1.9: Linear Combinations of Waves
- Page ID
- 49372
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\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)Next, we consider the combinations of different complex exponential functions. For example, in Figure 1.9.1 we plot a wavefunction that could describe an electron that equiprobable at position \(x_{1}\) and position \(x_{2}\). The k-space representation is simply the superposition of two complex exponential functions corresponding to \(x_{1}\) and \(x_{2}\).\(^{†}\)
\[ \psi(x)=c_{1}\delta(x-x_{1})+c_{2}(x-x_{2}) \Leftrightarrow A(\omega) = c_{1}e^{-ikx_{1}}+c_{2}e^{-ikx_{2}} \nonumber \]

We can also generalize to an arbitrary distribution of positions, \(\psi(x)\). If \(\psi(x)\) describes an electron, for example, the probability that the electron is located at position x is \(|\psi(x)|^{2}\). Thus, in k-space the electron is described by the sum of complex exponentials \(e^{-ikx}\) each oscillating in k-space and weighted by amplitude \(\psi(x)\).
\[ A(k)=\int^{+\infty}_{-\infty}\psi(x)e^{-ikx}dx \nonumber \]
You may recognize this from 6.003 as a Fourier transform. Similarly, the inverse transform is
\[ \psi(x)=\frac{1}{2\pi}\int^{+\infty}_{-\infty}A(k)e^{ikx}dk \nonumber \]
To convert between time and angular frequency, use
\[ A(\omega) =\int^{+\infty}_{-\infty} \psi(t)e^{i\omega t}dt \nonumber \]
and
\[ \psi(t)=\frac{1}{2\pi}\int^{+\infty}_{-\infty} A(\omega)e^{-i\omega t}d\omega \nonumber \]
Note that the factors of \(\frac{1}{2\pi}\) are present each time you integrate with respect to k or \(\omega\). Note also that when converting between complex exponentials and delta functions, the following identity is useful:
\[ 2\pi\delta(u)=\int^{+\infty}_{-\infty} \text{exp}[iux]dx \nonumber \]
\(^{†}\)Note that this wave function is not actually normalizable.