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Energy States of Electrons in a Plasma II

If \bgroup\color{black}$\vec{A}=\left(0,Bx,0\right)$\egroup, then

\begin{displaymath}\bgroup\color{black}\vec{B}=\vec\nabla\times\vec{A}={\partial A_y\over{\partial x}}\hat{z}=B\hat{z}.\egroup\end{displaymath}

This \bgroup\color{black}$A$\egroup gives us the same B field. We can then compute H for a constant B field in the z direction.

\begin{displaymath}\bgroup\color{black}H={1\over {2 m_e}}\left(\vec{p}+{e\over c...
...^2_x+\left(p_y
+ {eB\over c} x\right)^2 + p^2_z\right) \egroup\end{displaymath}


\begin{displaymath}\bgroup\color{black} = {1\over {2 m_e}}\left(p^2_x+p^2_y + {2...
... c}x p_y
+ \left(eB\over c\right)^2 x^2 + p^2_z\right) \egroup\end{displaymath}

With this version of the same problem, we have the

\begin{displaymath}\bgroup\color{black}\left[H,p_y\right]=\left[H,p_z\right]=0.\egroup\end{displaymath}

We can treat \bgroup\color{black}$p_z$\egroup and \bgroup\color{black}$p_y$\egroup as constants of the motion and solve the problem in Cartesian coordinates.

\begin{displaymath}\bgroup\color{black}\psi=v(x)e^{ik_yy}e^{ik_zz}\egroup\end{displaymath}


\begin{displaymath}\bgroup\color{black}{1\over {2 m_e}}\left(-\hbar^2{d^2\over{d...
...ght)v(x)
=\left(E-{\hbar^2k_z^2\over 2 m_e}\right)v(x) \egroup\end{displaymath}

This is the same as the 1D harmonic oscillator equation with \bgroup\color{black}$\omega={eB\over{ m_e c}}$\egroup and \bgroup\color{black}$x_0={\hbar c k\over{eB}}$\egroup.


\begin{displaymath}\bgroup\color{black}E=\left(n+{1\over 2}\right)\hbar\omega={\...
...c}}\left(n+{1\over 2}\right)
+{\hbar^2k_z^2\over 2 m_e}\egroup\end{displaymath}

So we get the same energies with a much simpler calculation. The resulting states are somewhat strange and are not analogous to the classical solutions.


next up previous
Next: A Hamiltonian Invariant Under Up: Derivations and Computations Previous: Energy States of Electrons
James Branson
2001-09-17