When the Hamiltonian is independent of time, the state function can be written as a product of a function of time and a function of position.

Substituting into the time-dependent Schrödinger equation:

Since \(\Psi\) does not depend on t and \(\hat{H}\) does not depend on either, we can take \(\Psi (q)\) from the time derivative and \(f(t)\) from the Hamiltonian.

Dividing the terms of equation (3) by \(f(t)\Psi (q)\) gives us:

The member on the left depends only on t and the one on the right only on the coordinates q. Thus, equality is only possible if both terms are equal to a constant that we will call E.

The first equation gives us the temporal evolution of the system (temporal Schrödinger equation). The second equation is the spatial or time-independent Schödinger equation.
We integrate the temporal Schrödinger equation:

where C is the constant of integration. Taking antilogarithms, the function f(t) is obtained.

The constant A can be included in the function \(\Psi (q)\) as a multiplicative factor, thus, we can write the above equation as:

Therefore, in those systems in which the Hamiltonian does not depend on t, the state function can be written:

The states of a physical system that can be written in the above way are characterized by having a constant energy and are called stationary states. Stationary states are characterized by having a probability density independent of time.

Therefore, for a system with \(\hat{H}\) independent of t, the total energy is constant and the probability that the particle has its coordinates between \(q\) and \(q+dq\) is not it changes over time.