The time-independent Schrödinger equation is the energy eigenvalue equation for the Hamiltonian operator:
Here is the reduced Planck constant. A corresponding stationary wavefunction evolves as , which follows by substitution in the Time-dependent Schrödinger equation. Its position probability density is time independent because the time factor has unit modulus. Physical energy eigenstates must also satisfy the system's boundary conditions; for a bound state, wavefunction normalization requires .
Define the reflected function . The chain rule gives and . Evaluating the time-independent Schrödinger equation for at and using the even function identity gives
Thus reflection preserves the energy eigenvalue. The same substitution in the norm gives
This is the action of the parity operator , which is a unitary operator. For a reflection-symmetric physical problem it preserves the Hamiltonian operator's operator domain as well as its differential expression.
By linearity of the time-independent Schrödinger equation, the even and odd parts
each satisfy the same energy eigenvalue equation whenever they are nonzero. They obey and , so they have definite parity. At least one is nonzero, and . Each nonzero part can be normalized separately.
Therefore a basis of stationary solutions can be chosen to have definite parity, and solving the even and odd sectors loses no energy eigenvalues. This does not assert that every possible quantum superposition has definite parity; a superposition of the two sectors need not. For one-dimensional bound states in the usual regular setting, nondegeneracy of one-dimensional bound states further implies that each individual energy eigenstate has definite parity.

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