2.1: Representing states in the full Hilbert space
- Page ID
- 20878
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\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)Given a representation of the states that span the spin Hilbert space, we now need to consider the problem of representing the the states the span the full Hilbert space:

We will work with the following complete set of commuting observables (CSCO): \(\{X,Y,Z,S^2,S_z\}\), which means that the basis vectors which span the full Hilbert space must be simultaneous eigenvectors of these five operators. These will be represented as

that is, they will be a tensor product of the usual coordinate eigenvector and the simultaneous eigenvector of \(S^2\) and \(S_z\). Thus, they will satisfy the eigenvalue equations:
\(\displaystyle X\vert{\bf r}\;\;s\;m_s\rangle\) | \(\textstyle =\) | \(\displaystyle x \vert{\bf r}\;\;s\;m_s\rangle\) | |
\(\displaystyle Y\vert{\bf r}\;\;s\;m_s\rangle\) | \(\textstyle =\) | \(\displaystyle y \vert{\bf r}\;\;s\;m_s\rangle\) | |
\(\displaystyle Z\vert{\bf r}\;\;s\;m_s\rangle\) | \(\textstyle =\) | \(\displaystyle z \vert{\bf r}\;\;s\;m_s\rangle\) | |
\(\displaystyle S^2\vert{\bf r}\;\;s\;m_s\rangle\) | \(\textstyle =\) | \(\displaystyle s(s+1)\hbar^2 \vert{\bf r}\;\;s\;m_s\rangle\) | |
\(\displaystyle S_z\vert{\bf r}\;\;s\;m_s\rangle\) | \(\textstyle =\) | \(\displaystyle m_s\hbar \vert{\bf r}\;\;s\;m_s\rangle\) |
The basis vectors will also satisfy an orthogonality relation:

Any arbitrary vector \(\vert\phi\rangle\) in the Hilbert space can be expanded in terms of these basis vectors:

The expansion coefficients can, as usual, be designated as functions of \({\bf r}\):

For the case of spin-1/2, the expansion takes the form
\(\displaystyle \vert\phi\rangle\) | \(\textstyle =\) | ![]() | |
\(\textstyle =\) | ![]() |
The coefficients are designated by
![]() | |||
![]() |
Then, since the basis vectors are:
\(\displaystyle \left\vert{\bf r}\;\;{1 \over 2}\;{1 \over 2}\right>\) | \(\textstyle =\) | ![]() | |
\(\displaystyle \left\vert{\bf r}\;\;{1 \over 2}\;-{1 \over 2}\right>\) | \(\textstyle =\) | ![]() |
the expansion can be written as
\(\displaystyle \vert\phi\rangle\) | \(\textstyle =\) | ![]() | |
\(\textstyle =\) | ![]() | ||
\(\textstyle =\) | ![]() |
The vector

is called a two-component spinor. Note that
\(\displaystyle \langle \phi\vert\phi\rangle\) | \(\textstyle =\) | ![]() | |
\(\textstyle =\) | ![]() | ||
\(\textstyle =\) | ![]() |
Example: If we have a spin-independent Hamiltonian that is also spherically symmetric, then the quantum numbers that characterize the states will be \(n,l,m,s,m_s\). Thus, for the hydrogen atom,
![\begin{displaymath}
H = \left[-{\hbar^2 \over 2\mu}{1 \over r}{\partial^2 \over ...
...l r^2}r +
{l(l+1)\hbar^2 \over 2\mu r^2}-{e^2 \over r}\right]
\end{displaymath}](http://www.nyu.edu/classes/tuckerman/quant.mech/lectures/lecture_6/img40.png)
which is spin independent. The ground state will, therefore, be twofold degenerate with the two eigenfunctions being:
\(\displaystyle \psi_{100{1 \over 2}\;{1 \over 2}}(r,\theta,\varphi)\) | \(\textstyle =\) | \(\displaystyle \left({1 \over \pi a_0^3}\right)^{1/2}e^{-r/a_0}{\left(\matrix{1 \cr 0}\right)}\) | |
\(\displaystyle \psi_{100{1 \over 2}\;-{1 \over 2}}(r,\theta,\varphi)\) | \(\textstyle =\) | \(\displaystyle \left({1 \over \pi a_0^3}\right)^{1/2}e^{-r/a_0}{\left(\matrix{0 \cr 1}\right)}\) |