III. Direct evolution of the density: The Liouville Operator

Similar documents
The Quantum Theory of Atoms and Molecules: The Schrodinger equation. Hilary Term 2008 Dr Grant Ritchie

Lecture #11: Wavepacket Dynamics for Harmonic Oscillator

ψ ( t) = c n ( t) t n ( )ψ( ) t ku t,t 0 ψ I V kn

7.3. QUANTUM MECHANICAL TREATMENT OF FLUCTUATIONS: THE ENERGY GAP HAMILTONIAN

ψ ( t) = c n ( t ) n

Comparison between the Discrete and Continuous Time Models

2.3 SCHRÖDINGER AND HEISENBERG REPRESENTATIONS

( ) = b n ( t) n " (2.111) or a system with many states to be considered, solving these equations isn t. = k U I ( t,t 0 )! ( t 0 ) (2.

F (u) du. or f(t) = t

Homework Solution Set # 3. Thursday, September 22, Textbook: Claude Cohen Tannoudji, Bernard Diu and Franck Lalo, Second Volume Complement G X

ln y t 2 t c where c is an arbitrary real constant

ψ(t) = V x (0)V x (t)

Two Coupled Oscillators / Normal Modes

02. MOTION. Questions and Answers

Some Basic Information about M-S-D Systems

Physics 127b: Statistical Mechanics. Fokker-Planck Equation. Time Evolution

Additional Exercises for Chapter What is the slope-intercept form of the equation of the line given by 3x + 5y + 2 = 0?

Lecture 9: Advanced DFT concepts: The Exchange-correlation functional and time-dependent DFT

Scattering and Decays from Fermi s Golden Rule including all the s and c s

From Particles to Rigid Bodies

ODEs II, Lecture 1: Homogeneous Linear Systems - I. Mike Raugh 1. March 8, 2004

System of Linear Differential Equations

Structural Dynamics and Earthquake Engineering

( ) ( ) if t = t. It must satisfy the identity. So, bulkiness of the unit impulse (hyper)function is equal to 1. The defining characteristic is

LAPLACE TRANSFORM AND TRANSFER FUNCTION

10. State Space Methods

THE MYSTERY OF STOCHASTIC MECHANICS. Edward Nelson Department of Mathematics Princeton University

Wave Mechanics. January 16, 2017

û s L u t 0 s a ; i.e., û s 0

23.2. Representing Periodic Functions by Fourier Series. Introduction. Prerequisites. Learning Outcomes

Module 3: The Damped Oscillator-II Lecture 3: The Damped Oscillator-II

Lecture 2-1 Kinematics in One Dimension Displacement, Velocity and Acceleration Everything in the world is moving. Nothing stays still.

Numerical Dispersion

where the coordinate X (t) describes the system motion. X has its origin at the system static equilibrium position (SEP).

t is a basis for the solution space to this system, then the matrix having these solutions as columns, t x 1 t, x 2 t,... x n t x 2 t...

3.1.3 INTRODUCTION TO DYNAMIC OPTIMIZATION: DISCRETE TIME PROBLEMS. A. The Hamiltonian and First-Order Conditions in a Finite Time Horizon

Wall. x(t) f(t) x(t = 0) = x 0, t=0. which describes the motion of the mass in absence of any external forcing.

Maxwell s Equations and Electromagnetic Waves

Chapter 2. First Order Scalar Equations

Our main purpose in this section is to undertake an examination of the stock

CHEMISTRY 047 STUDY PACKAGE

Lecture 4 Kinetics of a particle Part 3: Impulse and Momentum

Physics 235 Chapter 2. Chapter 2 Newtonian Mechanics Single Particle

Program: RFEM 5, RSTAB 8, RF-DYNAM Pro, DYNAM Pro. Category: Isotropic Linear Elasticity, Dynamics, Member

Math Week 15: Section 7.4, mass-spring systems. These are notes for Monday. There will also be course review notes for Tuesday, posted later.

Many Electron Theory: Time dependent perturbations and propagation.

Math 333 Problem Set #2 Solution 14 February 2003

Linear Surface Gravity Waves 3., Dispersion, Group Velocity, and Energy Propagation

Class Meeting # 10: Introduction to the Wave Equation

Today in Physics 218: radiation reaction

Solutions to Assignment 1

The expectation value of the field operator.

k 1 k 2 x (1) x 2 = k 1 x 1 = k 2 k 1 +k 2 x (2) x k series x (3) k 2 x 2 = k 1 k 2 = k 1+k 2 = 1 k k 2 k series

THE CATCH PROCESS (continued)

Chapter 6. Systems of First Order Linear Differential Equations

Linear Dynamic Models

Theory of! Partial Differential Equations!

Excel-Based Solution Method For The Optimal Policy Of The Hadley And Whittin s Exact Model With Arma Demand

Differential Equations

Solutions of Sample Problems for Third In-Class Exam Math 246, Spring 2011, Professor David Levermore

1 1 + x 2 dx. tan 1 (2) = ] ] x 3. Solution: Recall that the given integral is improper because. x 3. 1 x 3. dx = lim dx.

Electrical Circuits. 1. Circuit Laws. Tools Used in Lab 13 Series Circuits Damped Vibrations: Energy Van der Pol Circuit

Theory of! Partial Differential Equations-I!

dt = C exp (3 ln t 4 ). t 4 W = C exp ( ln(4 t) 3) = C(4 t) 3.

ANALYSIS OF LINEAR AND NONLINEAR EQUATION FOR OSCILLATING MOVEMENT

INDEX. Transient analysis 1 Initial Conditions 1

TMA4329 Intro til vitensk. beregn. V2017

Chapter Q1. We need to understand Classical wave first. 3/28/2004 H133 Spring

Designing Information Devices and Systems I Spring 2019 Lecture Notes Note 17

Notes 04 largely plagiarized by %khc

2001 November 15 Exam III Physics 191

Product Operators. Fundamentals of MR Alec Ricciuti 3 March 2011

15. Vector Valued Functions

Linear Time-invariant systems, Convolution, and Cross-correlation

Lecture #8 Redfield theory of NMR relaxation

28. Quantum Physics Black-Body Radiation and Plank s Theory

MOMENTUM CONSERVATION LAW

Math Final Exam Solutions

V.sin. AIM: Investigate the projectile motion of a rigid body. INTRODUCTION:

!!"#"$%&#'()!"#&'(*%)+,&',-)./0)1-*23)

4. Electric field lines with respect to equipotential surfaces are

d 1 = c 1 b 2 - b 1 c 2 d 2 = c 1 b 3 - b 1 c 3

The motions of the celt on a horizontal plane with viscous friction

MTH Feburary 2012 Final term PAPER SOLVED TODAY s Paper

Waves are naturally found in plasmas and have to be dealt with. This includes instabilities, fluctuations, waveinduced

Stochastic Reliability Analysis of Two Identical Cold Standby Units with Geometric Failure & Repair Rates

Traveling Waves. Chapter Introduction

IB Physics Kinematics Worksheet

Continuous Time. Time-Domain System Analysis. Impulse Response. Impulse Response. Impulse Response. Impulse Response. ( t) + b 0.

arxiv:cond-mat/ May 2002

Announcements: Warm-up Exercise:

Effects of Coordinate Curvature on Integration

Linear Response Theory: The connection between QFT and experiments

On two general nonlocal differential equations problems of fractional orders

Physics 1402: Lecture 22 Today s Agenda

EE650R: Reliability Physics of Nanoelectronic Devices Lecture 9:

Chapter 8 The Complete Response of RL and RC Circuits

Math 10B: Mock Mid II. April 13, 2016

Reading from Young & Freedman: For this topic, read sections 25.4 & 25.5, the introduction to chapter 26 and sections 26.1 to 26.2 & 26.4.

Stochastic Structural Dynamics. Lecture-6

Transcription:

Cem 564 Lecure 8 3mar From Noes 8 003,005,007, 009 TIME IN QUANTUM MECANICS. I Ouline I. Te ime dependen Scroedinger equaion; ime dependence of energy eigensaes II.. Sae vecor (wave funcion) ime evoluion A. 3 cases of a -sae problem B. cases of linear combinaion of infinie number of eigensaes: wave paces ) an oscillaing wave pace (model for a laser); gaussian pace in parabolic well ) a free "paricle": propagaion of a gaussian wave pace under no force. III. Direc evoluion of e densiy: Te Liouville Operaor I. Energy Eigensaes ave Saionary Densiy (are saionary saes) Te ime dependen Scroedinger equaion, Ψ( x, ) ˆ Ψ( x, ) is arguably e mos fundamenal equaion discovered by umanind. I predics e fuure providing we now e presen. Aloug we canno now e wave funcion of e world, be can in cerain experimens now e wave funcion of a small isolaed par of e world and use is equaion o undersand e resuls of e experimen. If Ψ EΨ, en e above equaion says Ψ( x, ) E Ψ( x, ) and e soluion is: Ψ or ( x, ) Ψ( x,0) e E Ψ Ψ E ( Ψ ( x, ) Ψ ( x, ) e. Tus, a any ime,, Ψ Ψ( x, ) ( x, ) f( x) i.e., is independen of ime. )

Cem 564 Lecure 8 3mar II. Time Dependence of Wave funcions (wo-level sysem) Recipe: ) Use Scroedinger Eq. o ge Ψ. (inegrae dψ () ) ) ge densiy from Ψ*() Ψ (). Le Θ > c () > + c () >, were > and > depend on space only. Ten, Ψ c() c() ) ) + c() i c() Ge wo equaions by muliplying on e lef by < and by <. c i c i () () c () c i c i () () c () Scroedinger equaion. Tis is e exac wo-sae form of e We nex examine ree special cases. Te general resul is a mixure of ese ree cases. Case : Resonance, real ineracion: > 0 ; 0 c i () c () c i () c () Te soluion is : c () cos( ) cos( ω ) c () isin( ) sin( ω ) wi ω as can readily be demonsraed by subsiuion ino e wo coupled equaions above.

Cem 564 Lecure 8 3mar 3 Evoluion if c (0) and c (0) 0 c : 0-0 c : 0 -i 0 i 0 We see a e resul is a periodic reurn o e iniial sae--e caracerisic of resonance. In erms of e sae funcion (vecor): i i + i i i + i Tis resul says a e sronger e ineracion e iger e frequency and e sorer e period of oscillaion. Tis is e fases possible rae for moving from sae > o sae >. Te ime required o cange compleely from sae > o sae > is e ime suc a /ћ π/, i.e., wen π/ 4 A pysical example of suc a resonance is an excied aom nex o an unexcied one. A* B A B* As depiced, e ineracion can be roug space (coulombic), called resonance energy ransfer, or e exciaion could be ransfered by double elecron excange creaed by orbial overlap, or BOT. A* B A B*

Cem 564 Lecure 8 3mar 4 Densiy Marix Evoluion In e end, wa couns is e ow e probabiliy densiy canges in ime. Densiy is given by Ψ Ψ ( c + c )( c + c ) cc + cc + cc + cc, wic defines e densiy marix, cc cc ρ() cc cc cos ( ω) icos( ω) sin( ω) icos( ω) sin( ω) sin ( ω) wic evolves in e periodic manner: 0 0 0 05. i05. 0 0 05 05 i.. 0 05. 05. 0 05 05 i.. 0 0 Case : Resonance, imaginary ineracion: - ib, b>0 ; 0 Same as case excep for e pase: c ( ) cos(cos( ω ) c () sin( ω ) wi ω Te evoluion of e densiy marix in is case is: 0 0 0 05. 05. 0 0 05 05 0 05 05 0.. 05 05.... 0 0

Cem 564 Lecure 8 3mar 5 Case 3: Non-resonance, no ineracion : 0 ; 0 Tis is a simple linear combinaion of wo energy eigensaes. Tis resuls in wo uncoupled equaions. c i c i E () () c() c i c i E () () c () Te soluion of eac is jus as in e opening lines of is andou. owever, now we will loo o see ow e densiy canges in ime. Noe a e diagonal is ime independen, i.e., e probabiliies o be in e saes > and > are consan in ime if 0. owever e densiy does oscillae. Consider a 50% mixure a ime 0: Ψ ( 0) c() 0 c() 0 c() 0 c() 0 e ρ ( E E) * * c () 0 c () 0 e c () 0 c () 0 c () c () 0 e,, + ( E ) ( E E) * * ρ c ( 0) c ( 0) + c ( 0) c ( 0) + c ( 0) c ( 0) e + c ( 0) c ( 0) e If < s and < p and bo are real, ρ 0.5(s + p ) +cos(ω ) (ss), were ω (E p - E s )/ħ. Wen ω 0, e funcion is a ybrid orbial poining o e rig: and wen ω π, e funcion is a ybrid orbial poining o e lef: ( E E ) ( E E) ( E E) + i ρ( ) + e + e ( E E )

Cem 564 Lecure 8 3mar 6 In is case ere is an oscillaing dipole. Tis oscillaing dipole (called e elecric dipole ransiion momen or ransiion dipole) is wa ineracs wi lig during absorpion and emission. Is magniude deermines e rae of absorpion of lig. Wenever wo saes differ by one node as in is case, e ransiion dipole will be large and e ransiion will be srongly allowed. For a general superposiion of energy eigensaes: ( E ) Ψ () c ( 0) e m, ( E Em) * c () 0 c () 0 e m m ( E) m ( Em) i ω m * ω m c( 0) c( 0) + ( c( 0) cm( 0) e m + cm() 0 c() 0 e m ), * ρ Ψ() Ψ() ( c () 0 e )( c () 0 e m) were w m ( E Em) < m Noe a e wo erms in e second summaion are complex conjugaes, so e densiy is real, as i mus be. Eac erm in e second sum modulaes e saic average densiy given by e firs sum. Te Fourier ransform of e densiy would reveal one erm for every disinc energy difference beween e various energy eigenvalues represened. m B. Wave Paces. Coeren superposiion of armonic oscillaor wave funcions: Te oscillaing Gaussian wave pace. For e armonic oscillaor eigenvalues: E n (n +½) ħω. Consider e idealizaion of a very sor and inense laser pulse a elecronically excied a diaomic molecule wose excied sae vibraional poenial minimum is displaced from e ground minimum by an amoun d. Ten λ ½d / ħω

Cem 564 Lecure 8 3mar 7 Te vibraional funcion creaed in erms of e armonic oscillaor eigensaes on e upper surface are given by Ψ () e n/ / λ λ n 0 n! e i( n+ ) ω Noice a e squares of e coefficiens are e now familiar Franc-Condon facors (Poisson disribuion formula). Te densiy arising from is wave funcion as an amazing beavior. Te modulaing cross erms conspire o eep e gaussian sape of e iniial probabiliy densiy a all imes, bu is cener moves in ime precisely as would a classical paricle of e same mass in a poenial saring wi zero velociy a a poin! n

Cem 564 Lecure 8 3mar 8. Gaussian Superposiion of Momenum Eigenfuncions: Moion of A Free "Paricle" Below is sown an x-momenum eigenfuncion being operaed upon by e x-momenum operaor: i x e ix e ix Te energy of ese saes is E p /m ħ /m. Terefore e wave funcion wi is ime facor is given by: i m i( x ω ) Ψ ( x, ) e ix e e A superposiion of momenum eigenfuncions is erefore: Ψ () c e i( x ω ) If e c form a gaussian funcion, c ( ) a ( ) e 4 0 wi infiniesimally spaced values, e above summaion becomes e inegral below: 4 i( x ω ) Ψ ( x, ) N e e d a a ( ) 0 Tis inegral is sraigforward, and leads o e following expression for e probabiliy densiy (see Coen-Tannoudji, pp 6-65): ΨΨ * N a () e 0 a ( x ) m 4 4 a + m i.e., e densiy is a gaussian wic moves in e x direcion wi velociy ħ 0 /m and wose wid is increasing in ime. Te normalizaion consan erefore also increases in ime. Wiou e parabolic poenial energy well o eep refocusing e pace, i spreads wi increasing ime.

Cem 564 Lecure 8 3mar 9 III. Direc ime dependence of e DENSITY: Te Liouville Operaor Tae e ime derivaive of e densiy operaor: ( ) ρ $ () () () () () () Ψ Ψ Ψ Ψ + Ψ Ψ, ( ) i $ bu Ψ Ψ() adj $ and, Ψ() i Ψ() so, ρ i $ $ $ Ψ() Ψ() Ψ() Ψ() + i Ψ() Ψ() ( ) ρ i ρ ρ i $ $ $ $ [ $ i, ρ $ ] L $ ρ $ adj were L e Liouville Operaor or e Liouvillian and e above equaion is nown as e Liouville Equaion. I is equivalen o e Scroedinger Equaion in is form, bu if one allows e bras and es o evolve separaely in ime, i is more powerful. ρ i $ $(,') Ψ() Ψ(') Ψ() Ψ(') + i Ψ() Ψ(') $ adj Te laer form is necessary o properly describe cerain penomena.