Newton's laws of motion are three fundamental classical mechanics rules that define the relationship between an object's motion and the forces acting on it. These laws are summarised as follows:
F = dp/dt = mdv/dt = ma
There are three equations of motion that only apply to uniformly accelerated motion. The following are the equations:
Where

In the first configuration (1) as shown in the figure, four identical charges \( q_0 \) are kept at the corners A, B, C and D of square of side length \( a \). In the second configuration (2), the same charges are shifted to mid points C, E, H, and F of the square. If \( K = \frac{1}{4\pi \epsilon_0} \), the difference between the potential energies of configuration (2) and (1) is given by: