3.10: Continuous Eigenvalues
- Page ID
- 146491
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\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)In the previous two sections, it was tacitly assumed that we were dealing with operators possessing discrete eigenvalues and square-integrable eigenstates. Unfortunately, some operators—most notably, \(x\) and \(p\)—possess eigenvalues that lie in a continuous range and non-square-integrable eigenstates (in fact, these two properties go hand in hand). Let us, therefore, investigate the eigenstates and eigenvalues of the displacement and momentum operators.
Let \(\psi_x(x,x')\) be the eigenstate of \(x\) corresponding to the eigenvalue \(x'\). It follows that
\[x\,\psi_x(x,x') = x'\,\psi_x(x,x') \nonumber \]
for all \(x\). Consider the Dirac delta-function \(\delta(x-x')\). We can write
\[x\,\delta(x-x') = x'\,\delta(x-x'), \nonumber \]
because \(\delta(x-x')\) is only non-zero infinitesimally close to \(x=x'\). Evidently, \(\psi_x(x,x')\) is proportional to \(\delta(x-x')\). Let us make the constant of proportionality unity, so that
\[\psi_x(x,x') = \delta(x-x'). \nonumber \]
It is easily demonstrated that
\[\int_{-\infty}^{\infty} \delta(x-x')\,\delta(x-x'')\,dx = \delta(x'-x''). \nonumber \]
Hence, \(\psi_x(x,x')\) satisfies the orthonormality condition
\[ \int_{-\infty}^\infty \psi_x^\ast(x,x')\,\psi_x(x,x'')\,dx = \delta(x'-x''). \label{e4.143} \]
This condition is analogous to the orthonormality condition \ref{e3.125} satisfied by square-integrable eigenstates. Now, by definition, \(\delta(x-x')\) satisfies
\[\int_{-\infty}^\infty f(x)\,\delta(x-x')\,dx = f(x'), \nonumber \]
where \(f(x)\) is a general function. We can thus write
\[ \psi(x) = \int_{-\infty}^\infty c(x')\,\psi_x(x,x')\,dx', \label{e4.144} \]
where \(c(x')=\psi(x')\), or
\[ c(x') = \int_{-\infty}^\infty \psi_x^\ast(x,x')\,\psi(x)\,dx. \label{e4.145} \]
In other words, we can expand a general wavefunction \(\psi(x)\) as a linear combination of the eigenstates, \(\psi_x(x,x')\), of the displacement operator. Equations \ref{e4.144} and \ref{e4.145} are analogous to Equations \ref{e3.123} and \ref{e3.126}, respectively, for square-integrable eigenstates. Finally, by analogy with the results in Section 1.9, the probability density of a measurement of \(x\) yielding the value \(x'\) is \(|c(x')|^2\), which is equivalent to the standard result \(|\psi(x')|^2\). Moreover, these probabilities are properly normalized provided \(\psi(x)\) is properly normalized [cf., Equation \ref{e3.127}]: that is,
\[\int_{-\infty}^\infty |c(x')|^2\,dx'= \int_{-\infty}^\infty |\psi(x')|^2\,dx' =1. \nonumber \]
Finally, if a measurement of \(x\) yields the value \(x'\) then the system is left in the corresponding displacement eigenstate, \(\psi_x(x,x')\), immediately after the measurement. That is, the wavefunction collapses to a “spike-function”, \(\delta(x-x')\), as discussed in Section [scoll].
Now, an eigenstate of the momentum operator \(p\equiv -{\rm i}\,\hbar\,\partial/\partial x\) corresponding to the eigenvalue \(p'\) satisfies
\[-{\rm i}\,\hbar\,\frac{\partial \psi_p(x,p')}{\partial x} = p'\,\psi_p(x,p'). \nonumber \]
It is evident that
\[ \psi_p(x,p') \propto \rm e^{+{\rm i}\,p'\,x/\hbar}. \label{e4.148} \]
We require \(\psi_p(x,p')\) to satisfy an analogous orthonormality condition to Equation \ref{e4.143}: that is,
\[\int_{-\infty}^\infty \psi_p^\ast(x,p')\,\psi_p(x,p'')\,dx = \delta(p'-p''). \nonumber \]
Thus, it follows from Equation \ref{e3.72} that the constant of proportionality in Equation \ref{e4.148} should be \((2\pi\,\hbar)^{-1/2}\): that is,
\[ \psi_p(x,p') =\frac{ \rm e^{+{\rm i}\,p'\,x/\hbar}}{(2\pi\,\hbar)^{1/2}}. \label{e4.148a} \]
Furthermore, according to Equations \ref{e3.64} and \ref{e3.65},
\[ \psi(x) = \int_{-\infty}^\infty c(p')\,\psi_p(x,p')\,dp', \label{e4.152} \]
where \(c(p') = \phi(p')\) [see Equation \ref{e3.65}], or
\[ c(p') = \int_{-\infty}^\infty \psi_p^\ast(x,p')\,\psi(x)\,dx. \label{e4.153} \]
In other words, we can expand a general wavefunction \(\psi(x)\) as a linear combination of the eigenstates, \(\psi_p(x,p')\), of the momentum operator. Equations \ref{e4.152} and \ref{e4.153} are again analogous to Equations \ref{e3.123} and \ref{e3.126}, respectively, for square-integrable eigenstates. Likewise, the probability density of a measurement of \(p\) yielding the result \(p'\) is \(|c(p')|^2\), which is equivalent to the standard result \(|\phi(p')|^2\). The probabilities are also properly normalized provided \(\psi(x)\) is properly normalized [cf., Equation \ref{e3.83}]: that is,
\[\int_{-\infty}^\infty |c(p')|^2\,dp'= \int_{-\infty}^{\infty} |\phi(p')|^2\,dp' = \int_{-\infty}^\infty |\psi(x')|^2\,dx' =1. \nonumber \]
Finally, if a mesurement of \(p\) yields the value \(p'\) then the system is left in the corresponding momentum eigenstate, \(\psi_p(x,p')\), immediately after the measurement.

