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beginner · Physics · The Schrödinger Equation (Intro)

The Hamiltonian

In classical mechanics the total energy of a particle is the sum of its kinetic and potential energies. In quantum mechanics that same quantity is promoted to an operator — the Hamiltonian H^\hat{H} — and it plays a central role in the time-dependent Schrödinger equation:

iΨt=H^Ψ.i\hbar \frac{\partial \Psi}{\partial t} = \hat{H}\,\Psi.

The equation says: the Hamiltonian acting on the wave function tells you how the wave function changes in time. Everything about the dynamics of a quantum system is encoded in H^\hat{H}.

Building the Hamiltonian from classical energy

For a single particle of mass mm moving in one dimension under a potential V(x,t)V(x, t), the classical total energy is

E=p22m+V(x,t).E = \frac{p^2}{2m} + V(x, t).

Quantum mechanics replaces the momentum pp with the momentum operator

p^=ix,\hat{p} = -i\hbar \frac{\partial}{\partial x},

so p2p^2 becomes p^2=22/x2\hat{p}^2 = -\hbar^2 \partial^2/\partial x^2. Substituting gives the explicit form of the Hamiltonian:

H^=22m2x2+V(x,t).\hat{H} = -\frac{\hbar^2}{2m}\frac{\partial^2}{\partial x^2} + V(x, t).

This is the operator that appears on the right-hand side of the Schrödinger equation. The first term is the kinetic energy operator; the second is the potential energy operator.

The Hamiltonian is the total-energy operator

The key identification is this: the eigenvalues of H^\hat{H} are the allowed total energies of the system. If a wave function ψ\psi satisfies

H^ψ=Eψ\hat{H}\,\psi = E\,\psi

for some real number EE, then ψ\psi is an energy eigenstate and EE is the corresponding energy. In a state that is not an energy eigenstate, the Hamiltonian still determines how the state evolves in time, but a measurement of energy can yield any of the eigenvalues with probabilities set by the Born rule.

Why the Hamiltonian is special

Among all observables, H^\hat{H} is unique because it appears explicitly in the equation of motion. For any observable A^\hat{A} that does not depend on time, the Ehrenfest theorem gives

ddtA^=i[H^,A^],\frac{d}{dt}\langle \hat{A} \rangle = \frac{i}{\hbar}\langle [\hat{H}, \hat{A}] \rangle,

where [H^,A^]=H^A^A^H^[\hat{H}, \hat{A}] = \hat{H}\hat{A} - \hat{A}\hat{H} is the commutator. If [H^,A^]=0[\hat{H}, \hat{A}] = 0, the expectation value of A^\hat{A} is constant in time — it is a conserved quantity. Energy itself is conserved whenever H^\hat{H} does not depend explicitly on time, because [H^,H^]=0[\hat{H}, \hat{H}] = 0 identically.

This mirrors the classical result: in Hamiltonian mechanics, any quantity that Poisson-commutes with the Hamiltonian is conserved. The quantum commutator plays the same role as the classical Poisson bracket, and the Hamiltonian is the generator of time evolution in both frameworks.

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