Expand the wavefunction in the complete orthonormal energy eigenstates. The Time-dependent Schrödinger equation makes each coefficient satisfy , so
The series is interpreted in the Hilbert space norm. Its norm is conserved because the phase factors have modulus one and the energy eigenstates are orthonormal. For initial data in the domain of the Hamiltonian operator, this is a strong solution of the equation; for any square-summable coefficients it gives the corresponding unitary time evolution.
In the two-dimensional span of the first two energy eigenstates, the measured observable has matrix . Its square is , and its trace is zero, giving eigenvalues . The orthogonal complement has eigenvalue zero. Thus the full spectrum is .
The normalized eigenstates for and are respectively
The lowest measurement outcome prepares up to an irrelevant overall phase. The subsequent unitary time evolution gives
By the Born rule, the probability of measuring the lowest eigenvalue again is the squared projection onto its one-dimensional eigenspace:
This is the two-level quantum return probability with . At the probability is one; if the two energies happen to be equal it remains one for every time.

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