The Setup
A Repulsive Push
Imagine you are holding a tiny positive charge q near an infinitely long, positively charged wire. The wire has a uniform linear charge density λ. Because like charges repel, the moment you let go of the charge from its initial distance r0, it will accelerate outwards.
Our mission is to find out how its speed v depends on its distance r from the wire at any given instant. To do this, we must first understand the environment the charge is moving through. By applying Gauss's Law to a cylindrical surface around the wire, we know that the electric field E at any radial distance x is given by:
The Variable Force and Work Done
As the charge moves, it experiences an electrostatic force F=qE. Substituting our electric field expression, the force becomes:
Notice a crucial detail here: the force is not constant. It is inversely proportional to the distance x. Because the force changes continuously as the particle moves, we cannot rely on our standard constant-acceleration kinematic equations (like v2=u2+2as). Instead, we must use the power of calculus to find the work done.
For an infinitesimally small displacement dx, the tiny amount of work done dW by the electric field is simply Fdx. To find the total work done W as the charge moves from its starting point r0 to a new distance r, we integrate this expression:
Pulling the constants out of the integral, we are left with the integral of 1/x, which evaluates to the natural logarithm ln(x):
W=2πϵ0qλ[lnx]r0r=2πϵ0qλ(lnr−lnr0)
Using the properties of logarithms, we can condense this beautifully into:
The Work-Energy Connection
Now, we ask ourselves: what does this work actually do? According to the Work-Energy Theorem, the net work done on an object translates directly into a change in its kinetic energy (ΔK).
Since the charge was released from rest, its initial kinetic energy was zero. Therefore, the final kinetic energy is simply 21mv2. Equating the work done to this kinetic energy gives us our master equation:
We are looking for a proportionality relationship for the speed v. If we strip away all the constants (like mass m, charge q, λ, and ϵ0), we can clearly see how v2 depends on the spatial variables:
Taking the square root of both sides reveals the final, elegant truth of the particle's motion:
This tells us that while the particle continues to speed up as it moves away, its rate of acceleration drops drastically, governed by the slow growth of the square root of a natural logarithm.