Concentric conducting spherical shells

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The discussion focuses on the electrostatics of three concentric conducting shells with specified potentials and radii. For Laplace's equation to apply, the potential at the surfaces must remain constant, and the electric field must approach zero at infinity. The potential is derived to be ø = A + B/r, with specific values for A and B determined by boundary conditions at the inner and middle shells. The electric field is found to be zero within the inner shell and follows E = (bø_0)/(2r^2) for the region outside the middle shell. Finally, the charge density and electrostatic energy are calculated, revealing σ_b = (ø_0ε_0)/(2b) and a specific expression for the energy stored in the system.
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Homework Statement



Consider three concentric conducting shells, with potentials 0, ø_0, 0 and radius a, b ,c where a < b < c.

(a)State conditions for Laplace to work and boundary conditions for E

(b)Show ø is of the form:

(c) Find ø and E everywhere.

(d) Find the charge density and electrostatic energy.

29bey38.png

Homework Equations


The Attempt at a Solution



Part (a)

Condition for laplace: Potential at surface of shells must be constant
Boundary Conditions for E: As r → \infty |\vec {E}| → 0

Part (b)
29vxs8n.png


Consider r → \infty , V → const.

\sum_{l=0}^{\infty} (A_l r^l)P_{l cosθ} → const.

This implies that l = 0 is the only solution.

Thus, general solution for ø:
ø = A + \frac {B}{r}

Part (c)
1. ø must be continuous at r= a, so ø_{in} = ø_{out} at r=a.
2. Potential at r = a is 0.
We obtain two simultaneous equations:
A = \frac {B}{a}
0 = A + \frac {B}{a}
So this implies A = B = 0 for the first shell.

Middle shell
At r = b, ø_0 = A + \frac {B}{a}
Continuity: ø_{in} = ø_{out} <br /> so Ab = B<br /> Solving, we get ø_{in} = \frac {ø_0}{2}, ø_{out} = \frac{bø_0}{2r}<br /> <br /> <b>Outermost Shell</b><br /> Does nothing, as shown above.<br /> <br /> Using superposition principle, so far we have:<br /> ø = \frac {ø_0}{2} (0 &amp;lt; r &amp;lt;b)<br /> ø = \frac {ø_0b}{2r} (r &amp;gt; b)<br /> <br /> Using E = - \nabla ø<br /> <br /> E = 0 (0 &amp;lt; r &amp;lt; b)<br /> E = \frac {bø_0}{2r^2} (r &amp;gt; b)<br /> <br /> <b><u>Graphs</u></b><br /> <div class="bbImageWrapper js-lbImage" title="212cw15.png" data-src="https://www.physicsforums.com/attachments/212cw15-png.166574/" data-lb-sidebar-href="" data-lb-caption-extra-html="" data-single-image="1"> <img src="https://www.physicsforums.com/attachments/212cw15-png.166574/" data-url="" class="bbImage" data-zoom-target="1" style="" alt="212cw15.png" title="212cw15.png" width="712" height="321" loading="lazy" decoding="async" /> </div><br /> <br /> <u><b>Part(d)</b></u><br /> <br /> At r = b, \vec{E} = -\nabla V<br /> (\frac {\partial {V_{out}}}{\partial {r}} - \frac{\partial {V_{in}}}{\partial {r}}) = -\frac {σ_b}{ε_0}<br /> (\frac {-bø_0}{2b^2}) = -\frac {σ}{ε_0}<br /> σ_b = \frac {ø_0ε_0}{2b}<br /> <br /> For r = a,<br /> (\frac {\partial {V_{a,out}+V_{b,in}}}{\partial r} - \frac {\partial {V_{a,out}+V_{b,in}}}{\partial r}) = 0<br /> So σ_a = 0<br /> <br /> Energy = \frac{1}{2} ε_0 \int_{a}^{c} E^2 dV = \frac {1}{2} ε_0 \int_b^c \frac {bø_0}{2r^2} dr = \frac {1}{4}ε_0bø_0(\frac {c-b}{bc})
 
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