(From my book http://physics-quest.org/Book_Chapter_Klein_Gordon.pdf)
Spreading of the free field wave packet
The speed of the wave packet is given by the derivative of the Hamiltonian against the momentum.
\begin{equation}
v ~~=~~ \frac{\partial H}{\partial p} ~~=~~ \frac{\partial E}{\partial p} ~~=~~ \frac{p c^2}{\sqrt{(pc)^2+(mc^2)^2}} ~~=~~ \frac{p c^2}{E~}
\end{equation}
The wave-packet would not spread in the case of a single $v$ such as in the case of a massless particle which is represented by a wave-function which moves unchanged at the speed of light.
However, a localized field with a Gaussian shape has (via the Fourier transform) a Gaussian distribution of $p$ in momentum space. The relation
\begin{equation}E = \sqrt{(pc)^2+(mc^2)^2}\end{equation}
means that there will be a range of speeds instead of a single one and so, in general, the wave-packet will spread.
figure 1.
The variation is approximately given by.
\begin{equation}
\frac{\Delta v}{\Delta p}~\approx~\frac{\partial v}{\partial p} ~~\longrightarrow~\Delta v ~\approx~ \frac{\partial^2 E}{\partial\,p^2}~\Delta p
\end{equation}
Given that Heisenberg's uncertainty relation $\Delta x \Delta p \geq \hbar/2$ can be derived by Fourier analysis, which in the case of a Gaussian shaped wave-function becomes $\Delta x \Delta p = \hbar/2$, the minimum value, we can write.
\begin{equation}
\Delta v ~\approx~ \frac{\partial^2 E}{\partial\,p^2}~\frac{\hbar}{2\Delta x}
\end{equation}
Where $\Delta x$ is the width. One can reason that the overall shape of a wave-function changes faster if $\Delta x$ is smaller for a given speed-variation $\Delta v$. We can define a dimension-less quantity shape, which has derivative in time which gives us an approximation of the relative spreading of the wave-function in time.
\begin{equation}
\frac{\partial}{\partial t}\Big\{ \mbox{shape} \Big\} ~~ \approx ~~ \frac{\Delta v}{\Delta x} ~~ \approx ~~ \frac{\partial^2 E}{\partial\, p^2}~\frac{\hbar}{2(\Delta x)^2}
\end{equation}
Working out the second order derivative gives us.
\begin{equation}
\frac{\partial^2 E}{\partial\, p^2} ~=~ \frac{(mc^2)^2~c^2}{~\big(~(pc)^2+(mc^2)^2~\big)^{3/2}~} ~=~ \frac{E_o^2\,c^2}{E^3} ~=~\frac{c^2}{E\gamma^2}
\end{equation}
Which leads us to our final expression here.
\begin{equation}
\frac{\partial}{\partial t}\Big\{ \mbox{shape} \Big\} ~~ \approx ~~ \frac{\hbar\,c^2}{2E(\gamma\Delta x)^2}
\end{equation}
If we remove the gamma's then we get the expression for the rest frame.
\begin{equation}
\frac{\partial}{\partial t}\Big\{ \mbox{shape} \Big\} ~~ \approx ~~ \frac{\hbar\,c^2}{2mc^2(\Delta x)^2}
\end{equation}
We can summarize the results as:
- The spreading of the wave-function is inversely proportional to the frequency (the phase change rate in time) of the particle, Higher mass particles spread slower.
- The spreading of the wave-function is proportional to the square of the momentum spread. The smaller the initial volume in which the initial wave-function was contained the faster it spreads and keeps spreading.
figure 2
From figure. 2 we can read the mathematical mechanism which leads to spreading. The variation $\Delta p$ of the momentum stays the same over time. It is the frequency dependency on the momentum
$E=\sqrt{(pc)^2+(mc^2)^2}$
which leads to a phase change over $p$.
The phase change is opposite at both sides of the center-momentum. These phase-changes lead to (opposite) translations of the wave-function in position space, this is the spreading. The value $\Delta x$ in our expression stays constant because $\Delta p$ stays constant, it is the initial $\Delta x$ corresponding to the pure Gaussian at $t$=$0$.
Some actual spreading rate numbers
We can work out a few numerical example to get an idea of the spreading rates. From the wide range of wavelength sizes, we can classify the Compton radius as the small size limit, although there is in principle no real barrier to go to even smaller sized wave-packets.
If we replace $\Delta x$ with twice the Compton radius $r_c=\hbar/mc$ then, assuming that our approximation is still reasonably valid in this range.
\begin{equation}
\frac{\partial}{\partial t}\Big\{ \mbox{shape} \Big\} ~~ \approx ~~ \frac{c}{8\,r_c}
\end{equation}
If we recall the rest-frequency of the particle: $f_o=c/(2\pi\,r_c)$ (in case of the electron $f_o=1.2355899729\,10^{20}$ Hz ), then we see that spreading speed approaches the speed of light in this range. The spread in momentum is so large that it includes velocities from close to $-c$ up to $+c$.
To confine an electron-field to a Compton radius-like volume one needs a positive charge of $~$137e, The inner-most electrons of heavy elements come close to being confined into such a small area. The Compton radius for electrons is $3.861592696\,10^{-13}$ meter.
More commonly, electrons freed from a bound state, take off with a much larger radius, comparable to the Bohr radius. ($5.291772131\,10^{-11}$ meter) This means that the spreading speed is much lower, $ v < 0.01c$, but still quite high.
The size of the wave-packet will grow fast. For instance, the famous single electron interference experiment of Akira Tomomura (see figure 3), which demonstrated the single-electron build-up of an interference pattern, shows that the electron fields in the experiment must at least be several micrometers wide. This is a factor 100,000 wider as in the confinement of the Bohr radius.
figure 3
Hans