Applying Gauss' Law: Planar Symmetry — Question 4

Section 23-7 · Physics pages 3758–3759

Question 4 A uniformly charged slab produces harmonic motion inside its volume An infinite insulating slab occupies |x| < a and has fixed uniform density ρ > 0. There are no other fields. A weak particle of mass m and charge −q, with q > 0, starts at rest at x = A, where 0 < A < a. Ignore collisions and radiation. x −a a −q Edge-on view of an infinite planar slab; its transverse dimensions are unbounded. (a) Derive the interior and exterior slab fields from symmetry and Gauss law. (b) Derive the particle trajectory and period, and show that the entire orbit remains within the region where the interior expression applies.
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Question 4 - Solution A uniformly charged slab produces harmonic motion inside its volume x −a a −q (a) Method and calculation x > 0 : 2Ex(x)S = 2ρxS/ϵ0 ⇒Ex(x) = ρx/ϵ0 (|x| < a). Ex(x) = ρa ϵ0 sgn(x) (|x| > a). (b) Interpretation and further calculation m¨x = −qEx = −qρ ϵ0 x, ω = √qρ mϵ0 . x(t) = A cos ωt, T = 2π √mϵ0 qρ , |x(t)| ≤A < a. Physical check The amplitude restriction matters: a larger excursion would enter the constant-field exterior and would not remain purely harmonic.

Question 4

A uniformly charged slab produces harmonic motion inside its volume

An infinite insulating slab occupies |x|<a|x|<a and has fixed uniform density ρ>0\rho>0. There are no other fields. A weak particle of mass m and charge −q-q, with q>0q>0, starts at rest at x=Ax=A, where 0<A<a0<A<a. Ignore collisions and radiation.

Diagram shown in the original SVG worksheet.

  1. Derive the interior and exterior slab fields from symmetry and Gauss law.

  2. Derive the particle trajectory and period, and show that the entire orbit remains within the region where the interior expression applies.

Question 4 - Solution

A uniformly charged slab produces harmonic motion inside its volume

Diagram shown in the original SVG worksheet.

(a) Method and calculation

x>0:2Ex(x)S=2ρxS/ϵ0⇒Ex(x)=ρx/ϵ0(|x|<a).x>0:\quad 2E_x(x)S=2\rho xS/\epsilon_0\Rightarrow E_x(x)=\rho x/\epsilon_0\quad(|x|<a).Ex(x)=ρaϵ0sgn⁡(x)(|x|>a).E_x(x)=\frac{\rho a}{\epsilon_0}\operatorname{sgn}(x)\quad(|x|>a).

(b) Interpretation and further calculation

mẍ=−qEx=−qρϵ0x,ω=qρmϵ0.m\ddot x=-qE_x=-\frac{q\rho}{\epsilon_0}x,\quad\omega=\sqrt{\frac{q\rho}{m\epsilon_0}}.x(t)=Acos⁡ωt,T=2πmϵ0qρ,|x(t)|≤A<a.x(t)=A\cos\omega t,\quad T=2\pi\sqrt{\frac{m\epsilon_0}{q\rho}},\quad|x(t)|\le A<a.

Physical check

The amplitude restriction matters: a larger excursion would enter the constant-field exterior and would not remain purely harmonic.