{ "cells": [ { "cell_type": "markdown", "metadata": {}, "source": [ "## Finite Difference Method for Solving Schrödinger Equation\n", "### Hydrogen radial equation\n", "\n", "The radial equation for hydrogen (in SI units) is \n", "\n", "$$ \n", "-\\frac{\\hbar^2}{2mr}\\frac{d^2}{d r^2}\\, (r\\psi) \n", " + \\frac{\\hbar^2}{2m}\\, \\frac{l(l+1)}{r^2}\\psi \n", " - \\frac{e^2}{4\\pi\\epsilon_0}\\frac{1}{r} \\psi = E\\psi.\n", "$$\n", "\n", "It's standard to rewrite this in terms of a so-called radial wavefunction $u$,\n", "where \n", "\n", "$$\n", "\\psi \\equiv \\frac{u(r)}{r}.\n", "$$\n", "\n", "The radial equation can then be written in the form\n", "\n", "$$\n", "-\\frac{d^2u}{dr^2} + \\frac{l(l+1)}{r^2}u - \\frac{2me^2}{4\\pi\\epsilon_0 \\hbar^2 r}u\n", " = \\frac{2mE}{\\hbar^2}u.\n", "$$\n", "\n", "Experienced physicists might be immediately inclined to rewrite this equation \n", "in terms of the dimensionless length paramater $r^\\prime \\equiv r/a_0$, where\n", "$a_0$ is the Bohr radius, but such previous acquaintance woth the hydrogen atom\n", "isn't essential. Each term in this form of the radial equation has dimensions of (length)$^{-2}$. Examination of the third term on the left side of the equation \n", "suggests that it might useful to use a dimensionless length parameter made up of fundamental constants characterizing the appropriate scale for this system,\n", "\n", "$$\n", "r^\\prime = \\frac{r}{a},\n", "$$\n", "\n", "where \n", "\n", "$$\n", "a \\equiv \\frac{4\\pi\\epsilon_0\\hbar^2}{me^2}.\n", "$$\n", "\n", "This is, in fact the Bohr radius.\n", "\n", "Written terms of $r^\\prime$ the radial equation becomes\n", "\n", "$$\n", "-\\frac{d^2u}{d{r^\\prime}^2} + \\frac{l(l+1)u}{{r^\\prime}^2} - \\frac{2u}{r^\\prime} \n", " = \\frac{2\\hbar^2 (4\\pi\\epsilon_0)^2}{me^4} E u.\n", "$$\n", "\n", "or, defining a dimensionless energy \n", "\n", "$$\n", "E^\\prime \\equiv \\frac{E}{\\frac{me^4}{2\\hbar^2 (4\\pi\\epsilon_0)^2}} = \\frac{E}{13.6\\, \\mbox{eV}},\n", "$$\n", "\n", "the radial equation becomes\n", "\n", "$$\n", "-\\frac{d^2u}{d{r^\\prime}^2} + \\frac{l(l+1)u}{{r^\\prime}^2} - \\frac{2u}{r^\\prime} \n", " = E^\\prime u.\n", "$$\n", "\n", "This is now in a good form for computational work, with no messy physical constants.\n", "\n", "\n", "I use a finite-difference method to turn the solving of Schrödinger's into an eigenvalue problem. Briefly, after discretizing $r$, (i.e., $r^\\prime_j = \n", "j\\Delta$), an approximate version of Schrödinger's equation can be written as \n", "\n", "$$\n", "\\frac{-u_{j+1} + 2u_j - u_{j-1}}{\\Delta^2} + \\left(\\frac{l(l+1)}{{r^\\prime_j}^2} \n", " - \\frac{2}{r^\\prime_j}\\right) u_j = E^\\prime u_j.\n", "$$\n", "\n", "The term in parentheses is sometimes called an effective potential $U_{\\rm eff}$.\n", "\n", "This is an eigenvalue problem:\n", "\n", "$$ \n", "H_{ji}\\psi_i = E^\\prime \\psi_j,\n", "$$\n", "\n", "where \n", "\n", "\n", "$$\n", "H_{ji} = \\left\\{\\begin{array}{cl}\n", " \\frac{2}{\\Delta^2} + U_{\\rm eff}(r^\\prime_i) & \\mbox{for $i=j$} \\\\\n", " -\\frac{1}{\\Delta^2} & \\mbox{for $i = j\\pm 1$}\\\\\n", " 0 & \\mbox{otherwise}\n", " \\end{array}\\right.\n", "$$\n", "\n", "The eigenvalues give the energy of the states, and the eigenvectors are numerical\n", "approximations of the wavefunctions.\n", "\n", "[The method can be extended to more than one dimension and to situations with more than \n", "one particle. I have used this technique for a variety of one-dimensional potentials, \n", "and I have extended it to treat the two-dimensional harmonic oscillator, \n", " excited states of helium. For a recent pedagogical discussion of the method, \n", "see Matrix Numerov method for solving Schrödinger's equation,\n", "Mohandas Pillai, Joshua Goglio, and Thad G. Walker, Am. J. Phys. 80, 1017 (2012)]" ] }, { "cell_type": "code", "execution_count": 1, "metadata": {}, "outputs": [], "source": [ "import numpy as np\n", "from scipy import linalg\n", "\n", "import matplotlib as mpl\n", "import matplotlib.pyplot as plt" ] }, { "cell_type": "code", "execution_count": 2, "metadata": {}, "outputs": [], "source": [ "# Following is an Ipython magic command that puts figures in the notebook.\n", "%matplotlib notebook\n", "\n", "# M.L. modification of matplotlib defaults\n", "# Changes can also be put in matplotlibrc file, \n", "# or effected using mpl.rcParams[]\n", "mpl.style.use('classic')\n", "plt.rc('figure', figsize = (6, 4.5)) # Reduces overall size of figures\n", "plt.rc('axes', labelsize=16, titlesize=14)\n", "plt.rc('figure', autolayout = True) # Adjusts supblot parameters for new size" ] }, { "cell_type": "code", "execution_count": 3, "metadata": {}, "outputs": [], "source": [ "def u(x): # Effective potential energy function\n", " return l*(l+1)/x**2 - 2/x" ] }, { "cell_type": "code", "execution_count": 4, "metadata": {}, "outputs": [], "source": [ "n = 2000 # Number of intervals (J=1 in my notes)\n", "dim = n - 1 # Number of internal points\n", "xl = 0 # xl corresponds to origin\n", "xr = 200. # \n", "delta = (xr-xl)/n\n", " \n", "x = np.linspace(xl+delta,xr-delta,dim)\n", "\n", "l = 1 # orbital quantum number\n", "\n", "#Fill Hamiltonian\n", "h = np.zeros((dim,dim),float)\n", "for i in range(len(h)-1):\n", " h[i,i+1] = h[i+1,i] = -1/delta**2 \n", "\n", "for i in range(len(h)):\n", " h[i,i] = 2./delta**2 + u(x[i]) \n", "\n", "vals, vecs = linalg.eigh(h) #Note: eigenvectors in columns of vecs" ] }, { "cell_type": "code", "execution_count": 5, "metadata": {}, "outputs": [ { "data": { "application/javascript": [ "/* Put everything inside the global mpl namespace */\n", "window.mpl = {};\n", "\n", "\n", "mpl.get_websocket_type = function() {\n", " if (typeof(WebSocket) !== 'undefined') {\n", " return WebSocket;\n", " } else if (typeof(MozWebSocket) !== 'undefined') {\n", " return MozWebSocket;\n", " } else {\n", " alert('Your browser does not have WebSocket support. 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