In quantum chemistry, linear combinations of atomic orbitals (LCAO) have long been used to construct molecular orbitals. This Demonstration considers the Bohm trajectories of two initially separated excited metastable hydrogen atoms, separated by an internuclear distance . Keep in mind that in this special case, the standard LCAO method must be adjusted to fit, and it does not give exact solutions to the Schrödinger equation, but only first approximations. The most stable electronic state of an atom is called the ground state. An excited atom, which is called a Rydberg atom (with a very high principal quantum number ), in which the electron is not in the lowestenergy orbit, immediately emits energy in the form of light when the electron falls back into lowerenergy orbit. Metastable states are excited atoms with a long lifetime before they return to the ground state by emitting photons. An example of a metastable atom with a lifetime of about 0.12 seconds is the ( ) excited state of the hydrogen atom, which undergoes radiative decay to the ground state ( ), only by twophoton transitions [6]. As in standard treatments of the hydrogen atom, the nuclei are assumed to have infinite mass and thus remain stationary in space, with the specified internuclear distance parameter in the direction. Thus the model consists of electrons that are electrostatically attracted to the stationary protons. This approximation neglects the kinetic energy of the nuclei, and the system is approximated as two separate oneelectron molecular orbitals. In the Bohm picture, the electron acts like an actual particle, its velocity at any instant being fully determined by the gradient of the phase function, which in turn depends on the LCAO representation of the total molecular wavefunction. Dewdney and Malik [1], Holland [2] and Colijn and Vrscay [3] first examined the Bohmian trajectories associated with eigenstates for the hydrogen atom. Pauli's exclusion principle, which states that two identical electrons cannot occupy the same spinorbital within a quantum system, plays no role here since the two occupied molecular orbitals of the hydrogen molecule have opposite spins. There are four possible Bohm trajectories for two electrons in depending on the initial position , , and the internuclear distance parameter . If , you see only one electron with two possible orbits. In the interference region of the two hydrogen atoms, the component of the velocity is not equal to zero. In the graphic you see the wave density (if enabled); four possible orbits of two electrons, where one trajectory (blue) depends on the initial starting point ( , , ), and the initial starting points of the four trajectories (black points, shown as small spheres) and the actual position (colored points, shown as small spheres).
With the internuclear distance parameter , since the Coulomb potential is spherically symmetrical, the oneelectron Schrödinger equation can be solved analytically in spherical polar coordinates, with equal to the distance between the nucleus and the electron, derivatives written and so on: . For simplicity, set the reduced mass and equal to 1 (atomic units). This leads to the timedependent wavefunction with the associated Laguerre polynomials and the spherical harmonics : , with the energy eigenvalue and . The principal quantum number determines the energy, is called the orbital angular momentum quantum number and is the magnetic quantum number. To get Bohm trajectories, the hydrogen atom has to be excited because the magnetic number must be , which is only fulfilled for states with . When , the electron is at rest; for a stationary state with , the electron orbits the axis along a circle of constant radius and with constant angular speed, depending on the sign and magnitude of [2]. For ( state), the energy equals . For , , , in Cartesian coordinates with , , and , the spatial wavefunction on each of the two hydrogen atoms forms a linear combination that leads to LCAOMOlike application to , which is not the standard LCAOMO method, with: . For this very special case, the wavefunction becomes: . For , the wavefunction becomes an exact solution of the Schrödinger equation. From the wavefunction for , the equation for the phase function follows: In Cartesian coordinates, the components of the velocity could be declared by the gradient of the total phase function from the total wave function in the eikonal form, which lead in this special case to a corresponding autonomous differential equation system: For the limiting case and for the asymptotic behavior , the components of the velocity become: , and . For more detailed information about the hydrogenlike atom and Bohm theory, see [1–3, 6, 7], and for a general introduction to Bohmian mechanics, see [2, 4, 5]. In the program, to make the results more accurate, increase PlotPoints, MaxRecursion, AccuracyGoal, PrecisionGoal and MaxSteps. [1] C. Dewdney and Z. Malik, "AngularMomentum Measurement and Nonlocality in Bohm’s Interpretation of Quantum Theory," Physical Review A, 48(5), 1993 pp. 3513–3524. doi:10.1103/PhysRevA.48.3513. [2] P. Holland, The Quantum Theory of Motion: An Account of the de Broglie–Bohm Causal Interpretation of Quantum Mechanics, Cambridge: Cambridge University Press, 1993. [3] C. Colijn and E. R. Vrscay, "SpinDependent Bohm Trajectories for Hydrogen Eigenstates," Physics Letters A, 300(4–5), 2002 pp. 334–340. doi:10.1016/S03759601(02)008241. [6] L. P. Yatsenko, V. I. Romanenko, B. W. Shore, T. Halfmann and K. Bergmann,"TwoPhoton Excitation of the Metastable 2 s State of Hydrogen Assisted by LaserInduced Chirped Stark Shifts and Continuum Structure," Physical Review A, 71(3), 2005 pp. 1–10. doi:10.1103/PhysRevA.71.033418.
