Gauss' Law and Coulomb's Law — Question 7

Section 23-4 · Physics pages 3704–3705

Question 7 A dipole has zero closed flux while transferring flux between hemispheres A compact ideal dipole has moment pˆz. On a sufficiently distant centered sphere of radius R its radial field is Er = 2kp cos θ/R3. Treat this leading dipole field as the model. Here k = 1/(4πϵ0). R p Cross-section of concentric spherical surfaces; labels specify radii. (a) Integrate its total outward flux and relate the result to the total dipole charge. (b) Find the northern hemisphere flux and its dependence on R. Explain why zero whole-sphere flux does not force each open-surface flux to vanish.
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Question 7 - Solution A dipole has zero closed flux while transferring flux between hemispheres R p (a) Method and calculation Φ = 2kp R ∫2π 0 dϕ ∫π 0 cos θ sin θ dθ = 0. Qdipole = +q −q = 0. (b) Interpretation and further calculation ΦN = 4πkp R ∫π/2 0 cos θ sin θ dθ = 2πkp R . ΦS = −ΦN, ΦN(2R) = 1 2ΦN(R). The two hemispheres exchange equal signed contributions even though each generally has nonzero flux. Physical check The open-hemisphere flux falls as 1/R because dipole field falls as 1/R3 while area grows as R2.

Question 7

A dipole has zero closed flux while transferring flux between hemispheres

A compact ideal dipole has moment p𝒛̂p\hat{\mathbf z}. On a sufficiently distant centered sphere of radius R its radial field is Er=2kpcos⁡θ/R3E_r=2kp\cos\theta/R^3. Treat this leading dipole field as the model. Here k=1/(4πϵ0)k=1/(4\pi\epsilon_0).

Diagram shown in the original SVG worksheet.

  1. Integrate its total outward flux and relate the result to the total dipole charge.

  2. Find the northern hemisphere flux and its dependence on R. Explain why zero whole-sphere flux does not force each open-surface flux to vanish.

Question 7 - Solution

A dipole has zero closed flux while transferring flux between hemispheres

Diagram shown in the original SVG worksheet.

(a) Method and calculation

Φ=2kpR∫02πdϕ∫0πcos⁡θsin⁡θdθ=0.\Phi=\frac{2kp}{R}\int_0^{2\pi}\!d\phi\int_0^\pi\cos\theta\sin\theta\,d\theta=0.Qdipole=+q−q=0.Q_{\mathrm{dipole}}=+q-q=0.

(b) Interpretation and further calculation

ΦN=4πkpR∫0π/2cos⁡θsin⁡θdθ=2πkpR.\Phi_N=\frac{4\pi kp}{R}\int_0^{\pi/2}\cos\theta\sin\theta\,d\theta=\frac{2\pi kp}{R}.ΦS=−ΦN,ΦN(2R)=12ΦN(R).\Phi_S=-\Phi_N,\quad\Phi_N(2R)=\tfrac12\Phi_N(R).The two hemispheres exchange equal signed contributions even though each generally has nonzero flux.

Physical check

The open-hemisphere flux falls as 1/R1/R because dipole field falls as 1/R31/R^3 while area grows as R2R^2.