P301 Lecture 19 “Fourier Decomposition/analysis”

Slides:



Advertisements
Similar presentations
Schrödinger Representation – Schrödinger Equation
Advertisements

Introduction to Quantum Theory
Quantum One: Lecture 3. Implications of Schrödinger's Wave Mechanics for Conservative Systems.
Quantum Theory of Light A TimeLine. Light as an EM Wave.
Lecture 5 The Simple Harmonic Oscillator
Thanks to Zarah.
Application of quantum in chemistry
1Recap. 2 Quantum description of a particle in an infinite well  Imagine that we put particle (e.g. an electron) into an “infinite well” with width L.
PHY 102: Waves & Quanta Topic 14 Introduction to Quantum Theory John Cockburn Room E15)
Given the Uncertainty Principle, how do you write an equation of motion for a particle? First, remember that a particle is only a particle sort of, and.
1 Recap T.I.S.E  The behaviour of a particle subjected to a time-independent potential is governed by the famous (1-D, time independent, non relativisitic)
Almost all detection of visible light is by the “photoelectric effect” (broadly defined.) There is always a threshold photon energy for detection, even.
P460 - square well1 Square Well Potential Start with the simplest potential Boundary condition is that  is continuous:give: V 0 -a/2 a/2.
LECTURE 16 THE SCHRÖDINGER EQUATION. GUESSING THE SE.
Project topics due today. Next HW due in one week
Ch 9 pages ; Lecture 21 – Schrodinger’s equation.
PHYS 3313 – Section 001 Lecture #17
Volunteer via to: (Anne Foley) Or go to the front office. OPEN HOUSE 23 Oct
The Hydrogen Atom Quantum Physics 2002 Recommended Reading: Harris Chapter 6, Sections 3,4 Spherical coordinate system The Coulomb Potential Angular Momentum.
P460 - Sch. wave eqn.1 Solving Schrodinger Equation If V(x,t)=v(x) than can separate variables G is separation constant valid any x or t Gives 2 ordinary.
From last time: 1. show that is also a solution of the SE for the SHO, and find the energy for this state 2. Sketch the probability distribution for the.
To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are.
Some topics in research Atomic Physics at the EBIT center of Fudan University Gordon Berry Physics Department, University of Notre Dame A five-week class.
Particle in a Well (PIW) (14.5) A more realistic scenario for a particle is it being in a box with walls of finite depth (I like to call it a well) – Particles.
Ch ; Lecture 26 – Quantum description of absorption.
مدرس المادة الدكتور :…………………………
Young/Freeman University Physics 11e. Ch 40 Quantum Mechanics © 2005 Pearson Education.
1 Reading: QM course packet- ch 5.5 ENERGY EIGENFUNCTIONS & EIGENVALUES OF THE FINITE WELL.
Wednesday, Oct. 17, 2012PHYS , Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #13 Wednesday, Oct. 17, 2012 Dr. Jaehoon Yu Properties.
Physics 361 Principles of Modern Physics Lecture 14.
Topic 5: Schrödinger Equation
Physics 361 Principles of Modern Physics Lecture 11.
Simple Harmonic Oscillator (SHO) Quantum Physics II Recommended Reading: Harris: chapter 4 section 8.
Lecture 5 The Simple Harmonic Oscillator
Time-independent Schrodinger eqn QM Ch.2, Physical Systems, 12.Jan.2003 EJZ Assume the potential V(x) does not change in time. Use * separation of variables.
Monday, April 6, 2015PHYS , Spring 2015 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #17 Monday, April 6, 2015 Dr. Jaehoon Yu Normalization.
Two-slit experiment with particles
Physics 361 Principles of Modern Physics Lecture 13.
LECTURE 17 THE PARTICLE IN A BOX PHYSICS 420 SPRING 2006 Dennis Papadopoulos.
Modern Physics lecture 4. The Schroedinger Equation As particles are described by a wave function, we need a wave equation for matter waves As particles.
Lecture 12, p 1 Lecture 12: Particle in 1D boxes, Simple Harmonic Oscillators U  x n=0n=1n=2n=3 U(x)  (x)
An equation for matter waves Seem to need an equation that involves the first derivative in time, but the second derivative in space As before try solution.
1924: de Broglie suggests particles are waves Mid-1925: Werner Heisenberg introduces Matrix Mechanics In 1927 he derives uncertainty principles Late 1925:
Lectures in Physics, summer 2008/09 1 Modern physics 2. The Schrödinger equation.
Wavefunctions and Quantum Wells
Schrodinger’s Equation Solutions Finite Square Well
Solutions of Schrodinger Equation
Lecture 18 3D Cartesian Systems
UNIT 1 Quantum Mechanics.
Schrödinger Representation – Schrödinger Equation
QM Review and SHM in QM Review and Tunneling Calculation.
Quantum Mechanics.
Quantum Mechanics for Scientists and Engineers
CHAPTER 5 The Schrodinger Eqn.
PHYS274 Quantum Mechanics VII
“All of modern physics is governed by that magnificent and thoroughly confusing discipline called quantum mechanics...It has survived all tests and there.
What’s coming up??? Nov 3,5 Postulates of QM, p-in-a-box Ch. 9
From Last time… De Broglie wavelength Uncertainty principle
CHAPTER 5 The Schrodinger Eqn.
CHAPTER 5 The Schrodinger Eqn.
Solving Schrodinger Equation: ”Easy” Bound States
Elements of Quantum Mechanics
Quantum Mechanics.
Particle in a Box.
Source: D. Griffiths, Introduction to Quantum Mechanics (Prentice Hall, 2004) R. Scherrer, Quantum Mechanics An Accessible Introduction (Pearson Int’l.
Particle in a box Potential problem.
More Quantum Mechanics
Infinite Square Well.
More About Matter Waves
Wave-Particle Duality and the Wavefunction
Presentation transcript:

P301 Lecture 19 “Fourier Decomposition/analysis”

Two-slit experiment with particles

Schrodinger’s Equation The above is taken from Wikipedia, and here the “Laplacian” operator in the first term on the right hand side is simply a short-hand for (  2 = d 2 /dx 2 + d 2 /dy 2 d 2 /dz 2 ). We will concentrate (for the most part) upon the version that does not involve time and restrict ourselves to one dimension. The book goes through the details through the “separation of variables” technique, and the result is (for one dimension): This is the “time-independent Schrodinger equation” (the version we will deal with exclusively, in one dimension

P301 Lecture 19 “JITT question” 1.Describe, as simply as you can, the “boundary conditions” that were imposed on the open and closed ends of organ pipes in P221 (or whatever first semester intro Physics course you took). 7 answers were confused or confusing The boundaries were such that they did not cause destructive interference, that is, they were integer multiples of the wavelength of sound wave. (About 6 People concentrated on continuity of the function and wavelength.) [Never took P221 or P201, but I'll give it a shot...] Nodes must occur at closed ends, antinodes at open ends, and the wavelengths of the resonant frequencies must occur in such a way to allow this restriction for the ends of the pipes. (10 people concentrated on this: This is exactly what “BOUNDARY CONDITIONS” refers to) 18 didn’t answer.

 (x) must be finite “everywhere” (except possibly for a set of measure zero).  (x) must be single valued 3.For finite potentials both  (x) and d  (x)/dx must be continuous. 4.The integral of |  (x)| 2 must be finite (and is normally chosen to be equal to one for a “properly normalized” wavefunction) 5.Behaviour at boundaries must be correct in order for all of these above conditions to be met, e.g. for a particle in a box, y(x) must be equal to zero at the box’s boundaries. Schrodinger’s Equation Conditions on the function  (x) There is a nice “live” graph showing the wavefunctions for the particle in a box (1-D infinite square well) problem at: Interesting “shooting algorithm example of ODE solving at:

Schrodinger’s Equation Solutions Infinite Square Well Useful web site for integrating

Volunteer via to: (Susie Rogers) Or go to the front office. OPEN HOUSE 31 Oct 2009

Schrodinger’s Equation Solutions Finite Square Well Unlike the infinite case, in this case, there will only be a finite number of bound states (i.e. states for which there are classically forbidden regions where V>E.

What is the most significant difference you see between the wave functions for a particle in an “infinite square well” and those for a particle in a “finite square well” of the same width? Which of well would you expect to have higher energy for its ground state (again, assuming both have the same width)? Differences: Particle can exist outside the well for the finite case (11 answers) Larger for the finite case (3 answers) Other 5 No answer (21 answers) Higher Energy in which well? Infinite case (15 answers) Finite case (2 answers) ? (2 answers) Lecture 20 JITT question

Schrodinger’s Equation Solutions Finite Square Well Recall from class that we can recast the transcendental equation into a dimensionless form, where the controlling parameter is the ratio of the potential well depth to the “confinement energy”. You can get the spreadsheet for the even solutions from the website: 301/F09/Homework/ 301/F09/Homework/ The fig. shows the marginal case for two even solutions (3 overall)  =  2 For this case, you must solve a transcendental equation to find the solutions that obey the boundary conditions (in particular, continuity of the function and its derivative at the well boundary). For the geometry we considered in class, this takes on one of two forms: Even solutions  =k tan(ka/2) ; Odd solutions  = -k cot(ka/2)

Schrodinger’s Equation Solutions Harmonic Oscillator There are an infinite number of possible states, since the potential is defined to keep going up (of course this is an idealization). Interestingly, the energy levels are evenly spaced in this case: E = h  (n + ½) n = 0, 1, 2, …

How would you expect the light absorption spectrum for an electron trapped in a harmonic potential to differ from that for an electron trapped in an infinite square well potential? Yes, because just like in the finite square well, harmonic oscillators don't need to have nodes at their edges unlike infinite square wells. Therefore, they work with different types of waves. (several, like this, were tangential to the question, e.g. focused on wavefunction not absorption) I would expect it to take more energy to knock the infinite square well particles to a lower energy level, so they would emit more energetic photons. (about 4 people focused on absolute energy differences, but this depends on the parameters defining the wells, not just their shape). Energy levels for the infinite well vary with the square of quantum #, whereas for SHM they vary with (n+0.5). So spectrum bands for the SHM case should come at integral multiples of h-bar*omega whereas in the infinite well the bands will appear more irregular b/c of the exponential growth of E. (this is the key). Lecture 20 JITT question