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  If ψ<sup>2</sup> Has A Finite "http://wwwinformationdelightinfo/encyclopedia/entry/integral" class="copylinks">Integral over the whole of three-dimensional space, then it is possible to choose a ''normalising constant'', ''c'', so that by replacing ψ by ''c''ψ the integral becomes 1 Then the probability that a particle is within a particular region ''V'' is the integral over ''V'' of ψ<sup>2</sup> Which means, according to the Copenhagen Interpretation of Quantum Mechanics , that, if some observator tries to measure the quantity associated to this probability amplitude, the result of the measurement will lie within Σ with a probability P(Σ) given by
  ::<math> P(\Sigma) \int_\Sigma^{} \psi(x)^2 dx / \int_\Sigma^{} dx </math>
  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<sup>2</sup> See "http://wwwinformationdelightinfo/encyclopedia/entry/Schrödinger_equation" class="copylinks">Schrödinger Equation


abla \psi - \psi


The probability flux satisfies a quantum Continuity Equation , i.e.:
::
abla \cdot \mathbf{j} + { \partial \over \partial t} P(x,t) = 0
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 plane Wave Function ,
  :<math> J(x,t) A^2 {k \hbar \over m} </math>