% !TeX root = ../../script.tex \documentclass[../../script.tex]{subfiles} \begin{document} \section[Examples of the Stationary Schrödinger Equation]{Examples of the Stationary Schrödinger Equation} We now want to solve the Schrödinger equation \[ \frac{-\hbar^2}{2m} \dv[2]{\psi}{x} + \epot\psi = E\psi \] for a few simple, one-dimensional problems. These examples will illustrate the description of classical particles as waves and the following physical consequences. \subsection{The Free Particle} A particle is said to be free, if it is moving in a constant potention $\phi_0$, because then $\vec{F} = -\grad{\epot}$ means that no forces are acting on the particle. Through a suitable choice of the zero point energy we can set $\phi_0 = 0$, i.e. $\epot = 0$, and thus get the Schrödinger equation for a free particle \begin{equation}\label{eq:onedschroedinger} \frac{-\hbar^2}{2m} \dv[2]{\psi}{x} = E\psi \end{equation} The total energy $E = \ekin + \epot$ is because of $\epot$ now \[ E = \frac{p^2}{2m} = \frac{\hbar^2 k^2}{2m} \] Thus~\eqref{eq:onedschroedinger} gets reduced to \[ \dv[2]{\psi}{x} = -k^2 \psi \] which has the general solution \begin{equation}\label{eq:onedsolution} \psi(x) = Ae^{ikx} + Be^{-ikx} \end{equation} The time-dependent wave function \begin{equation} \psi(x, t) = \psi(x) \cdot e^{-i\omega t} = Ae^{i(kx - \omega t)} + Be^{-i(kx + \omega t)} \end{equation} represents the superposition of a planar wave travelling in the $+x$ and $-x$ direction. The coefficients $A$ and $B$ are the amplitudes of those waves, which are determined by the boundary conditions. For example, the wave function of electrons which are emitted from a cathode in $+x$ direction towards a detector, will have $B = 0$, since there are no particles moving in $-x$. From this experimental setup we know that the electrons are found along the length $L$ of the path between cathode and detector. This means their wave function can only be different from zero in this region of space. Using the normalization condition we get \begin{align*} &\int_0^L \abs{\psi(x)}^2 \dd{x} = 1 \\ &\implies A^2 \cdot L = 1 \implies A = \frac{1}{\sqrt{L}} \end{align*} To determine the location of a particle at time $t$ more accurately, we will have to construct \textit{wave packets} in place of planar waves~\eqref{eq:onedsolution} \begin{equation} \psi(x, t) = \int_{k_0 - \Delta k / 2}^{k_0 + \Delta k / 2} A(k) e^{i(kx - \omega t)} \dd{k} \end{equation} The location uncertainty of this packet at $t = 0$ is \[ \Delta x \ge \frac{\hbar}{2 \Delta p_x} = \frac{1}{2\Delta k} \] and depends on the pulse width $\Delta p_x = \hbar \Delta k$. The larger $k$ is, the more certainly $\Delta x(t = 0)$ can be determined, but the faster the wave packet spreads. Experimentally, this can be illustrated as follows: If we apply a short voltage pulse to the cathode at time $t = 0$, then electrons can start travelling towards the detector at this instance. The emitted electrons have a velocity distribution $\Delta v$, such that electrons with differing velocities $v$ will not necessarily be in the same location $x$ at a later point in time $t$. Instead they are spread over the interval $\Delta x(t) = t \cdot \Delta v$. The velocity distribution is described by $\Delta v \propto \Delta k$ of the wave packet, such that the location uncertainty $\Delta x$ \[ \dv{(\Delta x(t))}{t} = \Delta v(t = 0) = \frac{\hbar}{m} \Delta k(t = 0) \] changes proportionally to the initial impulse uncertainty. \end{document}