Gauss' Law and Coulomb's Law — Question 4

Section 23-4 · Physics pages 3698–3699

Question 4 Displacing a charge inside a sphere preserves flux but destroys constant field A positive charge q lies a distance b from the center of a spherical Gaussian surface of radius R, with 0 < b < R. The near and far poles lie on the displacement axis. Here k = 1/(4πϵ0). R q O Cross-section of concentric spherical surfaces; labels specify radii. (a) Find the outward normal fields at the two poles and their ratio. (b) Evaluate that ratio for b = R/2, then find the total flux. Explain why either pole field times 4πR2 gives the wrong total.
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Question 4 - Solution Displacing a charge inside a sphere preserves flux but destroys constant field R q O (a) Method and calculation En,near = kq (R −b)2 , En,far = kq (R + b)2 . En,near En,far = (R + b R −b )2 . (b) Interpretation and further calculation b = R/2 : En,near/En,far = 9. Φ = q/ϵ0. The charge is still enclosed, but the sphere is not centered on the source. Neither constant magnitude nor a radial field relative to the sphere center can be assumed. Physical check Both pole contributions are outward for an interior positive charge, although their magnitudes differ.

Question 4

Displacing a charge inside a sphere preserves flux but destroys constant field

A positive charge q lies a distance b from the center of a spherical Gaussian surface of radius R, with 0<b<R0<b<R. The near and far poles lie on the displacement axis. Here k=1/(4πϵ0)k=1/(4\pi\epsilon_0).

Diagram shown in the original SVG worksheet.

  1. Find the outward normal fields at the two poles and their ratio.

  2. Evaluate that ratio for b=R/2b=R/2, then find the total flux. Explain why either pole field times 4πR24\pi R^2 gives the wrong total.

Question 4 - Solution

Displacing a charge inside a sphere preserves flux but destroys constant field

Diagram shown in the original SVG worksheet.

(a) Method and calculation

En,near=kq(R−b)2,En,far=kq(R+b)2.E_{n,\mathrm{near}}=\frac{kq}{(R-b)^2},\quad E_{n,\mathrm{far}}=\frac{kq}{(R+b)^2}.En,nearEn,far=(R+bR−b)2.\frac{E_{n,\mathrm{near}}}{E_{n,\mathrm{far}}}=\left(\frac{R+b}{R-b}\right)^2.

(b) Interpretation and further calculation

b=R/2:En,near/En,far=9.b=R/2:\quad E_{n,\mathrm{near}}/E_{n,\mathrm{far}}=9.Φ=q/ϵ0.\Phi=q/\epsilon_0.The charge is still enclosed, but the sphere is not centered on the source. Neither constant magnitude nor a radial field relative to the sphere center can be assumed.

Physical check

Both pole contributions are outward for an interior positive charge, although their magnitudes differ.