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Flux Through a Slice of Ball

Irodov 3.21DifficultyDifficulty 2 of 5UniquenessUniqueness 3 of 5

Problem Irodov 3.21

A ball of radius RR carries charge spread uniformly through its volume with density ρ\rho. A plane at distance r0<Rr_0 < R from the ball’s centre cuts the ball in a flat circular section. Find the flux of the electric field through this section.

The ball in a section through its centre O, perpendicular to the cutting plane; the plane, seen edge-on as the dashed line, is r_0 from O and cuts the ball in a circular disc.

The ball in a section through its centre OO, perpendicular to the cutting plane; the plane, seen edge-on as the dashed line, is r0r_0 from OO and cuts the ball in a circular disc.

Given
  • RR
  • ρ\rho
  • r0<Rr_0 < R
Find
the flux Φ\Phi of E\vect E through the section

Solution

Step 1The field inside the ball

By symmetry the field is radial and of the same magnitude all over a concentric sphere of radius r<Rr < R, which encloses the charge 4πr3ρ/34\pi r^3\rho/3. Gauss’s law on it:

E⋅4πr2=4πr3ρ3ε0E\cdot 4\pi r^2 = \frac{4\pi r^3\rho}{3\varepsilon_0}

so at a point with position vector r\vect r from the centre

E=ρ3ε0 r(1) \vect E = \frac{\rho}{3\varepsilon_0}\,\vect r \tag{1}
Step 2The normal component on the section
A point P of the section at distance r from O. The radial field E resolved along the section and along its normal, E_n (drawn for ρ > 0).

A point PP of the section at distance rr from OO. The radial field E\vect E resolved along the section and along its normal, EnE_n (drawn for ρ>0\rho > 0).

Take the unit normal n\vect n of the section pointing away from the centre. Every point of the section lies at the same distance r0r_0 from the centre along n\vect n, so the normal part of its position vector is the same for all of them:

r⋅n=r0\vect r\cdot\vect n = r_0

Projecting (1) on n\vect n:

En=ρ3ε0 r⋅n=ρr03ε0(2) E_n = \frac{\rho}{3\varepsilon_0}\,\vect r\cdot\vect n = \frac{\rho r_0}{3\varepsilon_0} \tag{2}
Step 3Add up over the section

The section is a disc of radius R2−r02\sqrt{R^2 - r_0^2}, so its area is

S=π (R2−r02)S = \pi\,(R^2 - r_0^2)

With the constant normal component (2), the flux is that component times the area:

Φ=EnS=ρr03ε0⋅π (R2−r02)\Phi = E_n S = \frac{\rho r_0}{3\varepsilon_0}\cdot\pi\,(R^2 - r_0^2)
Φ=πρ r0 (R2−r02)3ε0\Phi = \frac{\pi\rho\, r_0\,(R^2 - r_0^2)}{3\varepsilon_0}
(3)

For ρ>0\rho > 0 the flux is outward, in the direction away from the centre.

Check

Both ends vanish as they should: at r0=0r_0 = 0 the section passes through the centre, where the radial field lies in the plane and crosses it nowhere; at r0=Rr_0 = R the section shrinks to a point. Units: ρr0/ε0\rho r_0/\varepsilon_0 is a field (the uniform-ball field ρr/(3ε0)\rho r/(3\varepsilon_0) has the same form), and a field times an area is a flux.

Remark

The flux is largest for an intermediate cut: setting dΦ/dr0d\Phi/dr_0 to zero gives R2−3r02=0R^2 - 3r_0^2 = 0, so the best cut is at r0=R/3r_0 = R/\sqrt 3. A cut near the centre is large but the field there barely crosses it; a cut near the surface is crossed steeply but has little area.