Probability amplitude

For a probability amplitude ψ, the associated probability density function is

ψ*ψ

which is equal to |ψ|². This is sometimes called just probability density, and may be found used without normalisation (to have the total 1).

If |ψ|² has a finite integral over the whole of three-dimensional space, then it is possible to choose a normalising constant, c, so that by replacing ψ by cψ the integral becomes 1. Then the probability that a particle is within a particular region V is the integral over V of |ψ|².

The change over time of this probability (in our example, this corresponds to a description of how the particle moves) is expressed in terms of ψ itself, not just the probability function |ψ|². See Schrödinger equation.

In order to describe the change over time of the probability density it is acceptable to define the probability flux (also called probability current). The probability flux j is defined as:
::
and measured in units of (probability)/(area*time) = r^-2t^-1.

The probability flux satisfies a quantum continuity equation, i.e.:
::
where P(x,t) is the probability density and measured in units of (probability)/(volume) = r^-3.
This equation is the mathematical equivalent of probability conservation law.

It is easy to show that for a plain wave function,
:
the probability flux is given by
:

The bi-linear form of the axiom has interesting consequences as well.