Schrodinger equation: Nonlinear Function
Created: May 08, 2020
Modified: May 16, 2020

Schrodinger equation

This page is from my personal notes, and has not been specifically reviewed for public consumption. It might be incomplete, wrong, outdated, or stupid. Caveat lector.
  • Basic of quantum mechanics from Wikipedia:
    • The quantum state of a system is a ray (equivalence class of vectors) in a separable (has a countable basis -> isomorphic to 2\ell^2) Hilbert space.
    • The Hilbert space associated with a composite system is the tensor product of spaces associated with the individual systems.
    • A physical observable is defined by a Hermitian matrix on H. Its expected value in a state represented by unit vector ψH\psi\in H is ψAψ\langle \psi | A | \psi \rangle.
    • Somehow??? this implies a probability measure on values of A.
      • The Born rule. For any self-adjoint operator AA with discrete spectrum, the value measured from a normalized wavefunction is always one of the eigenvalues of AA, λi\lambda_i, measured with probability ψλiλiψ\langle \psi | \lambda_i \rangle\langle \lambda_i | \psi \rangle where λi|\lambda_i \rangle is the corresponding eigenvector of AA.
    • Technical point: the wavefunction is normalized in the sense that ψ(t)2=ψ(t)(x)2dx=1\|\psi(t)\|_2 = \int |\psi(t)(x)|^2 dx = 1. That is, at any given time tt we have a specific wave function \psi(t)(x), and its squared amplitude at any state xx gives a probability density. So: the wave function itself is a unit vector in the Hilbert space of wave functions.
  • The Schrodinger picture of quantum mechanics says that state vectors ψ(t)| \psi(t) \rangle evolve over time. The time evolution of the system is a function from real-valued tt to state vectors ψ(t)|\psi(t)\rangle. This function is defined by a differential equation, the Schrodinger equation:
iddtψ(t)=Hψ(t)i \hbar \frac{d}{dt} | \psi(t) \rangle = H | \psi(t) \rangle

where \hbar is the Planck constant, and HH is a self-adjoint operator called the 'Hamiltonian' such that ψHψ\langle \psi | H | \psi \rangle is the total kinetic + potential energy of state ψ\psi.

  • If the system is stationary then we can use the time-independent form of the Schrodinger equation:
Hψ=EψH|\psi\rangle = E | \psi \rangle

where EE is a constant energy level.