Note 2. Ling fong Li. 1 Klein Gordon Equation Probablity interpretation Solutions to Klein-Gordon Equation... 2

Similar documents
Lorentz Group. Ling Fong Li. 1 Lorentz group Generators Simple representations... 3

Lecture 6/7 (February 10/12, 2014) DIRAC EQUATION. The non-relativistic Schrödinger equation was obtained by noting that the Hamiltonian 2

( ) r! t. Equation (1.1) is the result of the following two definitions. First, the bracket is by definition a scalar product.

Chapter 6. Rotations and Tensors

G : Statistical Mechanics

Advanced Quantum Mechanics

The Feynman path integral

Inner Product. Euclidean Space. Orthonormal Basis. Orthogonal

Quantum Mechanics I - Session 4

3. Stress-strain relationships of a composite layer

THEOREMS OF QUANTUM MECHANICS

Scattering of two identical particles in the center-of. of-mass frame. (b)

we have E Y x t ( ( xl)) 1 ( xl), e a in I( Λ ) are as follows:

A finite difference method for heat equation in the unbounded domain

Lowest-Order e + e l + l Processes in Quantum Electrodynamics. Sanha Cheong

Lagrangian Field Theory

Andre Schneider P622

LECTURE 21 Mohr s Method for Calculation of General Displacements. 1 The Reciprocal Theorem

9 Characteristic classes

14 The Postulates of Quantum mechanics

Associative Memories

Salmon: Lectures on partial differential equations. Consider the general linear, second-order PDE in the form. ,x 2

Poisson brackets and canonical transformations

Quantum Mechanics for Scientists and Engineers. David Miller

n α j x j = 0 j=1 has a nontrivial solution. Here A is the n k matrix whose jth column is the vector for all t j=0

k p theory for bulk semiconductors

Snce h( q^; q) = hq ~ and h( p^ ; p) = hp, one can wrte ~ h hq hp = hq ~hp ~ (7) the uncertanty relaton for an arbtrary state. The states that mnmze t

PHYS 705: Classical Mechanics. Hamilton-Jacobi Equation

Quantum Runge-Lenz Vector and the Hydrogen Atom, the hidden SO(4) symmetry

A how to guide to second quantization method.

Deriving the Dual. Prof. Bennett Math of Data Science 1/13/06

First day August 1, Problems and Solutions

Lectures - Week 4 Matrix norms, Conditioning, Vector Spaces, Linear Independence, Spanning sets and Basis, Null space and Range of a Matrix

763622S ADVANCED QUANTUM MECHANICS Solution Set 1 Spring c n a n. c n 2 = 1.

The Order Relation and Trace Inequalities for. Hermitian Operators

Phys304 Quantum Physics II (2005) Quantum Mechanics Summary. 2. This kind of behaviour can be described in the mathematical language of vectors:

SL n (F ) Equals its Own Derived Group

The Lorentz group. Generate the group SO(3,1) To construct representa;ons a more convenient (non- Hermi;an) basis is. i j ijk k. j ijk k.

Gaussian Conditional Random Field Network for Semantic Segmentation - Supplementary Material

Week3, Chapter 4. Position and Displacement. Motion in Two Dimensions. Instantaneous Velocity. Average Velocity

APPENDIX A Some Linear Algebra

HW #6, due Oct Toy Dirac Model, Wick s theorem, LSZ reduction formula. Consider the following quantum mechanics Lagrangian,

PHYS 705: Classical Mechanics. Canonical Transformation II

Foundations of Arithmetic

MARKOV CHAIN AND HIDDEN MARKOV MODEL

MEM 255 Introduction to Control Systems Review: Basics of Linear Algebra

PHYS 705: Classical Mechanics. Calculus of Variations II

Solution 1 for USTC class Physics of Quantum Information

Convexity preserving interpolation by splines of arbitrary degree

7. Products and matrix elements

Group Theory in Physics

Cyclic Codes BCH Codes

The Dirac Equation for a One-electron atom. In this section we will derive the Dirac equation for a one-electron atom.

Solution 1 for USTC class Physics of Quantum Information

Physics 443, Solutions to PS 7

Monica Purcaru and Nicoleta Aldea. Abstract

where the sums are over the partcle labels. In general H = p2 2m + V s(r ) V j = V nt (jr, r j j) (5) where V s s the sngle-partcle potental and V nt

Modelli Clamfim Equazione del Calore Lezione ottobre 2014

Bezier curves. Michael S. Floater. August 25, These notes provide an introduction to Bezier curves. i=0

The stress functions of the Cosserat continuum

Quantum Mechanics I Problem set No.1

C/CS/Phy191 Problem Set 3 Solutions Out: Oct 1, 2008., where ( 00. ), so the overall state of the system is ) ( ( ( ( 00 ± 11 ), Φ ± = 1

Robert Eisberg Second edition CH 09 Multielectron atoms ground states and x-ray excitations

Chat eld, C. and A.J.Collins, Introduction to multivariate analysis. Chapman & Hall, 1980

Boundary Value Problems. Lecture Objectives. Ch. 27

Modelli Clamfim Equazioni differenziali 22 settembre 2016

12. The Hamilton-Jacobi Equation Michael Fowler

Notes on Analytical Dynamics

Transfer Functions. Convenient representation of a linear, dynamic model. A transfer function (TF) relates one input and one output: ( ) system

Physics 5153 Classical Mechanics. Principle of Virtual Work-1

The Prncpal Component Transform The Prncpal Component Transform s also called Karhunen-Loeve Transform (KLT, Hotellng Transform, oregenvector Transfor

2.3 Nilpotent endomorphisms

LECTURE 9 CANONICAL CORRELATION ANALYSIS

ON AUTOMATIC CONTINUITY OF DERIVATIONS FOR BANACH ALGEBRAS WITH INVOLUTION

This model contains two bonds per unit cell (one along the x-direction and the other along y). So we can rewrite the Hamiltonian as:

Lower bounds for the Crossing Number of the Cartesian Product of a Vertex-transitive Graph with a Cycle

5 The Rational Canonical Form

On the formulation of the laws of Nature with five homogeneous coordinates

PHYS 215C: Quantum Mechanics (Spring 2017) Problem Set 3 Solutions

1 Vectors over the complex numbers

Modelli Clamfim Equazioni differenziali 7 ottobre 2013

Now that we have laws or better postulates we should explore what they imply

The Multiple Classical Linear Regression Model (CLRM): Specification and Assumptions. 1. Introduction

1 (1 + ( )) = 1 8 ( ) = (c) Carrying out the Taylor expansion, in this case, the series truncates at second order:

Linear Approximation with Regularization and Moving Least Squares

THE VIBRATIONS OF MOLECULES II THE CARBON DIOXIDE MOLECULE Student Instructions

Canonical transformations

Difference Equations

Solutions to Exercises in Astrophysical Gas Dynamics

Advanced Circuits Topics - Part 1 by Dr. Colton (Fall 2017)

Physics 5153 Classical Mechanics. D Alembert s Principle and The Lagrangian-1

SOME CHARACTERS OF THE SYMMETRIC GROUP R. E. INGRAM, SJ.

D hh ν. Four-body charm semileptonic decay. Jim Wiss University of Illinois

10. Canonical Transformations Michael Fowler

NP-Completeness : Proofs

Hidden Markov Models & The Multivariate Gaussian (10/26/04)

Generalized Linear Methods

Representation theory and quantum mechanics tutorial Representation theory and quantum conservation laws

Research on Complex Networks Control Based on Fuzzy Integral Sliding Theory

A particle in a state of uniform motion remain in that state of motion unless acted upon by external force.

Transcription:

Note 2 Lng fong L Contents Ken Gordon Equaton. Probabty nterpretaton......................................2 Soutons to Ken-Gordon Equaton............................... 2 2 Drac Equaton 3 2. Probabty nterpretaton..................................... 4 2.2 Souton to Drac equaton................................... 4 2.3 Drac equaton under Lorentz transformaton.......................... 5 Ken Gordon Equaton Casscay, the energy momentum reaton s of the form E = p 2 2m + V (~r) For the quantzaton of ths system, we do the repacement E @ @t, p r and act on a wavefuncton @ @t = [ 2m r2 + V (~r)] Schrodnger equaton Ths equaton does not work for reatvstc system because spata coordnate x and tme t are not on equa footng. In other words, ths s not nvarant under Lorentz transformatons. For reatvstc free partce, we have nstead E 2 = ~p 2 + m 2 The correspondng wave equaton s then Ths s known as Ken-Gordon equaton.. Probabty nterpretaton From Ken-Gordon equaton and ts compex conjugate, we can derve the contnuty equaton, where (r 2 + m 2 ) = @ 2 0 ( + m 2 ) = 0; where = @ 2 0 r 2 = @ @ = @ 2 (@ 2 0 r 2 + m 2 ) = 0 (@ 2 0 r 2 + m 2 ) = 0 @ @t + r j = 0 = ( @ 0 @ 0 ); ~j = ( r r )

Then P = R d 3 x s conserved,.e. dp dt = V @ @t d3 x = V r j d 3 x = I S j ds = 0 f j = 0; on S Snce P s conserved, we woud ke to nterpret t as probabty. However t s easy to see that P s not postve as requred by the de nton of probabty. For exampe, f ~e Et (x) ; then = 2E j (x)j 2 0. e. we get negatve probabty and t s not vabe. On the other hand f we take the probabty densty to be = whch s postve as n the case of Schrodnger equaton, then t s easy to see that t s not conserved, d d 3 x 6= 0 dt Thus t s not possbe to have probabty nterpretaton for Ken-Gordon equaton..2 Soutons to Ken-Gordon Equaton The Ken Gordon equaton ( + m 2 ) (x) = ( r 2 + @ 2 0 + m 2 ) (x) = 0; s a d erenta equaton wth constant coe cents and has pan wave souton, (x) = e px f p 2 0 P 2 m 2 = 0 or p 0 = p ~p 2 + m 2 (a) Postve energy souton: P 0 = p = p ~p 2 + m 2 ; ~p arbtrary (+) (x) = exp p t + p x (b) Negatve energy souton: P 0 = p = p ~p 2 + m 2 ( ) (x) = exp p t p x Note that postve energy soutons (+) (x) togather wth the negatve energy souton ( ) (x) form a compete set of soutons. The most genera souton s a near superposton of postve energy and negatve energy souutons, (x) = = d 3 k p (2) 3 2 k [a(k)e ~ k~x k t + a(k) + e ~ k~x+ k t ] d 3 k p (2) 3 2 k [a(k)e kx + a(k) + e kx ] () where kx = k t ~ k ~x

2 Drac Equaton Drac(928) want to construct a reatvstc wave equaton rst order n tme dervatve just ke Schrodnger equaton whch has conserved probabty and postve. By speca reatvty the wave equaton s aso rst order n spata coordnates. He assume an Ansatz where ; are assumed to be matrces. Then E = p + 2 p 2 + 3 p 3 + m = ~ ~p + m (2) E 2 = ( p + 2 p 2 + 3 p 3 + m) 2 = 2 ( j + j )p p j + 2 p 2 + ( + )m To get reatvstc energy momentum reaton, we requre From Eq( 3) we get j + j = 2 j (3) + = 0 (4) 2 = (5) 2 = (6) Togather wth Eq(5) we see that ; a have egenvaues. Eq( 3) aso mpes Takng the trace Thus Smary, 2 = 2 =) 2 = 2 T r 2 = T r ( 2 ) = T r 2 2 = T r (2 ) T r ( ) = 0 (7) T r () = 0 From Eqs(6,7) we get the mportant resut that ; a have even dmenson. Reca that Pau matrces ; 2 ; 3 are a traceess and ant-commutng. But here we need 4 such matrces. Thus ; a have to be 4 4 matrces. One conveent chocs s that used by Bjoken and Dre where matrces take the form 0 = 0 ; = 0 0 Drac equaton s obtaned from Eq(2) by the repacenments, E @ @t ; ~p r For conveent, de ne a new set of matrces ( ~ r + m) = @ @t ( ~ r @ t + m) = 0 0 = ; = and n Bjorken and Dre notaton, 0 = 0 0 = 0 0 (8)

Drac equaton s then ( @ 0 @ 0 + m) = 0; or ( @ + m) = 0 Ths s usuay referred to as Drac equaton n covarant form. Note that the ant-commutatons are now n a smper form, f ; g = 2g 2. Probabty nterpretaton We can now show that Drac equaton gve a correct form for the peobabty. From the Drac equaton n the hermtan form we get @ y = (f ~ r + m) g) y @t and ( @ y @t Integrate over space, we get d dt + y @ @t ) = y ( ~ r + m) f( ~ r + m) g y d 3 x( y ) = f y (~ r) f(~ r) g y gd 3 x = r y (~ r) d 3 x = 0 The probabty R d 3 x( y ) s conserved and postve. 2.2 Souton to Drac equaton We ook for souton n the pane wave form, (x) = e px u where u and are 2 components coumn vector. Then Drac equaton becomes u ( /p m) = 0 where /p = p Usng the representaton gven n Eq(8), we get m ~ ~p ~ ~p m u u = p 0 (p0 m)u (~ ~p) = 0 (~ ~p)u + (p 0 + m) = 0 (9) These are homogeneous near equatons of u and : Non-trva souton exsts f p 0 m ~ ~p ~ ~p p 0 + m = 0 It s easy to see that ths determnanta condton gves p 2 0 = ~p 2 + m 2 or p 0 = p ~p 2 + m 2

(a) Postve energy souton p 0 = E = p ~p 2 + m 2, Substtute ths nto Eqs(9) we get, We can wrte the souton n the form, = e px u = ~ ~p E + m u = e px N Here s an arbtrary 2 components vector and N s normazaton constant to be determned ater. (b) Negatve energy souton p 0 = E = p ~p 2 + m 2, Smary, the souton can be wrtten as, = e px N The standard notaton for these 4-component coumn vector, spnors are, u(p:s) = N s v(p; s) = e px N s N = p E + m Drac conjugate One of the unua features of Drac equaton n momentum space ( /p m) (p) = 0 s not hermtan. Ths s because n the Hermtan conjugate y (p)( /p y m) = 0 0 s are not hermtan, But we can wrte y 0 = 0 y = y = 0 0 Then y (p)( 0 0 p m) = 0 or y (p) 0 ( p m) = 0 ( /p m) = 0 where = y 0 Drac conjugate 2.3 Drac equaton under Lorentz transformaton Unke the Ken-Gordon equaton whch s nvarant under Lorentz transformaton, Drac equaton s not. We now study how Drac equaton ( @ m) (x) = 0 behaves under Lorentz transformaton x x 0 = x

In the new coordnate system, the Drac equaton s of the form ( @ 0 m) 0 (x 0 ) = 0 (0) Note that we have used the same matrces (In genera, d erent sets of -matrces are reated by smarty transformaton - Pau s theorem). Assume that 0 (x 0 ) and (x) are reated by a near transformaton, 0 (x 0 ) = S (x) We need to nd the operator S: Invert the Lorentz transformaton x = x 0 =) @ @x 0 = @ @x @x @x 0 = @ @x Then Eq(0) becomes ( @ m)s (x) = 0 or ((S S) @ m) (x) = 0 In order for ths equaton to be equvaent to the orgna Drac equaton, we requre (S S) = or (S S) = () To construct S, we consder n ntesma transformaton = g + + O( 2 ) wth j j << Pseudo-othogonaty mpes Wrte S as S = Identfyng coe cent of " ; we get g (g + )(g + ) = g + = 0; =) antsymmetrc 4 + O( 2 ) then S = + 4 : 4 4 matrces. Then Eq() yeds, ( + 4 ) ( It s straghtforward to check that gven by 4 ) = (g + ) 4 [ ; ] = = 2 (g g ) [ ; ] = 2(g g ) (2) = 2 [ ; ] satsfy Eq(2). It s not hard to see that for the nte Lorentz transformaton, we have Note that 0 (x 0 ) = S (x); wth S = exp[ y = 0 0 and S y = 0 S 0 4 ] (3)

Thus S s not untary. From 0 (x 0 ) = S _ we get y 0 (x 0 ) = y S y = y 0 S 0 ; or 0 (x 0 ) = _ (x)s Ths shows that has smpe transformaton property. Fermon bnears Even though the Drac wave functon has rather compcate transformaton under the Lorentz transformaton as shown n Eq(3). The fermon b-nears (x) (x) has rather smpe transformaton. For exampe, 0 (x 0 ) 0 (x 0 ) = (x)s S (x) = (x) (x) Ths means that the combnaton (x) (x) s Lorentz nvarant. Smary, we can work out the other combnaton to get the foowng resuts. 5 5 4-vector axa vector 2nd rank antsymmetrc ensor pseudo scaar where 5 = 0 2 3 Hoe Theory ( Drac 9 ) To sove the probem wth negatve energy states, Drac proposed that the vaccum s the one n whch E < 0 states are a ed and E > 0 states are empty. Then Pau excuson prncpe w prevent an eectron from movng nto E<0 states. In ths pcture hoe n the negatve sea,.e. absence of an eectron wth charge jej wth negatve energy jej s equvaent to a presence of a partce wth energy jej and charge + jej. Ths new partce s caed "postron" and sometme aso caed ant partce. Ths correspondence of partce and ant-partce s caed charge conjugaton: