Using the position as an independent variable, and time as the dependent variable, we derive the function ({mathcal{P}}^{(pm )}=pm sqrt{2m({mathcal{H}}-{mathcal{V}}(q))}), which generates the space evolution under the potential ({mathcal{V}}(q)) and Hamiltonian ({mathcal{H}}). No parametrization is used. Canonically conjugated variables are the time and minus the Hamiltonian ((-{mathcal{H}})). While the classical dynamics do not change, the corresponding Quantum operator ({{{hat{mathcal P}}}}^{(pm )}) naturally leads to a 1/2-fractional time evolution, consistent with a recent proposed space–time symmetric formalism of the Quantum Mechanics. Using Dirac’s procedure, separation of variables is possible, and while the two-coupled position-independent Dirac equations depend on the 1/2-fractional derivative, the two-coupled time-independent Dirac equations lead to positive and negative shifts in the potential, proportional to the force. Both equations couple the (±) solutions of ({{{hat{mathcal P}}}}^{(pm )}) and the kinetic energy ({mathcal{K}}_{0}) (separation constant) is the coupling strength. Thus, we obtain a pair of coupled states for systems with finite forces, not necessarily stationary states. The potential shifts for the harmonic oscillator (HO) are (pm {hbar {omega}} /2), and the corresponding pair of states are coupled for ({mathcal{K}}_{0}ne 0). No time evolution is present for ({mathcal{K}}_{0}=0), and the ground state with energy ({hbar {omega}} /2) is stable. For ({mathcal{K}}_{0}>0), the ground state becomes coupled to the state with energy (-{hbar {omega}} /2), and this coupling allows to describe higher excited states in the HO. Energy quantization of the HO leads to the quantization of ({mathcal{K}}_{0}=k{hbar {omega}}) ((k=1,2,ldots)). For the one-dimensional Hydrogen atom, the potential shifts become imaginary and position-dependent. Decoupled case ({mathcal{K}}_{0}=0) leads to plane-waves-like solutions at the threshold. Above the threshold (({mathcal{K}}_{0}>0)), we obtain a plane-wave-like solution, and for the bounded states (({mathcal{K}}_{0}<0)), the wave-function becomes similar to the exact solutions but squeezed closer to the nucleus.