If the particle has spin, it has a corresponding magnetic moment, so an extra term needs to be added incorporating the spin interaction with the electromagnetic field. In SI units: where S is the spin vector of the particle with corresponding spin magnetic moment μS and spin quantum numbers. In Gaussian units:
Connection with classical mechanics
The wave function can also be written in the complex exponential form: where R and S are real functions of r and t. Written this way, the probability density is and the probability current is: The exponentials and R∇R terms cancel: Finally, combining and cancelling the constants, and replacing R2 with ρ, If we take the familiar formula for the current: where v is the velocity of the particle, we can associate the velocity with ∇S/m, which is the same as equating ∇S with the classical momentum p = mv. This interpretation fits with Hamilton–Jacobi theory, in which in Cartesian coordinates is given by ∇S, where S is Hamilton's principal function.
The definition of probability current and Schrödinger's equation can be used to derive the continuity equation, which has exactly the same forms as those for hydrodynamics and electromagnetism: where the probability density is defined as If one were to integrate both sides of the continuity equation with respect to volume, so that then the divergence theorem implies the continuity equation is equivalent to the integral equation where the V is any volume and S is the boundary of V. This is the conservation law for probability in quantum mechanics. In particular, if Ψ is a wavefunction describing a single particle, the integral in the first term of the preceding equation, sans time derivative, is the probability of obtaining a value within V when the position of the particle is measured. The second term is then the rate at which probability is flowing out of the volumeV. Altogether the equation states that the time derivative of the probability of the particle being measured in V is equal to the rate at which probability flows into V.
Transmission and reflection through potentials
In regions where a step potential or potential barrier occurs, the probability current is related to the transmission and reflection coefficients, respectively T and R; they measure the extent the particles reflect from the potential barrier or are transmitted through it. Both satisfy: where T and R can be defined by: where jinc, jref and jtrans are the incident, reflected and transmitted probability currents respectively, and the vertical bars indicate the magnitudes of the current vectors. The relation between T and R can be obtained from probability conservation: In terms of a unit vector nnormal to the barrier, these are equivalently: where the absolute values are required to prevent T and R being negative.
Examples
Plane wave
For a plane wave propagating in space: the probability density is constant everywhere; but the probability current is nonzero – the square of the absolute amplitude of the wave times the particle's speed; illustrating that the particle may be in motion even if its spatial probability density has no explicit time dependence.
Particle in a box
For a particle in a box, in one spatial dimension and of length L, confined to the region; the energy eigenstates are and zero elsewhere. The associated probability currents are since
Discrete definition
For a particle in one dimension on, we have the Hamiltonian where is the discrete Laplacian, with being the right shift operator on. Then the probability current is defined as, with the velocity operator, equal to and is the position operator on. Since is usually a multiplication operator on, we get to safely write. As a result, we find: