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The Anomalous Zeeman Effect

We compute the energy change due to a weak magnetic field using first order Perturbation Theory.


\begin{displaymath}\bgroup\color{black}\left<\psi_{n\ell jm_j}\left\vert{eB\over{2mc}}(L_z+2S_z)\right\vert\psi_{n\ell jm_j}\right>\egroup\end{displaymath}


\begin{displaymath}\bgroup\color{black}(L_z+2S_z)=J_z+S_z\egroup\end{displaymath}

The \bgroup\color{black}$J_z$\egroup part easy.

\begin{displaymath}\bgroup\color{black}\left<\psi_{n\ell jm_j}\left\vert{eB\over...
...\vert\psi_{n\ell jm_j}\right>
= {eB\over{2mc}}\hbar m_j\egroup\end{displaymath}

The \bgroup\color{black}$S_z$\egroup is harder. We need \bgroup\color{black}$\left<\psi_{n\ell jm_j}\left\vert{eB\over{2mc}}S_z\right\vert\psi_{n\ell jm_j}\right>$\egroup, but we don't know how \bgroup\color{black}$S_z$\egroup acts on these. So, we must write \bgroup\color{black}$\left\vert\psi_{njm_j\ell s}\right>$\egroup in terms of \bgroup\color{black}$\left\vert\psi_{n\ell m_\ell sm_s}\right>$\egroup.


\begin{displaymath}\bgroup\color{black} E^{(1)}_n = \left<\psi_{nj\ell m_j}\left...
...\over{2mc}}(J_z+S_z)\right\vert \psi_{nj\ell m_j}\right>\egroup\end{displaymath}


\begin{displaymath}\bgroup\color{black} = {eB\over{2mc}}\left( m_j \hbar+\left<\...
...eft\vert S_z \right\vert \psi_{nj\ell m_j}\right>\right)\egroup\end{displaymath}

from Ch.15


\begin{displaymath}\bgroup\color{black}\psi_{n(\ell+{1\over 2})\ell (m+{1\over 2...
... = \alpha Y_{\ell m}\chi_+ + \beta Y_{\ell (m+1)}\chi_- \egroup\end{displaymath}


\begin{displaymath}\bgroup\color{black}\psi_{n(\ell-{1\over 2})\ell (m+{1\over 2...
... = \beta Y_{\ell m}\chi_+ - \alpha Y_{\ell (m+1)}\chi_- \egroup\end{displaymath}


\begin{displaymath}\bgroup\color{black}\alpha=\sqrt{\ell +m+1\over {2\ell + 1}} \qquad
\beta=\sqrt{\ell -m\over {2\ell + 1}} \egroup\end{displaymath}

\bgroup\color{black}$j=\ell+{1\over 2}$\egroup:


\begin{displaymath}\bgroup\color{black}\left<\psi_{nj\ell m_j}\left\vert S_z\rig...
...chi_+
+ \beta Y_{\ell (m_j+{1\over 2})} \chi_- \right> \egroup\end{displaymath}


\begin{displaymath}\bgroup\color{black} = {1\over 2}\hbar\left(\alpha^2 -\beta^2\right)_{m=m_j -{1\over 2}}\egroup\end{displaymath}

and for \bgroup\color{black}$j=\ell-{1\over 2}$\egroup,

\begin{displaymath}\bgroup\color{black}\left<\psi_{nj\ell m_j}\left\vert S_z\rig...
...}\hbar\left(\beta^2 -\alpha^2\right)_{m=m_j -{1\over 2}}\egroup\end{displaymath}

We can combine the two formulas for \bgroup\color{black}$j=\ell\pm{1\over 2}$\egroup.

\begin{displaymath}\bgroup\color{black}\left<\psi_{nj\ell m_j}\left\vert S_z\rig...
...\pm {\hbar\over 2} {\ell + m+1-\ell + m\over{2\ell +1}} \egroup\end{displaymath}


\begin{displaymath}\bgroup\color{black} = \pm {\hbar\over 2} {2(m_j -{1\over 2})+1\over {2\ell + 1}}
= \pm {m_j \hbar\over{2\ell + 1}} \egroup\end{displaymath}

So adding this to the (easier) part above, we have

\begin{displaymath}\bgroup\color{black} E^{(1)}_n ={eB\over {2mc}}\left(m_j\hbar...
...r B\over {2mc}}m_j \left(1\pm {1\over{2\ell +1}}\right) \egroup\end{displaymath}

for \bgroup\color{black}$j=\ell\pm{1\over 2}$\egroup.

In summary then, we rewrite the fine structure shift.

\begin{displaymath}\bgroup\color{black}\Delta E = -{1\over 2}mc^2\left(Z\alpha\r...
...n^3}}\left[ {1\over{j+{1\over 2}}} -{3\over{4n}}\right].\egroup\end{displaymath}

To this we add the anomalous Zeeman effect

\begin{displaymath}\bgroup\color{black}\Delta E = {e\hbar B\over {2mc}}m_j \left(1\pm {1\over{2\ell +1}}\right).\egroup\end{displaymath}


next up previous
Next: Homework Problems Up: Derivations and Computations Previous: The Darwin Term
James Branson
2001-09-17