Feynman’s Lectures on Physics: Chapter 11-6 – Newton’s Laws in Vector Notation
From three equations to one universal law One of the great achievements of Newtonian mechanics was to establish a mathematical framework capable of describing the motion of objects, from falling stones to orbiting planets. Yet the way we express these laws mathematically has an important bearing on how we understand their universality. In Chapter 11-6 of The Feynman Lectures on Physics , Richard Feynman brings together the ideas developed in the preceding sections on vectors, vector addition and rotations to show how Newton’s laws can be expressed in a form that is independent of our choice of coordinate system. The central idea is deceptively simple: Newton’s laws are not fundamentally statements about motion along the x, y and z axes. They are statements about physical quantities in space. By expressing them using vectors, we can write a single law that applies equally well regardless of how we orient our coordinate system. Acceleration as a vector We are accustomed to thinking of...