Moving electron - finding the wavefunction

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Homework Statement


On our modern physics class e did a problem:
Write down a wavefunction of an electron which is mooving from left to
right and has an energy ##100eV##.
At first i said: "Oh i know this!" and solved the case like this.

Homework Equations


Lorentz invariant: ##E=\sqrt{{E_0}^2 + p^2c^2}##
Schrödinger equation where ##V(x)=0##.

The Attempt at a Solution


The energy ##100eV## must be the kinetic energy of the electron. So i said ok this kinetic energy is very small compared to the rest energy and i can say that ##pc \ll E_0## which means i have a classical limit where:

\begin{align}
E=\sqrt{{E_0}^2 + p^2c^2}\\
E=\sqrt{{E_0}^2 + 0}\\
\boxed{E=E_0}
\end{align}

So now i can write the general wavefunction for a free right-mooving particle like this:

$$\psi=Ae^{iLx}\quad L=\sqrt{\tfrac{2mE}{\hbar^2}}$$

So if i want to get the speciffic solution i need to calculate the constant ##L## and then normalise the ##\psi##. Because ##E=E_0## i calculated the constant ##L## like this:

$$L=\sqrt{\frac{2mE_0}{\hbar^2}}$$

while my professor states that i should do it like this:

$$L=\sqrt{\frac{2mE_k}{\hbar^2}}$$

where ##E_k## is the kinetic energy of the electron. Who is wrong? I mean whaaaaat? The constant ##L## is afterall defined using the full energy and not kinetic energy...
 
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Thank you.

But can you explain to me why don't we generaly use the rest energy when dealing with a classical approximations. In books everyone explains the rest energy but what it really is? I mean i know how to calculate it and whatsoever but when does it appear and why do we have to take it into the calculation?

I am confused only because of that Lorentz invariance which says that if a particle is mooving slowly most of its energy is the rest energy. On the other hand we just neglect it like it isn't there... It seems to me like a contradiction...
 
It's just the way you're doing the classical approximation isn't correct. A plane wave is given by $$\psi = e^{i(kx-\omega t)}$$ where ##p= \hbar k## and ##E = \hbar \omega##. For the spatial dependence, you need to find the classical approximation for the momentum p:
\begin{align*}
pc &= \sqrt{E^2 - (mc^2)^2} \\
&= \sqrt{(mc^2+K)^2 - (mc^2)^2} \\
&= \sqrt{2mc^2 K + K^2} \\
&\cong \sqrt{2mc^2 K}
\end{align*} where K is the kinetic energy. The rest energy term cancels out.

The other way to look at it is that ##k = \sqrt{\frac{2mE}{\hbar^2}}## is equivalent to the relationship ##E = \frac{(\hbar k)^2}{2m} = \frac{p^2}{2m}##. This latter expression is clearly the classical quantity for the kinetic energy of a particle of mass m, not the total energy.
 
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