int_v\frac{\rho_b}{r}d\tau. The answer i get using this integral is different. i would like to know if in the first place this integral is applicable? if I'm trying to get the potential inside, do i still consider the surface bound charge?

the best i managed was an answer negative to the correct one. (but this had 1 dubioius step involved). also, i could only attempt to get the potential inside. can anyone make the last method work (for both outside and inside)? or share why it doesnt?

thanks.
 
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\sigma_b is not spherically symmetric, so E iinside is not.
You can't use Gauss as you do in that case.
Your integrals should give the right answer if you mean r-r'
when you write r.
 
Last edited:
Gauss's law actually gives the right answers. \sigma_b=kR everywhere on the surface if you apply the definition. likewise, \rho_b=-3k. these are symmetric and so is E inside and out.

as for the r-r' hint. i don't see it yet, but i will try it. thanks.

i was wrong though, about my claim that i got E=0 outside using the second method. that's another issue - how to get that result.
 
abode_x said:
Gauss's law actually gives the right answers. \sigma_b=kR everywhere on the surface if you apply the definition. likewise, \rho_b=-3k. these are symmetric and so is E inside and out.

as for the r-r' hint. i don't see it yet, but i will try it. thanks.

i was wrong though, about my claim that i got E=0 outside using the second method. that's another issue - how to get that result.
\sigma_b does not equal kR. It equals kR cos\theta because of the dot product. Go back and study Griffriths some more, then come back to the problem.
 
Meir Achuz said:
\sigma_b does not equal kR. It equals kR cos\theta because of the dot product. Go back and study Griffriths some more, then come back to the problem.

Meir Achuz, I don't quite understand this.

If P(r)=kr \vec{e_r}
Then, won't \sigma_b be

\sigma_b = \vec{P}.\hat{n} = k R (\vec{e_r}.\vec{e_r}) = kR
 
Last edited:
Whoops. I apologize. I had read it as P=a fixed vector.
Using Gauss as in the first post gives the right answer.
To use the potential integrals still requires r-r'.
Thanks for catching my carelessness.
 

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