Using the position as an independent variable, and time as the dependent
variable, we derive the function P(Β±), which generates the space
evolution under the potential V(q) and Hamiltonian H.
Canonically conjugated variables are the time and minus the Hamiltonian. While
the classical dynamics do not change, the corresponding quantum operator
naturally leads to a 1/2βfractional time evolution, consistent with a
recently proposed spacetime symmetric formalism of quantum mechanics. Using
Dirac's procedure, separation of variables is possible, and while the coupled
position-independent Dirac equations depend on the 1/2-fractional derivative,
the coupled time-independent Dirac equations (TIDE) lead to positive and
negative shifts in the potential, proportional to the force. Both equations
couple the (Β±) solutions of P^(Β±) and the kinetic energy
K0β is the coupling strength. We obtain a pair of coupled states for
systems with finite forces. The potential shifts for the harmonic oscillator
(HO) are Β±βΟ/2, and the corresponding pair of states are coupled
for K0βξ =0. No time evolution is present for K0β=0, and the
ground state with energy βΟ/2 is stable. For K0β>0, the
ground state becomes coupled to the state with energy ββΟ/2, and
\textit{this coupling} allows to describe higher excited states. Energy
quantization of the HO leads to quantization of K0β=kβΟ
(k=1,2,β¦). For the one-dimensional Hydrogen atom, the potential shifts
become imaginary and position-dependent. Decoupled case K0β=0 leads to
plane-waves-like solutions at the threshold. Above the threshold, we obtain a
plane-wave-like solution, and for the bounded states the wave-function becomes
similar to the exact solutions but squeezed closer to the nucleus.Comment: 11 pages, 6 figure