Calculation the resistance of a spherical shape

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The discussion focuses on calculating the resistance of nested spherical shells using Ohm's law. It highlights the relationship between current density, electric field, and potential, with the potential expressed as V = C/r + D, where C and D are constants. The electric field is radially directed, and the flux remains constant due to the absence of charges inside the conductor. The potential difference between two points is derived, leading to the formula for resistance, R = (b-a)/(4πabσ). The original poster concludes that their question is resolved.
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hello there!
I was reading about ohm rule in a MIT physics course and they calculate the resistance of a nested spherical shells like this :

attachment.php?attachmentid=27628&stc=1&d=1282143758.jpg


and they but the microscopic form of ohm's law which is :
J=\sigma_q E
and
I=A J
so
I=(4 \pi r^2 ) (\sigma_q E)
and
E=-\frac{\partial V}{\partial r}
and he said that the potential must be like this form
V=\frac{C}{r}+D
where : C and D are constant .
so my question is what is this form and why he did that and i could calculate the potential easily :
V_{ab}=\int E . dr.
thank you
 

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For symmetry, the electric field is directed radially. Since there are no charges inside the conductor, the flux

\Phi=4\pi r^2 E

must be constant. The difference of potential between a and b is

\Delta V=\int_a^b\frac{\Phi dr}{4\pi r^2}=\frac{\Phi(b-a)}{4\pi ab}.

But, as you said, I=\sigma\Phi, so

\Delta V=\frac{I(b-a)}{4\pi ab\sigma}\equiv RI

and hence

R=\frac{(b-a)}{4\pi ab\sigma}
 
thank you i think it is solved now .
 
It may be shown from the equations of electromagnetism, by James Clerk Maxwell in the 1860’s, that the speed of light in the vacuum of free space is related to electric permittivity (ϵ) and magnetic permeability (μ) by the equation: c=1/√( μ ϵ ) . This value is a constant for the vacuum of free space and is independent of the motion of the observer. It was this fact, in part, that led Albert Einstein to Special Relativity.
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