![]() So I’ll talk about it probably next time near the end, depending on how much time there is. There are some things left, of course, that we won’t do, but this goes a long way. That’s like saying if I can do Einstein’s relativistic kinematics at low velocities, I will regain Newtonian mechanics. ![]() ![]() It contains Newton’s laws as part of it, because if you can do the quantum theory, you can always find hidden in it the classical theory. That’s called the Schrödinger equation, and just about anything you see in this room, or on this planet, anything you can see or use is really described by this equation I’m going to write down today. Professor Ramamurti Shankar: All right, today’s topic is the theory of nearly everything, okay? You wanted to know the theory of everything? You’re almost there, because I’m finally ready to reveal to you the laws of quantum dynamics that tells you how things change with time. Fundamentals of Physics II PHYS 201 - Lecture 24 - Quantum Mechanics VI: Time-Dependent Schrödinger EquationĬhapter 1: The “Theory of Nearly Everything”
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