[Return to Physics Homepage]     [Return to Mike Coombes' Homepage]     [Return to List of Handouts]     [Return to List of Notes and Examples]

Electric Field Due to a Charge Distribution


We consider a volume (or line or area, as appropriate) element of the object. We set an origin and determine the location of the field point P and source point S in rectilinear coordinates.

The electric field due to the element is given by

dE = (kdq/a3) a .

Note that a = P - S. Express a in rectilinear coordinates.

The element chosen should reflect the symmetry of the object - linear, rectilinear, polar, cylindrical, or spherical. This makes the limits of integration easier to find.

The angle α will occur in your solution since dEx = dEcos(α) and dEy = dEsin(α). Recall that

cos(α) = (a • P) / |a| |P| ,

and

sin(α) = (a × P) / |a| |P| .

By doing the dot and cross products, cos(α) and sin(α) can be expressed in simpler form.

The charge element dq is related to the element of integration by the charge density

dq = λds lines and arcs
dq = ΣdA areas
dq = ρdV volumes

where λ, Σ, and ρ are the linear, surface, and volume charge densities respectively.

The elements of integration

Coordinate System
Elements
ds

(linear)
dA

(area)
dV

(volume)
rectilinear
(lines, rectangles, cubes)
dx, dx, dy
dx
dxdy
dxdydz
polar
(arcs, circles, pie slices)
dr, rdθ
Rdθ
rdrdθ
-
cylindrical polar
(cans, cylinders)
dz, dr, rdθ
-
Rdθdz
rdrdθdz
spherical
(balls, part of spheres)
dr, rdθ, rsin(θ)dφ
-
R2sin(θ) dθdφ
r2sin(θ) dθdφdr

Conversion to rectilinear coordinates

Coordinate System
x
y
z
Range
polar rsin(θ) rcos(θ) - 0 £ q £ 2π
-
cylindrical polar rsin(θ) rcos(θ) z 0 £ q £ 2π
-
spherical rsin(θ)cos(θ) rsin(θ)sin(θ) rcos(θ) 0 £ q £ π 0 £ f £ 2π

Example

What is the electric field at point P = (X, 0, 0) due to a disk of radius R and charge density located at the origin? Note that X > R.

The components of the electric field are dEx = dE cos(α) and dEy = -dE sin(α), where

dE = (kdq/a3) .

Now dq = rdrdθ. As well, S = (rcos(θ), rsin(θ)). Thus the vector a is

a = P - S = (X - rcos(θ), rsin(θ)) .

We also need the magnitude of a,

a = |a| = [X2 - 2Xrcos(θ) + r2]½ .

The cosine and sine are

cos(α) = (a • P) / |a| |P| = (X - rcos(θ))/a ,

and

sin(α) = (a × P) / |a| |P| = -rsin(θ)/a .

Our integrals, therefore, are

Ex = ò0 dθ ò0R dr kΣ r(X - rcos(θ))/[X2 - 2Xrcos(θ) + r2]3/2 ,

and

Ey = +ò0 dθ ò0R dr kΣ r2 sin(θ))/[X2 - 2Xrcos(θ) + r2]3/2 .


[Return to Physics Homepage]     [Return to Mike Coombes' Homepage]     [Return to List of Handouts]     [Return to List of Notes and Examples]

Questions? mike.coombes@kwantlen.ca

[Return to Kwantlen Homepage]