The field E at a point r caused by
a distributed charge density ρ(r) is given by
where r' points from the origin to the element of volume dV'
and the integration is over all the space containing the charge.
If the charge is distributed over a plane then replace ρ(r')dV'
by σ(r')da'. Similarly, for a line of charge replace ρ(r')dV'
by λ(r')dV'.
Field lines are a common way to represent vector fields. They obey the rules
1) Lines are everywhere parallel to the field.
2) Lines start and end only on charges.
3) Field lines are more closely spaced in regions of high field and further
apart in regions of low field.
4) Field lines are elastic (stretchy, but don't like it), flexible (bendy,
but don't like it) and repulsive (they repel each other as if they were all
positively charged).
The Electric Potential difference between two points r1
and r2 is defined to be
![]()
where the integral is along a line joining r1 to r2.
If the E field is caused only by static charges then the value of the integral
does not depend on the path taken and the potential is unique. In that case
we say that the field E is conservative.
In many situations we use an absolute electric potential that is defined by
specifying a unique place at which the potential is set to zero. This is commonly
the point at infinity.
The electric potential at point r arising from a set of
charges Qi at positions ri is given
by
V(r) = ∑i Qi
4πε0|r
- ri|
Note that if the charge distribution is continuous then the sum will become
an integral over the volume containing the charge.
The field from an infinite straight line of charge with
density λ Coulombs/metre depends
only on the perpendicular distance r from the line and is given
by
E = __λ__ρ__
2πε0 |ρ|2