Calculating Potential Between Conducting Shells

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Homework Help Overview

The discussion revolves around calculating the electric potential between two conducting shells, one with an inner radius R1 and an outer radius R2. The problem involves understanding the distribution of charges Q1 and Q2 on the respective surfaces and how these affect the potential in different regions, particularly between the shells and inside the inner shell.

Discussion Character

  • Mixed

Approaches and Questions Raised

  • Participants explore the use of Gauss' Law to calculate electric fields and potentials, questioning how to account for grounded surfaces and the implications of charge distributions.

Discussion Status

The discussion is active, with various interpretations of the problem being explored. Some participants suggest using superposition principles, while others question the relationships between the charges and the implications of grounding. There is no explicit consensus on the correct approach or interpretation of the problem.

Contextual Notes

Participants note the importance of charge distributions and the grounding condition of the outer shell, which complicates the potential calculations. There is also confusion regarding the assumptions about the thickness of the shells and how that affects the electric field and potential in different regions.

  • #31
assuming this thing is ground to the earth, if we placed charge on the inner shell, wouldn't all the charge just travel to the outer shell and into the earth?
 
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  • #32
oops, yes you're right!
 
  • #33
ok i thought i was missing something there... thanks gabba
 
  • #34
gabbagabbahey said:
My advice is to exploit the spherical symmetry in the problem, by using Gauss' Law to calculate the electric field and then integrating it to find the potential.

one more thing... how do we do this using integration? (the problem with two thin shells)
 
  • #35
Do you mean directly using the integral form of Poisson's equation for a surface charge density (\sigma_i=\frac{Q_i}{4 \pi R_i^2})? Namely:

V(\vec{r})=V_1(\vec{r})+V_2(\vec{r})=\sum_{i=1,2} \frac{1}{4 \pi \epsilon_0} \int_{\mathcal{S}_i} \frac{\sigma_i}{|\vec{r}-\vec{r_i'}|} d^3 r'
 
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  • #36
I'm not sure if this makes any sense but for the potential to be zero at infinity, don't we need to integrate from infinity to the outer shell for the potential outside the outer shell (which would give 0)

then, to get the potential between R2>r>R1 we integrate from R2 to R1

using gauss law we can find the E-field in between the shells

E=\frac{kQ_1}{r^2}

then the potential would be:

V=-k Q_1 \int_{R_2}^r \frac{1}{r^2} dr

V = kQ_1 \left( \frac{1}{r} - \frac{1}{R_2} \right)
 
  • #37
I'm reading in the book that the notation for integration should be:

V=-\int_a^b \vec{E} \cdot d \vec{r}

where the field at a is higher then b

if this is the case shouldn't the integral then be switched
<br /> V=-k Q_1 \int_{r}^{R_2} \frac{1}{r^2} dr <br />

My question how do we know the integral should go from R2 to r and not the other way around?
 

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