time-dependent Schrödinger equation
The time-dependent Schrödinger equation is the full, general version of Schrödinger's law. It states that the wavefunction's rate of change in time equals the Hamiltonian acting on the wavefunction, multiplied by a factor involving the imaginary unit and Planck's constant. In symbols it is written iℏ ∂ψ/∂t = Ĥψ, and it applies whether or not the system has a definite energy.
This is the equation you reach for whenever something is actually happening: a wave packet spreading out, an electron sloshing between two atoms, a spin flipping under a changing magnetic field. Because it is first order in time, knowing the wavefunction at one instant fixes it for all later instants — quantum evolution carries no hidden extra information beyond the present state.
Its solutions are smooth, continuous, and reversible: run the clock backward and the equation works equally well. The imaginary factor of i is what makes the wavefunction oscillate rather than simply grow or decay, giving quantum systems their wavelike, interfering behaviour rather than the exponential settling you see in ordinary diffusion.
The general law of quantum motion, written out with kinetic and potential energy terms.
Despite the lone factor of i, the equation conserves total probability: |ψ|² integrated over all space stays equal to one for all time. The imaginary unit governs phase, not a loss or gain of probability.