| Questions: | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 |
We calculate the potential by direct integration in much the same way that we calculate the electric field. The exception is that potential is a scalar quantity and that dV = k dq/r.
The shape of the object suggests the use of polar coordinates for the integration variables. The diagram below shows the origin and coordinate system that I have chosen.

Note that r has both x and y components. The source point is given by S = i Rcos(θ) + j Rsin(θ). The field point is P = j y. Thus r = P S = i Rcos(θ) j [Rsin(θ) + y]. The distance from source to field point is given r = |r| = {R2 + y2 + 2Rysin(q )}½. Therefore the potential
dv = kl Rdq /{R2 + y2 + 2Rysin(q )}½ .
The integral is evaluated from θ = 0 to θ = π. The integral for the total potential is therefore
V = kλR ò0p dq / {R2 + y2 + 2Rysin(q )}½ . (1)
Unfortunately the integral does not have a simple solution but may be solved numerically if desired.
The gradient along the y direction is Ey = j dV/dy. Taking the derivative of equation (1) yields
Ey = j kλR ò0p dθ (y + Rsin(q ))/{R2 + y2 + 2Rysin(q )}3/2 .
If we take the limit as y goes to zero, we find
Ey = j (kl/R) ò0p dθ sin(q ) = j 2kl/R .
As we had before.

We calculate the potential by direct integration in much the same way that we calculate the electric field. The exception is that potential is a scalar quantity and that dV = kdq/r.
The shape of the object suggests the use of polar coordinates for the integration variables. The diagram below shows the origin and coordinate system that I have chosen.

Note that b has both x and y components. The source point is given by S = i rcos(θ) + j rsin(θ). The field point is P = i a. Thus b = P S = i [a rcos(θ)] + j rsin(θ). The distance from source to field point is given b = |b| = {r2 + a2 2arcos(q )}½. Therefore the potential
dV = ks rdrdq /{r2 + a2 2arcos(q )}½ .
The variables of integration range from r = 0 to r = R and q = 0 to q = 2π . Therefore the total potential is
V = ks ò02π dq ò0R dr r /{r2 + a2 2arcos(q )}½.
Again the integral is messy to try and solve.

In both cases the setup is the same. We select a tiny piece of the surface which has charge dq = s R2sinq dq df . We assume it is at some position S = ix + jy + kz. Expressing x, y, and z in spherical coordinates, we have
S = iR sinq cosf + jR sinq sinf + kR cosq .
Hence, r = P S becomes
r = iR sinq cosf jR sinq sinf + k(a R cosq ) .
The magnitude of r is
|r|2 = |P|2 + |S|2 2PS = a2 + R2 2aR cosq .
The small portion of electric potential is
dV = kdq / r
which we need to integrate over the entire surface of the sphere.

The integral over f gives 2π . The integral over q is exact but we must be careful of the two cases. We find

The potential depends only on the distance from the centre of the shell. To find the electric field, we use E = ÑV which reduces to E = a ∂V/∂a in the case of radial symmetry. Here a is the unit radial vector. We find (after changing a to r)


There is no clear-cut symmetry here. The key to solving this problem is to break the object into two simpler pieces, with obvious symmetry, as shown below

The flat back piece exhibits Cartesian symmetry and the front piece has cylindrical symmetry. We do the back first.

We select a tiny piece of the surface which has charge dq = s dxdz. We assume it is at some position S = ix + kz. The field point is P = jd.
Hence, r = P S becomes
r = ix + jd kz .
The magnitude of r is
r = |r| = [x2 + d2 + z2]½ .
The small portion of the electric potential is
dV = kdq/r
which we need to integrate over the entire surface of the plate. Thus

Next we consider the cylindrical piece.

We select a tiny piece of the surface which has charge dq = s Rdq dz. We assume it is at some position S = ix + jy + kz. Expressing x, y, and z in cylindrical coordinates, we have
S = i R cosq + j R sinq + k z .
Hence, r = P S becomes
r = i R cosq + j (d R sinq ) k z .
The magnitude of r is
r = |r| = d2 + R2 + z2 2dR sinq .
The small portion of electric potential is
dV = kdq/r
which we need to integrate over the entire surface of the half-cylinder.


We select a tiny piece of the volume which has charge dq = ρ rsinq drdq dz. We assume it is at some position S = ix + jy + kz. Expressing x, y, and z in cylindrical coordinates, we have
S = i r cosq + j r sinq + k z .
Hence, G = P S becomes
G = i r cosq + j (d r sinq ) k z .
The magnitude of G is
G = |G| = d2 + r2 + z2 2dr sinq .
The small portion of electric field is dV = kdq/G which we need to integrate over the entire surface of the half-cylinder.


The fact that the electric field drops as 1/r2 for large r indicates that we are dealing with spherical symmetry not cylindrical. Notice the jumps in E at r = R, r = 2R, and r = 3R. This only occurs when we cross a shell of charge at each radius. There is no charge between the shells since again the field drops as 1/r2. There is obviously no charge inside the first shell since E is zero. The first shell must have charge Q. Now Gauss' Law for spherical charge distributions reduces to
E(r) = Qinside / 4πε0r2 . (1)
At r = 2R, Qinside = Q1 + Q2 = Q + Q2. Also from the graph we know, E(2R) = Q/4πε0R2. Substituting this information in Eq. (1), we have
Q/4πε0R2 = (Q + Q2)/4πε0(2R)2 ,
or, eliminating common factors,
Q = (Q + Q2)/4 .
We thus have Q2 = 3Q.
We repeat this approach at the next shell. At r = 3R, Qinside = Q1 + Q2 + Q3 = 4Q + Q3. Also from the graph we know, E(3R) = Q/4πε0R2. Substituting this information in Eq. (1), we have
Q/4πε0R2 = (4Q + Q3)/4πε0(3R)2 ,
or, eliminating common factors,
Q = (4Q + Q3)/9 .
We thus have Q3 = 5Q.

The fact that there is a drop in the electric field at r = 2R indicates a charged cylindrical shell at that point. The fact that the electric field drop to zero indicates that the total charge between 0 and 2R is zero from Gauss' Law. The fact that the field drops as 1/r between R and 2R indicates a vacuum, as this is the typical drop in the electric field as you move away from a long charged cylinder. The fact that the field rises between 0 and R tells us that the charge is spread out over the volume of the cylinder. Gauss' Law for uniform charge distributions is
E(r) = Qinside/2πε0rL ,
usually written
E(r) = l/2πε0r ,
where l = Qinside/L. Now
Qinside = ò inside ρ dV = 2πL ò 0r ρ(a) a da ,
where a is our radial variable of integration. Thus we have
E(r) = (1/ε 0r) ò 0r ρ (a) a da . (2)
We are trying to find a form of ρ (a) that will yield are r2 behaviour in E. The presence of 1/r outside the integral, indicates that the integral must produce an r3 result. This in turn requires that ρ (a) = Ca where C is a constant. Using this form we evaluate Eq. (2) and find
E(r) = Cr2/3ε0 .
We know E(R) = l/2πε0R, therefore C = 3l/2πR3 and ρ(r) = 3lr/2πR3. The outside shell must have linear charge density l.

The fact that the potential drops as 1/r for large r indicates that we are dealing with spherical symmetry not cylindrical. Notice the change in the slope of V at r = 2R. This only occurs when we cross a shell of charge at that radius. There is also a change in the slope of V at r = R so there is surface charge there as well. The flat region from R to 2R of constant potential occurs for volumes with zero electric field so this regions is uncharged space. The rising potential from r = 0 to r = R indicates some charge distribution. Thus what we have is a sphere of radius R with unknown charge density ρ . On the surface of that sphere is some unknown charge density sR. Then there is a gap followed by a shell with surface density s2R as shown below.

We know that the potential outside any charged sphere with radial symmetry is V = Qtotal/4πε0r. At r = 2R, the graph says V = Q/8πε0R. So here the total charge enclosed must be Q. Therefore, using Gauss' Law
Qsphere + sR4πR2 + s2R4π(2R)2 = Q . (1)
Inside R, the potential must be given by
V = Cr2 . (2)
To find the constant C, we compare Eq. (2) with the value of V at r = R from the graph
CR2 = Q/8πε0R . (3)
We find that C = Q/8πε0R3. Hence
V(r) = Qr2/8πε0R3 . (4)
To find Qsphere, sR, and s2R, we need to use the boundary conditions at R and 2R. At R,
∂V/∂ r|R+ ∂V/∂r|R- = sR/ε0 .
Above r = R, we know ∂V/∂r|R+ = 0 since the potential is flat. Below r = R, ∂V/∂r|R- = Q/4πε0R2 using Eq. (4). Hence sR = -Q/4πR2. Repeating for r = 2R,
∂V/∂r|2R+ ∂V/∂r|2R- = s2R/ε0 .
Above r = 2R we know from the graph that V(r) = Q/4πεor. Thus ∂V/∂r|2R+ = Q/16πε0R2. Below r = 2R, the potential is flat and ∂V/∂r|2R- = 0. Thus s2R = Q/16πR2. We can now find Qsphere by substituting these results back into Eq. (1),
Qsphere + (-Q/4πR2)4πR2 + (Q/16πR2)4π(2R)2 = Q . (5)
Hence Qsphere = Q. The inner shell has charge - Q and the outer shell has charge +Q. The charge density in the sphere is thus ρ = Q/(4πR3/3).
Questions? mike.coombes@kwantlen.ca