H&M Chapter 5 Review of Dirac Equation

Similar documents
Physics 214 UCSD/225a UCSB Lecture 11 Finish Halzen & Martin Chapter 4

Lecture 4 - Dirac Spinors

3.3 Lagrangian and symmetries for a spin- 1 2 field

Quantum Physics 2006/07

129 Lecture Notes More on Dirac Equation

3 Quantization of the Dirac equation

11 Spinor solutions and CPT

L = e i `J` i `K` D (1/2,0) (, )=e z /2 (10.253)

Lecture 9/10 (February 19/24, 2014) DIRAC EQUATION(III) i 2. ( x) σ = = Equation 66 is similar to the rotation of two-component Pauli spinor ( ) ( )

Lecture 4 - Relativistic wave equations. Relativistic wave equations must satisfy several general postulates. These are;

Particle Physics WS 2012/13 ( )

Fermi Fields without Tears

Chapter 17 The bilinear covariant fields of the Dirac electron. from my book: Understanding Relativistic Quantum Field Theory.

Lecture 7 From Dirac equation to Feynman diagramms. SS2011: Introduction to Nuclear and Particle Physics, Part 2 2

The Dirac Field. Physics , Quantum Field Theory. October Michael Dine Department of Physics University of California, Santa Cruz

Particle Notes. Ryan D. Reece

Particle Physics Dr M.A. Thomson Part II, Lent Term 2004 HANDOUT V

Particle Physics. Michaelmas Term 2011 Prof. Mark Thomson. Handout 2 : The Dirac Equation. Non-Relativistic QM (Revision)

Particle Physics Dr. Alexander Mitov Handout 2 : The Dirac Equation

1.7 Plane-wave Solutions of the Dirac Equation

x 3 x 1 ix 2 x 1 + ix 2 x 3

As usual, these notes are intended for use by class participants only, and are not for circulation. Week 6: Lectures 11, 12

Quantum Electrodynamics Test

4. The Dirac Equation

7 Quantized Free Dirac Fields

Lecture notes for FYS610 Many particle Quantum Mechanics

Construction of spinors in various dimensions

Introduction to Neutrino Physics. TRAN Minh Tâm

Parity P : x x, t t, (1.116a) Time reversal T : x x, t t. (1.116b)

Relativistic Waves and Quantum Fields

Maxwell s equations. electric field charge density. current density

129 Lecture Notes Relativistic Quantum Mechanics

The Dirac Equation. H. A. Tanaka

Quantum Field Theory

Plan for the rest of the semester. ψ a

Week 3: Renormalizable lagrangians and the Standard model lagrangian 1 Reading material from the books

QM and Angular Momentum

Lecture 10. The Dirac equation. WS2010/11: Introduction to Nuclear and Particle Physics

Representations of Lorentz Group

Attempts at relativistic QM

msqm 2011/8/14 21:35 page 189 #197

THE DIRAC EQUATION (A REVIEW) We will try to find the relativistic wave equation for a particle.

Introduction to Modern Quantum Field Theory

Standard Model of Particle Physics SS 2013

DISCRETE SYMMETRIES IN NUCLEAR AND PARTICLE PHYSICS. Parity PHYS NUCLEAR AND PARTICLE PHYSICS

Phys624 Formalism for interactions Homework 6. Homework 6 Solutions Restriction on interaction Lagrangian. 6.1.

752 Final. April 16, Fadeev Popov Ghosts and Non-Abelian Gauge Fields. Tim Wendler BYU Physics and Astronomy. The standard model Lagrangian

QFT. Unit 1: Relativistic Quantum Mechanics

Standard Model of Particle Physics SS 2012

As usual, these notes are intended for use by class participants only, and are not for circulation. Week 7: Lectures 13, 14.

Quantum Field Theory

Quantum Field Theory

You may not start to read the questions printed on the subsequent pages until instructed to do so by the Invigilator.

Standard Model of Particle Physics SS 2013

Vector Fields. It is standard to define F µν = µ ϕ ν ν ϕ µ, so that the action may be written compactly as

Lorentz-covariant spectrum of single-particle states and their field theory Physics 230A, Spring 2007, Hitoshi Murayama

Physics 214 UCSD Lecture 7 Halzen & Martin Chapter 4

Particle Physics WS 2012/13 ( )

The Dirac equation. L= i ψ(x)[ 1 2 2

Physics 217 FINAL EXAM SOLUTIONS Fall u(p,λ) by any method of your choosing.

LSZ reduction for spin-1/2 particles

REVIEW REVIEW. A guess for a suitable initial state: Similarly, let s consider a final state: Summary of free theory:

Part I. Many-Body Systems and Classical Field Theory

The quantum state as a vector

1 Spinor-Scalar Scattering in Yukawa Theory

Dr Victoria Martin, Spring Semester 2013

MSci EXAMINATION. Date: XX th May, Time: 14:30-17:00

1 Mathematical preliminaries

Outline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification

Physics 221B Spring 2018 Notes 44 Introduction to the Dirac Equation. In 1927 Pauli published a version of the Schrödinger equation for spin- 1 2

Extending the 4 4 Darbyshire Operator Using n-dimensional Dirac Matrices

Quantum Physics II (8.05) Fall 2002 Assignment 3

Lecture 10: A (Brief) Introduction to Group Theory (See Chapter 3.13 in Boas, 3rd Edition)

PRINCIPLES OF PHYSICS. \Hp. Ni Jun TSINGHUA. Physics. From Quantum Field Theory. to Classical Mechanics. World Scientific. Vol.2. Report and Review in

Tutorial 5 Clifford Algebra and so(n)

The Mirror Symmetry of Matter and Antimatter

Neutrino Interactions

The Klein Gordon Equation

Pion Lifetime. A. George January 18, 2012

Relativistic Wave Mechanics

Symmetries, Groups, and Conservation Laws

Spinor Formulation of Relativistic Quantum Mechanics

light-cone (LC) variables

Relativistic Quantum Mechanics

Symmetry Groups conservation law quantum numbers Gauge symmetries local bosons mediate the interaction Group Abelian Product of Groups simple

Dirac equation. Victor Kärcher. 07th of January Contents. 1 Introduction 2. 2 Relativistic theory of the electron 2

Disclaimer. [disclaimer]

PHY 396 K. Solutions for homework set #9.

Particle Physics I Lecture Exam Question Sheet

2.4 Parity transformation

Physics 582, Problem Set 1 Solutions

Mechanics Physics 151

221B Lecture Notes Quantum Field Theory II (Fermi Systems)

Repeated Eigenvalues and Symmetric Matrices

PARTICLE PHYSICS Major Option

Free totally (anti)symmetric massless fermionic fields in d-dimensional anti-de Sitter space

Electroweak Physics. Krishna S. Kumar. University of Massachusetts, Amherst

Introduction to particle physics Lecture 12: Weak interactions

Review and Notation (Special relativity)

The Lorentz and Poincaré Groups in Relativistic Field Theory

Transcription:

HM Chapter 5 Review of Dirac Equation Dirac s Quandary Notation Reminder Dirac Equation for free particle Mostly an exercise in notation Define currents Make a complete list of all possible currents Aside on Helicity Operator Solutions to free particle Dirac equation are eigenstates of Helicity Operator Aside on handedness

Dirac s Quandary Can there be a formalism that allows wave functions that satisfy the linear and quadratic equations simultaneously: H =(~ ~p + m H 2 =(~p ~p + m 2 If such a thing existed then the linear equation would provide us with energy eigenvalues that automatically satisfy the relativistic energy momentum relationship

Dirac s Quandary (2 Such a thing does indeed exist: Wave function is a 4 component object α i = # $ σ i σ i # β = I $ I ( ( α is thus a 3-vector of 4x4 matrices with special commutator relationships like the Pauli matrices. While β is a diagonal 4x4 matrix as shown. # σ = # (; σ $ 2 = i # (; σ $ i 3 = # (; I = ( $ $

The rest is history In the following I provide a very limited reminder of notation and a few facts. If these things don t sound familiar, then I encourage you to work through ch. 5 carefully.

Rewrite a little: H =(~ ~p + m H =( ~ ~p + 2 m =( ~ ~p + m ( H ~ ~p = m Now it looks covariant: ( p ~ ~p = m µ p µ = m p = m Where we have introduced: p µ =(H, ~p =, 5 i = i and for later use: 5 = i 2 3

They satisfy: { µ, } =2 µ In particular: ( 2 =, ( 2 =( 2 2 =( 3 2 = So they cannot be hermitian. In fact ( =, ( i = i Also: { 5, µ } =, ( 5 2 =, ( 5 = 5 6

Notation Reminder ( Sigma Matrices: # σ = # (; σ $ 2 = i # (; σ $ i 3 = # (; I = ( $ $ Gamma Matrices: $ γ = I $ σ ; γ j =,2,3 j =,2,3 $ = ; γ 5 = I I( σ j =,2,3 ( I ( State Vectors: #. (. ψ = (; ψ ψ T γ =.....( ( $. (

Notation Reminder (2 Obvious statements about gamma matrices γ ( j =,2,5T = γ ( j =,2,5 ; γ ( j =,3T = γ ( j =,3 γ ( j =,5T = γ ( j =,5 ; γ ( j =,2,3T = γ ( j =,2,3 Probability density ψ ψ T γ Scalar product of gamma matrix and 4-vector ψγ ψ =ψ T ψ =# /A µ A µ = A A 2 A 2 3 A 3 Is again a scalar formed from a 4-vector

Dirac Equation of free particle (i/@ m = i@ µ µ + m = Ansatz: = e ip x u(p or (i /@ + m = Explore this in restframe of particle: ψ + 2 = 2me imt $ $ ; ψ 2 = 2me imt ; ( ( Normalization chosen to describe 2E particles, as usual.

Particle vs antiparticle in restframe ψ + 2 = 2me imt $ $ ; ψ 2 = 2me imt ; ( ( Recall, particle antiparticle means E,p E, p Let s take a look at Energy Eigenvalues: particle " # $ mi mi u = Eu for p = we get this equation to satisfy by the energy eigenvectors It is thus obvious that 2 of the solutions have E <, and are the lower two components of the 4-component object u.

Particle Anti-particle ψ + 2 = 2me imt $ ( ; ψ 2 = 2me imt $ ( ; ψ + 2 = 2me imt $ ( ; ψ 2 = 2me imt $ ( ; Negative energy solution Positive energy solution

Not in restframe this becomes: The lower 2 components are thus coupled to the upper 2 via this matrix equation, leading to free particle and antiparticle solutions as follows.

(Anti-Particle not in restframe ψ + 2 = Ne ipx σ p E + m ( ( ; ψ 2 = Ne ipx σ p E + m ( ( ψ + 2 = Ne +ipx σ p E +m ( ( ; ψ 2 = Ne +ipx σ p E +m ( ( I suggest you read up on this in HM chapter 5 if you re not completely comfortable with it.

What we learned so far: Dirac Equation has 4 solutions for the same p: Two with E > Two with E < The E < solutions describe anti-particles. The additional 2-fold ambiguity describes spin ±/2. You will show this explicitly in Exercise HM 5.4, which is part of HW next week. We thus have a formalism to describe all the fundamental spin-/2 particles in nature.

Helicity Operator The helicity operator commutes with both H and P. Helicity is thus conserved for the free spin-/2 particle. The unit vector here is the axis with regard to which we define the helicity. For (,,, i.e., the z-axis, we get the desired ±/2 eigenvalues. # σ 3 = $ (

Dirac Equation for particle and anti-particle spinors It s sometimes notationally convenient to write the antiparticle spinor solution (i.e. the p, E as e ip x u (,2 (p an explicit antiparticle spinor that satisfies a modified Dirac equation: e i( p x u (3,4 ( p =e ip x v (,2 (p ( γ µ p µ mu = ( γ µ p µ + mv = particle antiparticle The v-spinor then has positive energy. We won t be using v-spinors in this course. HM Equation (5.33 and (5.34

Antiparticles We will stick to the antiparticle description we introduced in chapter 4: e - e - p,e -p,-e Initial state e + e - is an initial state e - e - with the positron being an electron going in the wrong direction, i.e. backwards in time.

Some more reflections on γ µ There are exactly 5 distinct γ matrices: $ γ = I $ σ ; γ j =,2,3 j =,2,3 $ = ; γ 5 = I I( σ j =,2,3 ( I ( γ 5 iγ γ γ 2 γ 3 Where Every one of them multiplied with itself gives the unit matrix. As a result, any product of 5 of them can be expressed as a product of 3 of them.

Currents Any bi-linear quantity can be a current as long as it has the most general form: ψ( 4x4ψ By finding all possible forms of this type, using the gamma-matrices as a guide, we can form all possible currents that can be within this formalism.

The possible currents ψψ ψγ 5 ψ ψγ µ ψ ψγ 5 γ µ ψ scalar pseudo-scalar vector pseudo-vector or axial-vector ψ i ( 2 γ µ γ ν γ ν γ µ ψ tensor Note: we define µ = i 2 ( µ µ

Electromagnetic Interactions Minimal substitution i@ µ! i@ µ + ea µ id µ Dirac: (i/@ m =! (i /D m = (i/@ + e /A m = (electron Had we started with positron we would have (i/@ e /A m C = 2

There must be a correspondence: complex conjugate the first (i/@ + e /A m = ( i µ @ µ + e µ A µ m = multiply by a matrix D D( i µ @ µ + e µ A µ md D = such that D µ D = µ and define C = D So that (i/@ e /A m C = It is convenient to define D = C, C = D so that C = C T and C = T C 22

EM-Current We have seen the vector: µ It is conserved: @ µ ( µ = (/@ + /@ = i (m mµ = and = = > has the interpretation of a density. For it to be a charge density of electrons, multiply by e j µ = e µ =(,~j j µ C = e C µ C = e T C µ C T = e T ( µ T T = e µ = j µ A Cµ j µ C =( A µ( j µ =A µ J µ EM is invariant under charge conjugation 23

Massless spin-/2: 2-component spinors H =(~ ~p + m need only α matrices { i, j } =2 ij i = i may take i = ± i (Pauli Massless Dirac: two decoupled equations for 2-component spinors E = ~ ~p E =+~ ~p Helicity: divide through by E = ~p 2 ~ ˆp = 2 2 ~ ˆp =+ 2 helicity = 2 =+ 2 invariant under boosts (since massless particles travel at speed of light 24

But we can also have solutions with negative energy E = ~p pz E = ~ ~p with, e.g., p along z-axis: E = p z Take 2 2 Negative energy: antiparticle. Use E, p in Feynman rules for anti-particle of energy/momentum +E,+p. So for negative energy solution 2 ~ ˆp =+ 2 helicity =+ 2 Particle is left-handed, L its anti-particle is right handed, R Parity(P: L R, so theory with only one type of 2-component spinor breaks P OK for weak interactions! 25

Weyl representation 2-component in 4-component notation: u =, i = i i corresponds to i = i i, I =, I 5 I =. I Projection operator 2 ( 5 u = I = projection operator: ( 2 ( 5 2 = 2 ( 5 26

Peak ahead into weak interactions There is a charged current, coupling electron to neutrino J µ = e µ 2 ( 5 and the hermitian conjugate J µ = 2 ( 5 µ e This is called a V A current, a vector minus a pseudo-vector (or axial vector 27