Relation Between the Wave Function and Probability Density

Quantum Mechanics A

Schrödinger Equation The most fundamental equation of quantum mechanics; given a Hamiltonian ${\mathcal {H}}$, it describes how a state $|\Psi \rangle$ evolves in time.

Physical Basis of Quantum Mechanics

Basic Concepts and Theory of Motion UV Catastrophe (Black-Body Radiation) Photoelectric Effect Stability of Matter Double Slit Experiment Stern-Gerlach Experiment The Principle of Complementarity The Correspondence Principle The Philosophy of Quantum Theory

Schrödinger Equation

Brief Derivation of Schrödinger Equation Relation Between the Wave Function and Probability Density Stationary States Heisenberg Uncertainty Principle Some Consequences of the Uncertainty Principle

Operators, Eigenfunctions, and Symmetry

Linear Vector Spaces and Operators Commutation Relations and Simultaneous Eigenvalues The Schrödinger Equation in Dirac Notation Transformations of Operators and Symmetry Time Evolution of Expectation Values and Ehrenfest's Theorem

Motion in One Dimension

One-Dimensional Bound States Oscillation Theorem The Dirac Delta Function Potential Scattering States, Transmission and Reflection Motion in a Periodic Potential Summary of One-Dimensional Systems

Discrete Eigenvalues and Bound States

Harmonic Oscillator Spectrum and Eigenstates Analytical Method for Solving the Simple Harmonic Oscillator Coherent States Charged Particles in an Electromagnetic Field WKB Approximation

Time Evolution and the Pictures of Quantum Mechanics

The Heisenberg Picture: Equations of Motion for Operators The Interaction Picture The Virial Theorem

Angular Momentum

Commutation Relations Angular Momentum as a Generator of Rotations in 3D Spherical Coordinates Eigenvalue Quantization Orbital Angular Momentum Eigenfunctions

Central Forces

General Formalism Free Particle in Spherical Coordinates Spherical Well Isotropic Harmonic Oscillator Hydrogen Atom WKB in Spherical Coordinates

The Path Integral Formulation of Quantum Mechanics

Feynman Path Integrals The Free-Particle Propagator Propagator for the Harmonic Oscillator

Continuous Eigenvalues and Collision Theory

Differential Cross Section and the Green's Function Formulation of Scattering Central Potential Scattering and Phase Shifts Coulomb Potential Scattering

Next, we wish to show that for any fixed time $t\!$, the probability to find a particle in space is equal to one.

The quantity $|\psi ({\textbf {r}},t)|^{2}$ can be interpreted as probability density. To show that this is true, two conditions must be met. First, the probability amplitude must be positive semi-definite (equal to or greater than zero). This condition is trivial because $|\psi ({\textbf {r}},t)|^{2}\!$ is always a positive function. Second, the probability amplitude must be conserved. This condition can be shown by proving that if the wavefunction is normalized at some time $t_{0}\!$ then it must be normalized for any time $t\!$:

$\int _{-\infty }^{\infty }d^{3}r|\psi ({\textbf {r}},t_{0})|^{2}=1\Rightarrow \int d^{3}r|\psi ({\textbf {r}},t)|^{2}=1\;\;\forall t$

The solution to the Schrödinger equation conserves probability, i.e. the probability to find the particle somewhere in the space does not change with time. To see that it does, consider

$i\hbar {\frac {\partial }{\partial t}}\psi ({\textbf {r}},t)=\left[-{\frac {\hbar ^{2}}{2m}}\nabla ^{2}+V({\textbf {r}})\right]\psi ({\textbf {r}},t)$

Now multiply both sides by the complex conjugate of $\psi ({\textbf {r}},t)\!$:

$i\hbar \psi ^{*}({\textbf {r}},t){\frac {\partial }{\partial t}}\psi ({\textbf {r}},t)=\psi ^{*}({\textbf {r}},t)\left[-{\frac {\hbar ^{2}}{2m}}\nabla ^{2}+V({\textbf {r}})\right]\psi ({\textbf {r}},t)$

Now, take the complex conjugate of this entire expression:

$-i\hbar \psi ({\textbf {r}},t){\frac {\partial }{\partial t}}\psi ^{*}({\textbf {r}},t)=\psi ({\textbf {r}},t)\left[-{\frac {\hbar ^{2}}{2m}}\nabla ^{2}+V({\textbf {r}})\right]\psi ^{*}({\textbf {r}},t)$

and taking the difference of the above equations, we finally find

${\frac {\partial }{\partial t}}\left(\psi ^{*}({\textbf {r}},t)\psi ({\textbf {r}},t)\right)+{\frac {\hbar }{2im}}\nabla \cdot \left[\psi ^{*}({\textbf {r}},t)\nabla \psi ({\textbf {r}},t)-(\nabla \psi ^{*}({\textbf {r}},t))\psi ({\textbf {r}},t)\right]=0$

Note that this is in the form of a continuity equation

${\frac {\partial }{\partial t}}\rho ({\textbf {r}},t)+\nabla \cdot {\textbf {j}}({\textbf {r}},t)=0$

where

$\rho ({\textbf {r}},t)=\psi ^{*}({\textbf {r}},t)\psi ({\textbf {r}},t)\!$

is the probability density, and

${\textbf {j}}({\textbf {r}},t)={\frac {\hbar }{2im}}\left[\psi ^{*}({\textbf {r}},t)\nabla \psi ({\textbf {r}},t)-(\nabla \psi ^{*}({\textbf {r}},t))\psi ({\textbf {r}},t)\right]$

is the probability current.

Once we know that the densities and currents constructed from the solution of the Schrödinger equation satisfy the continuity equation, it is easy to show that the probability is conserved. To see that note:

${\frac {\partial }{\partial t}}\int d^{3}r|\psi ({\textbf {r}},t)|^{2}=-\int d^{3}r(\nabla \cdot {\textbf {j}})=-\oint d{\textbf {A}}\cdot {\textbf {j}}=0$

where we used the divergence theorem which relates the volume integrals to surface integrals of a vector field. Since the wavefunction is assumed to vanish outside of the boundary, the current vanishes as well. So, this proved the probability of finding the particle in the whole space is independent of time.