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Next: Spin greater than one-half Up: Angular momentum Previous: Spin precession

Pauli two-component formalism

We have seen, in Sect. 5.4, that the eigenstates of orbital angular momentum can be conveniently represented as spherical harmonics. In this representation, the orbital angular momentum operators take the form of differential operators involving only angular coordinates. It is conventional to represent the eigenstates of spin angular momentum as column (or row) matrices. In this representation, the spin angular momentum operators take the form of matrices.

The matrix representation of a spin one-half system was introduced by Pauli in 1926. Recall, from Sect. 5.9, that a general spin ket can be expressed as a linear combination of the two eigenkets of $S_z$ belonging to the eigenvalues $\pm \hbar/2$. These are denoted $\vert\pm \rangle$. Let us represent these basis eigenkets as column matrices:

$\displaystyle \vert+\rangle$ $\textstyle \rightarrow$ $\displaystyle \left(\!\begin{array}{c}1\  0\end{array}\!\right) \equiv \chi_+,$ (476)
$\displaystyle [0.5ex]
\vert-\rangle$ $\textstyle \rightarrow$ $\displaystyle \left(\!\begin{array}{c}0\  1\end{array}\!\right) \equiv \chi_-.$ (477)

The corresponding eigenbras are represented as row matrices:
$\displaystyle \langle +\vert$ $\textstyle \rightarrow$ $\displaystyle (1, 0) \equiv \chi_+^{\dag },$ (478)
$\displaystyle \langle - \vert$ $\textstyle \rightarrow$ $\displaystyle (0, 1) \equiv \chi_-^{\dag }.$ (479)

In this scheme, a general bra takes the form
\begin{displaymath}
\vert A\rangle = \langle +\vert A\rangle \vert+\rangle + \la...
...\vert A\rangle\\
\langle -\vert A\rangle\end{array}\!\right),
\end{displaymath} (480)

and a general ket becomes
\begin{displaymath}
\langle A\vert =\langle A\vert+\rangle \langle +\vert + \lan...
...
\rightarrow (\langle A\vert+\rangle, \langle A\vert-\rangle).
\end{displaymath} (481)

The column matrix (480) is called a two-component spinor, and can be written
\begin{displaymath}
\chi \equiv \left(\!\begin{array}{c}\langle +\vert A\rangle\...
...
c_+\ c_- \end{array}\!\right) = c_+  \chi_+ + c_-  \chi_-,
\end{displaymath} (482)

where the $c_\pm$ are complex numbers. The row matrix (481) becomes
\begin{displaymath}
\chi^{\dag } \equiv (\langle A\vert+\rangle, \langle A\vert-...
...) =c_+^{ \ast}  \chi_+^{\dag } + c_-^{ \ast} \chi_-^{\dag }.
\end{displaymath} (483)

Consider the ket obtained by the action of a spin operator on ket $A$:

\begin{displaymath}
\vert A'\rangle = S_k \vert A\rangle.
\end{displaymath} (484)

This ket is represented as
\begin{displaymath}
\vert A'\rangle
\rightarrow
\left(\!\begin{array}{c}\langle...
...e\\
\langle -\vert A'\rangle\end{array}\!\right)\equiv \chi'.
\end{displaymath} (485)

However,
$\displaystyle \langle + \vert A'\rangle$ $\textstyle =$ $\displaystyle \langle + \vert S_k\vert +\rangle \langle +\vert A\rangle
+ \langle +\vert S_k \vert-\rangle \langle -\vert A\rangle,$ (486)
$\displaystyle \langle - \vert A'\rangle$ $\textstyle =$ $\displaystyle \langle - \vert S_k\vert +\rangle \langle +\vert A\rangle
+ \langle -\vert S_k \vert-\rangle \langle -\vert A\rangle,$ (487)

or
\begin{displaymath}
\left(\!\begin{array}{c}\langle +\vert A'\rangle\ [0.5ex]
\...
...\rangle\ [0.5ex]
\langle -\vert A\rangle\end{array}\!\right).
\end{displaymath} (488)

It follows that we can represent the operator/ket relation (484) as the matrix relation
\begin{displaymath}
\chi' =\left( \frac{\hbar}{2}\right)\sigma_k  \chi,
\end{displaymath} (489)

where the $\sigma_k$ are the matrices of the $\langle \pm \vert S_k\vert\pm \rangle$ values divided by $\hbar/2$. These matrices, which are called the Pauli matrices, can easily be evaluated using the explicit forms for the spin operators given in Eqs. (431)-(433). We find that
$\displaystyle \sigma_1$ $\textstyle =$ $\displaystyle \left(\!\begin{array}{cc} 0 &1\  1&0\end{array}\!\right),$ (490)
$\displaystyle \sigma_2$ $\textstyle =$ $\displaystyle \left(\!\begin{array}{cc} 0 &-{\rm i}\  {\rm i}&0\end{array}\!\right),$ (491)
$\displaystyle \sigma_3$ $\textstyle =$ $\displaystyle \left(\!\begin{array}{cc} 1 &0\  0&-1\end{array}\!\right).$ (492)

Here, 1, 2, and 3 refer to $x$, $y$, and $z$, respectively. Note that, in this scheme, we are effectively representing the spin operators in terms of the Pauli matrices:
\begin{displaymath}
S_k \rightarrow \left(\frac{\hbar}{2} \right)\sigma_k.
\end{displaymath} (493)

The expectation value of $S_k$ can be written in terms of spinors and the Pauli matrices:
\begin{displaymath}
\langle S_k \rangle = \langle A\vert S_k \vert A\rangle = \s...
...= \left(\frac{\hbar}{2}\right) \chi^{\dag }  \sigma_k  \chi.
\end{displaymath} (494)

The fundamental commutation relation for angular momentum, Eq. (421), can be combined with (493) to give the following commutation relation for the Pauli matrices:

\begin{displaymath}
\mbox{\boldmath$\sigma$}\times \mbox{\boldmath$\sigma$}= 2 {\rm i} \mbox{\boldmath$\sigma$}.
\end{displaymath} (495)

It is easily seen that the matrices (490)-(492) actually satisfy these relations (i.e., $\sigma_1  \sigma_2 - \sigma_2 \sigma_1 = 2 {\rm i}  \sigma_3$, plus all cyclic permutations). It is also easily seen that the Pauli matrices satisfy the anti-commutation relations
\begin{displaymath}
\{ \sigma_i, \sigma_j \} = 2  \delta_{ij}.
\end{displaymath} (496)

Let us examine how the Pauli scheme can be extended to take into account the position of a spin one-half particle. Recall, from Sect. 5.8, that we can represent a general basis ket as the product of basis kets in position space and spin space:

\begin{displaymath}
\vert x', y', z', \pm\rangle = \vert x', y', z'\rangle\vert \pm\rangle = \vert \pm\rangle
\vert x', y', z'\rangle.
\end{displaymath} (497)

The ket corresponding to state $A$ is denoted $\vert\vert A\rangle\rangle$, and resides in the product space of the position and spin ket spaces. State $A$ is completely specified by the two wave-functions
$\displaystyle \psi_+(x', y', z')$ $\textstyle =$ $\displaystyle \langle x', y', z' \vert\langle +\vert\vert A\rangle\rangle,$ (498)
$\displaystyle \psi_-(x', y', z')$ $\textstyle =$ $\displaystyle \langle x', y', z' \vert\langle -\vert\vert A\rangle\rangle.$ (499)

Consider the operator relation
\begin{displaymath}
\vert\vert A'\rangle\rangle = S_k \vert\vert A\rangle\rangle.
\end{displaymath} (500)

It is easily seen that
$\displaystyle \langle x', y', z'\vert \langle +\vert A'\rangle\rangle$ $\textstyle =$ $\displaystyle \langle + \vert S_k \vert+\rangle \langle x',y',z'\vert\langle +\vert\vert A\rangle\rangle$  
    $\displaystyle +\langle + \vert S_k \vert-\rangle \langle x',y',z'\vert\langle -\vert\vert A\rangle\rangle,$ (501)
$\displaystyle \langle x', y', z'\vert \langle -\vert A'\rangle\rangle$ $\textstyle =$ $\displaystyle \langle - \vert S_k \vert+\rangle \langle x',y',z'\vert\langle +\vert\vert A\rangle\rangle$  
    $\displaystyle +\langle -
\vert S_k \vert-\rangle \langle x',y',z'\vert\langle -\vert\vert A\rangle\rangle,$ (502)

where use has been made of the fact that the spin operator $S_k$ commutes with the eigenbras $\langle x', y', z'\vert$. It is fairly obvious that we can represent the operator relation (500) as a matrix relation if we generalize our definition of a spinor by writing
\begin{displaymath}
\vert\vert A\rangle\rangle \rightarrow \left(\! \begin{array...
...{\bf r}') \\
\psi_-({\bf r}')\end{array}\!\right)\equiv \chi,
\end{displaymath} (503)

and so on. The components of a spinor are now wave-functions, instead of complex numbers. In this scheme, the operator equation (500) becomes simply
\begin{displaymath}
\chi' = \left(\frac{\hbar}{2}\right) \sigma_k  \chi.
\end{displaymath} (504)

Consider the operator relation

\begin{displaymath}
\vert\vert A'\rangle\rangle = p_k \vert\vert A\rangle\rangle.
\end{displaymath} (505)

In the Schrödinger representation, we have
$\displaystyle \langle x', y', z'\vert \langle +\vert A'\rangle\rangle$ $\textstyle =$ $\displaystyle \langle x', y', z'\vert p_k \langle +\vert\vert A\rangle\rangle$  
  $\textstyle =$ $\displaystyle -{\rm i} \hbar\frac{\partial}
{\partial x_k'} \langle x', y', z'\vert \langle +\vert\vert A\rangle\rangle,$ (506)
$\displaystyle \langle x', y', z'\vert \langle -\vert A'\rangle\rangle$ $\textstyle =$ $\displaystyle \langle x', y', z'\vert p_k \langle -\vert\vert A\rangle\rangle$  
  $\textstyle =$ $\displaystyle -{\rm i} \hbar\frac{\partial}
{\partial x_k'} \langle x', y', z'\vert \langle -\vert\vert A\rangle\rangle,$ (507)

where use has been made of Eq. (168). The above equation reduces to
\begin{displaymath}
\left(\! \begin{array}{c} \psi_+'({\bf r}')\\
\psi_-' ({\bf...
... \partial \psi_-({\bf r}')/\partial x_k'\end{array}\!\right).
\end{displaymath} (508)

Thus, the operator equation (505) can be written
\begin{displaymath}
\chi' = p_k  \chi,
\end{displaymath} (509)

where
\begin{displaymath}
p_k \rightarrow -{\rm i} \hbar\frac{\partial}{\partial x_k'}  {\bf I}.
\end{displaymath} (510)

Here, ${\bf I}$ is the $2\times 2$ unit matrix. In fact, any position operator (e.g., $p_k$ or $L_k$) is represented in the Pauli scheme as some differential operator of the position eigenvalues multiplied by the $2\times 2$ unit matrix.

What about combinations of position and spin operators? The most commonly occurring combination is a dot product: e.g., ${\bf S}\!\cdot\! {\bf L} = (\hbar/2) \mbox{\boldmath$\sigma$}\! \cdot\! {\bf L}$. Consider the hybrid operator $\mbox{\boldmath$\sigma$}\!\cdot \!{\bf a}$, where ${\bf a} \equiv (a_x, a_y, a_z)$ is some vector position operator. This quantity is represented as a $2\times 2$ matrix:

\begin{displaymath}
\mbox{\boldmath$\sigma$}\! \cdot\! {\bf a} \equiv \sum_k a_k...
...,a_2\ [0.5ex]
a_1 + {\rm i} a_2 & -a_3 \end{array}\!\right).
\end{displaymath} (511)

Since, in the Schrödinger representation, a general position operator takes the form of a differential operator in $x'$, $y'$, or $z'$, it is clear that the above quantity must be regarded as a matrix differential operator which acts on spinors of the general form (503). The important identity
\begin{displaymath}
(\mbox{\boldmath$\sigma$}\!\cdot \!{\bf a} )  (\mbox{\boldm...
...} \mbox{\boldmath$\sigma$}\!\cdot \!({\bf a} \times {\bf b} )
\end{displaymath} (512)

follows from the commutation and anti-commutation relations (495) and (496). Thus,
$\displaystyle \sum_j \sigma_j  a_j \sum_k \sigma_k  b_k$ $\textstyle =$ $\displaystyle \sum_j \sum_k \left(\frac{1}{2} 
\{\sigma_j, \sigma_k\} + \frac{1}{2} [\sigma_j, \sigma_k]\right) a_j  b_k$  
  $\textstyle =$ $\displaystyle \sum_j \sum_k (\sigma_{jk} + {\rm i} \epsilon_{jkl}  \sigma_l) a_j  b_k$  
  $\textstyle =$ $\displaystyle {\bf a} \!\cdot\! {\bf b}
+{\rm i} \mbox{\boldmath$\sigma$}\!\cdot\! ({\bf a} \times {\bf b} ).$ (513)

A general rotation operator in spin space is written

\begin{displaymath}
T (\Delta\phi) = \exp\left(-{\rm i}  {\bf S}\!\cdot\!{\bf n} \Delta\varphi/\hbar\right),
\end{displaymath} (514)

by analogy with Eq. (444), where ${\bf n}$ is a unit vector pointing along the axis of rotation, and $\Delta\varphi$ is the angle of rotation. Here, ${\bf n}$ can be regarded as a trivial position operator. The rotation operator is represented
\begin{displaymath}
\exp\left(-{\rm i}  {\bf S}\!\cdot\!{\bf n} \Delta\varphi/...
...box{\boldmath$\sigma$}\!\cdot\!{\bf n} \Delta\varphi/2\right)
\end{displaymath} (515)

in the Pauli scheme. The term on the right-hand side of the above expression is the exponential of a matrix. This can easily be evaluated using the Taylor series for an exponential, plus the rules
$\displaystyle (\mbox{\boldmath$\sigma$}\!\cdot \!{\bf n})^n$ $\textstyle =$ $\displaystyle 1 \mbox{\hspace{1.79cm}for $n$ even},$ (516)
$\displaystyle (\mbox{\boldmath$\sigma$}\!\cdot \!{\bf n})^n$ $\textstyle =$ $\displaystyle (\mbox{\boldmath$\sigma$}\!\cdot \!{\bf n})
\mbox{\hspace{1cm}for $n$ odd}.$ (517)

These rules follow trivially from the identity (512). Thus, we can write
$\displaystyle \exp\left(-{\rm i}  \mbox{\boldmath$\sigma$}\!\cdot\!{\bf n} \Delta\varphi/2\right)$ $\textstyle =$ $\displaystyle \left[ 1 - \frac{(\mbox{\boldmath$\sigma$}\! \cdot \! {\bf n})^2}...
...cdot \! {\bf n})^4}{4!} \left(\frac{\Delta\varphi}{2}
\right)^4 + \cdots\right]$  
    $\displaystyle - {\rm i} \left[ (\mbox{\boldmath$\sigma$}\! \cdot {\bf n} )\left...
...\cdot \! {\bf n})^3}{3!} \left(\frac{\Delta\varphi}{2}\right)^3
+ \cdots\right]$  
  $\textstyle =$ $\displaystyle \cos(\Delta\varphi/2) {\bf I}- {\rm i} \sin (\Delta\varphi/2) \mbox{\boldmath$\sigma$}\!\cdot\! {\bf n}.$ (518)

The explicit $2\times 2$ form of this matrix is
\begin{displaymath}
\left(\begin{array}{cc}
\cos(\Delta\varphi/2) - {\rm i} n_...
.../2) + {\rm i}  n_z \sin(\Delta\varphi/2)
\end{array} \right).
\end{displaymath} (519)

Rotation matrices act on spinors in much the same manner as the corresponding rotation operators act on state kets. Thus,
\begin{displaymath}
\chi' = \exp\left(-{\rm i}  \mbox{\boldmath$\sigma$}\!\cdot\!{\bf n} \Delta\varphi/2\right) \chi,
\end{displaymath} (520)

where $\chi'$ denotes the spinor obtained after rotating the spinor $\chi$ an angle $\Delta\varphi$ about the ${\bf n}$-axis. The Pauli matrices remain unchanged under rotations. However, the quantity $\chi^\dagger  \sigma_k  \chi$ is proportional to the expectation value of $S_k$ [see Eq. (494)], so we would expect it to transform like a vector under rotation (see Sect. 5.9). In fact, we require
\begin{displaymath}
(\chi^\dagger  \sigma_k  \chi)' \equiv (\chi^\dagger)' \sigma_k  \chi' = \sum_l R_{kl} 
(\chi^\dagger \sigma_l  \chi),
\end{displaymath} (521)

where the $R_{kl}$ are the elements of a conventional rotation matrix. This is easily demonstrated, since
\begin{displaymath}
\exp\left(\frac{ {\rm i} \sigma_3  \Delta\varphi}{2}\righ...
...ight) = \sigma_1 \cos\Delta\varphi
-\sigma_2 \sin\Delta\varphi
\end{displaymath} (522)

plus all cyclic permutations. The above expression is the $2\times 2$ matrix analogue of (see Sect. 5.9)
\begin{displaymath}
\exp\left(\frac{ {\rm i} S_z  \Delta\varphi}{\hbar}\right...
...ar}\right) = S_x  \cos\Delta\varphi
-S_y  \sin\Delta\varphi.
\end{displaymath} (523)

The previous two formulae can both be validated using the Baker-Hausdorff lemma, (452), which holds for Hermitian matrices, in addition to Hermitian operators.


next up previous
Next: Spin greater than one-half Up: Angular momentum Previous: Spin precession
Richard Fitzpatrick 2006-02-16