Deriving Key SHM Relationships
One of the most useful equations in SHM is v = ±ω√A2−y2, which connects velocity to position at any moment. The derivation uses the trigonometric identity sin²θ + cos²θ = 1, transforming the basic equations into this practical form.
This equation tells you something fascinating: as displacement increases, velocity must decrease. At the extreme positions y=±A, velocity becomes zero, whilst at equilibrium y=0, velocity reaches its maximum value of ±ωA.
For pendulums, the period formula T = 2π√l/g only works for small angles. This is crucial for A-level problems - large amplitude pendulum swings don't follow simple harmonic motion.
Pro tip: The ± sign in the velocity equation accounts for direction - the object can be moving towards or away from equilibrium at any given displacement.