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Quantum Mechanics: Numerical Solution of Schrödinger's Equation, Study notes of Physics

An introduction to quantum mechanics, explaining why and when it became necessary to replace classical physics with this radical new theory. It covers the basics of quantum mechanics, including the concept of wavefunctions and the time-independent schrödinger equation. The document also discusses the numerical solution of schrödinger's equation and the concept of stationary states, allowing for only certain energies to be present.

Typology: Study notes

Pre 2010

Uploaded on 08/09/2009

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Download Quantum Mechanics: Numerical Solution of Schrödinger's Equation and more Study notes Physics in PDF only on Docsity! Lec9 • Intro to Quantum Mechanics • Numerical solution of Schödinger’s equa- tion 1 Why/when quantum ? • Newton’s laws give a very accurate descrip- tion of the behavior of everyday objects/motions. • But they fail miserably to describe atoms ! • This was a crisis for physics at turn of cen- tury ... • Eg Laws of EM + Newton mechanics pre- dicts atoms should be unstable • Electrons classically have any energy but see only discrete energies • Energy of electromagnetic waves in vac- uum infinite! 2 Basics • Discard notion that microscopic objects like electrons can a well defined position, veloc- ity etc. • Not a practical issue but one of principle! • Instead think of them as being described by a wavefunction Ψ(x,t). Like a usual wave in sense that electron is not localized like a classical particle. • But this is a probability wave. |Ψ(x, t)|2 yields probability of finding particle at (x, t). • Dynamics: replace Newton’s laws (simple ordinary differential equations) by Schrödnger’s equation (partial differential equation) 4 Points to note − h̄2 2m ∂2Ψ ∂x2 + V Ψ = ih̄ ∂Ψ ∂t • Equation looks like a funny wave equation (but only first order in t) • Involves square root of minus 1 (i). In gen- eral Ψ is complex! Hence need |Ψ|2 for positive real probability • New fundamental constant introduced h̄ = 1.05 × 10−34 Js. Planck’s constant. 5 Stationary states • Put Ψ = φ(x)e−iEt/h̄. Plug into equation. Find time independent Schrödinger equa- tion − h̄2 2m ∂2φ ∂x2 + V φ = Eφ • Such a wavefunction describes the allowed state of say electron in an atom with E being its energy. • Try to solve schematically. In general only certain energies allowed! 6 How to solve numerically ? Rewrite equations: dφ dx = p dp dx = [ 2m (V (x) − E) h̄2 ] φ Consider case V (−x) = V (x). Can show φ(x) is either even or odd function. In former case choose φ(0) = 1 and p(0) = 0 Choose some E and integrate equations using Euler/leapfrog. Look at |φ(x)| for large |x|, If it is growing will not be able to impose ∫ φ2 = 1. Choose another E and try again. Shooting method. 9 Summary • Find only discrete set of E work. So both wavefunction and E are output from cal- culation! • E0 > Vmin. Particle cannot be stationary at minimum of potential. Quantum fluc- tuations. • E increases with number of oscillations. 10
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