Quantum Physics 2006/07

Size: px
Start display at page:

Download "Quantum Physics 2006/07"

Transcription

1 Quantum Physics 6/7 Lecture 7: More on the Dirac Equation In the last lecture we showed that the Dirac equation for a free particle i h t ψr, t = i hc α + β mc ψr, t has plane wave solutions ψr, t = exp ip x/ h wp if the 4-component column vector wp, or 4-component Dirac spinor, satisfies the momentum- or p-space Dirac equation and p = ± { m c + p } /. p wp = α p + βmc wp Two-by-two block form of the Dirac equation The p-space Dirac equation can be solved for wp by brute force, but we shall introduce a more elegant formalism by writing the four-component spinor wp in terms of two twocomponent spinors φ and χ: φ w = χ The p-space Dirac equation, for plane wave solutions becomes φ p = mc σ p φ χ σ p mc χ Note that the elements of the block matrix are themselves matrices. More explicitly p φ = mc φ + σ p χ p χ = σ p φ mc χ 4 Positive energy solutions: Let us first choose p >, ie p = + m c + p / p + = E c E > Equation 4 can be used to solve for χ in terms of φ χ = which we can substitute back into equation to obtain } p σ p φ = {mc + φ p + mc σ p p + mc φ 5 but σ p = p exercise, therefore wp is a free particle solution of the Dirac equation for all two-component spinors φ if p + p mc = p mc + mc + p

2 which reduces to the usual relation between energy & momentum. Therefore, the two positive-energy plane-wave solutions can be written as φ, w, p = c σ p φ, It is conventional to choose the two linearly-independent two-spinors φ = and φ = Negative energy solutions: Now choose p <, ie p = m c + p / p = E c E > It is conventional to write down the two negative energy solutions with spatial momenta p, ie with p µ = p, p. By solving equation for φ in terms of χ we obtain exercise: c σ p χ, w,4 p = χ, For the negative energy solutions, it is conventional to choose the two linearly-independent two-spinors χ = and χ = The reason for the apparently perverse choice of negative momenta and two-spinors should become clearer when we interpret the negative energy states. Summary: With the above conventions, the two positive energy solutions with four momenta p µ + = E/c, p have components w cp p = and w cp p = ip cp + ip cp The two negative energy solutions with spatial momenta p, ie with p µ = E/c, p, have components cp ip cp w cp p = and w 4 cp p = + ip Note: The quantity E > in all equations above. Unfortunately, conventions in labelling the w i differ widely.

3 Rest-frame solutions, spin and angular momentum: w = w = w = When p = we have w 4 = and the positive-energy solutions are simply ψ = exp imc t/ h and ψ = exp imc t/ h These are degenerate in energy. Therefore, by the compatibility theorem, there must be another operator which commutes with the Hamiltonian for p = and whose eigenvalues label the states. One such operator is Σ σ σ = The rest-frame four-component spinors w i are eigenvectors of Σ with eigenvalues ±. The appearance of the Pauli spin matrix σ suggests that we interpret the Dirac equation as describing a spin / particle. If we introduce the three 4 4 matrices Then and Σ i σ i σ i h Σ h Σ Σ has h or, in vector notation Σ = 4 h ˆ = ss + h ˆ with s = eigenvalues ± h σ σ ŝ = h Σ ie we interpret as the spin operator for the Dirac theory the Dirac particle necessarily hσ has an intrinsic spin which is not related to ordinary orbital angular momentum. However, Σ does not commute with the hamiltonian cα ˆp + βmc in any frame other than the rest frame, p =, so the expectation value of Σ is not a conserved quanity. Also, the operator ˆL = ˆr ˆp does not commute with the Hamiltonian in any frame other than the rest frame, so orbital angular momentum isn t a conserved quantity either. However, the operator Ĵ = ˆL + h Σ commutes with the Hamiltonian in all frames, suggesting that it may be interpreted as the operator for the total angular momentum, and this is conserved tutorial. Helicity: As we have seen, there are two independent states for any given four-momentum. A different p-space operator which commutes with cα p + βmc, and which can be used

4 to label the states is the helicity operator ĥp = σ p p which has eigenvalues ±. Therefore, general plane wave states with p can be chosen to be helicity eigenstates. Of course, it still remains to interpret the negative energy states! σ p p Interpreting the negative energy solutions As we saw, the plane wave solutions of the Dirac equation satisfy the energy-momentum relation E = ± p c + m c 4 therefore either E mc or E mc ie there is a continuum of positive energy states starting at E = mc and a continuum of negative energy states going down from E = mc. Since the Dirac equation appears to describe spin-half particles, let s assume these particles are electrons, and let s take the negative energy solutions seriously. The problem we must address is the following: What is to prevent a positive energy electron from making transitions under the influence of a perturbation to negative energy states? A solution to this problem was suggested by Dirac in 9. cp +mc O mc The Dirac Sea: Taking the negative energy states seriously, Dirac proposed that all negative energy states are filled, each energy level holding two electrons with opposite spins. Since electrons are fermions, he then evoked the Pauli exclusion principle to prevent any transition of a positive energy electron to a negative energy state! In this picture the vacuum is an infinite sea of negative energy electrons the Dirac sea. He then argued that the infinite negative energy and infinite negative charge of this vacuum, are unobservable we only measure finite changes of charge and energy relative to this vacuum. 4

5 cp +mc O mc Particle Hole Radiation +E E Pair Production: One important consequence of this picture is that we can excite a negative energy particle from the sea into a positive energy state. Suppose an electron in the sea absorbs photons with sufficient energy > mc to make a transition to a state in the positive energy continuum. What we will observe is an electron of charge e and energy +E, say, together with a hole in the sea. The hole which is the absence of an electron with charge e and energy E would be interpreted by an observer as a particle of charge +e and energy +E, in other words as a positive energy anti-particle or positron. Furthermore, the threshold for this process is just mc, the size of the gap in the energy eigenvalue spectrum, and we have arrived at a description of electron-positron pair production. Thus Dirac predicted the existence of antiparticles. Although we started with a single-particle wave equation, the Dirac theory forces us into a many-particle interpretation. The positron was discovered four years later, thus confirming Dirac s prediction. The absence of a negative energy particle with spin up in its rest-frame is equivalent to the presence of a positive-energy particle with spin down. This explains the apparently perverse choice of negative-momentum solutions and two-component spinors we made on page. The full solution requires Relativistic Quantum Field Theory RQFT, the subject of a fifth-year course. The Dirac sea picture doesn t work for bosons. There is no Pauli principle, therefore nothing can seemingly stop the positive energy particles decaying into oblivion. This is one of the reasons that lead Dirac to discard the Klein-Gordon equation for spinless particles. However, it turns out that there is no such problem in RQFT. Covariant form of the Dirac equation non-examinable In most advanced applications of the Dirac equation, a covariant notation is used. Anyone taking RQFT next year is advised to become familiar with it now. Defining the natural system of units, h = c =, the Dirac equation for a free particle is i ψr, t = i α + β m ψr, t t At least two photons must be absorbed to conserve 4-momentum. 5

6 If we multiply by β: and introduce the matrices iβ ψr, t = i β α + m ψr, t 6 t γ β γ i β α i then we may rewrite equation 6 as { i γ x + γi x i where x = x µ µ =,,. More compactly, m } iγ µ µ m ψx = or i/ m ψx = where we have introduced the Feynman slash notation: pronounced a-slash. Similarly, / is d-slash. /a γ µ a µ = γ µ a µ ψx = Positive energy plane-wave solutions of the type ψx = exp ip x up thus satisfy γ µ p µ m up /p m up = whilst negative energy negative four-momentum solutions ψx = exp+ip x v p satisfy γ µ p µ + m v p /p + m v p = It is easy to verify that the gamma matrices satisfy the anticommutation relations known as the Clifford algebra γ µ γ ν + γ ν γ µ {γ µ, γ ν } = g µν In the standard representation of α and β σ γ i i = σ i and γ = so that γ is hermitian γ = γ, the γ i are anti-hermitian γ i = γ i, thus γ = and γ i =. It is also convenient to work with where ψ is pronounced psi-bar. ψ ψ γ and similarly u u γ The new notation treats space and time on an even more equal basis, and is known as the covariant formulation. One can derive the properties of the Dirac wave-function ψx under Lorentz boosts and use them to prove explicitly that the conserved current j µ ψ ψ, ψ α ψ = ψγ µ ψ does indeed transform as a 4-vector under Lorentz transformations. Similarly, one can show that the quantity ψψ is invariant under Lorentz transformations, ie it s a Lorentz scalar. 6

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

Particle Physics. Michaelmas Term 2011 Prof. Mark Thomson. Handout 2 : The Dirac Equation. Non-Relativistic QM (Revision) Particle Physics Michaelmas Term 2011 Prof. Mark Thomson + e - e + - + e - e + - + e - e + - + e - e + - Handout 2 : The Dirac Equation Prof. M.A. Thomson Michaelmas 2011 45 Non-Relativistic QM (Revision)

More information

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

Particle Physics Dr. Alexander Mitov Handout 2 : The Dirac Equation Dr. A. Mitov Particle Physics 45 Particle Physics Dr. Alexander Mitov µ + e - e + µ - µ + e - e + µ - µ + e - e + µ - µ + e - e + µ - Handout 2 : The Dirac Equation Dr. A. Mitov Particle Physics 46 Non-Relativistic

More information

Quantum Field Theory

Quantum Field Theory Quantum Field Theory PHYS-P 621 Radovan Dermisek, Indiana University Notes based on: M. Srednicki, Quantum Field Theory 1 Attempts at relativistic QM based on S-1 A proper description of particle physics

More information

Attempts at relativistic QM

Attempts at relativistic QM Attempts at relativistic QM based on S-1 A proper description of particle physics should incorporate both quantum mechanics and special relativity. However historically combining quantum mechanics and

More information

H&M Chapter 5 Review of Dirac Equation

H&M Chapter 5 Review of Dirac Equation 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

More information

Lecture 4 - Dirac Spinors

Lecture 4 - Dirac Spinors Lecture 4 - Dirac Spinors Schrödinger & Klein-Gordon Equations Dirac Equation Gamma & Pauli spin matrices Solutions of Dirac Equation Fermion & Antifermion states Left and Right-handedness Non-Relativistic

More information

3 Quantization of the Dirac equation

3 Quantization of the Dirac equation 3 Quantization of the Dirac equation 3.1 Identical particles As is well known, quantum mechanics implies that no measurement can be performed to distinguish particles in the same quantum state. Elementary

More information

Quantum Field Theory

Quantum Field Theory Quantum Field Theory PHYS-P 621 Radovan Dermisek, Indiana University Notes based on: M. Srednicki, Quantum Field Theory 1 Attempts at relativistic QM based on S-1 A proper description of particle physics

More information

Quantum Field Theory

Quantum Field Theory Quantum Field Theory PHYS-P 621 Radovan Dermisek, Indiana University Notes based on: M. Srednicki, Quantum Field Theory 1 Attempts at relativistic QM based on S-1 A proper description of particle physics

More information

3.3 Lagrangian and symmetries for a spin- 1 2 field

3.3 Lagrangian and symmetries for a spin- 1 2 field 3.3 Lagrangian and symmetries for a spin- 1 2 field The Lagrangian for the free spin- 1 2 field is The corresponding Hamiltonian density is L = ψ(i/ µ m)ψ. (3.31) H = ψ( γ p + m)ψ. (3.32) The Lagrangian

More information

The Dirac Equation. H. A. Tanaka

The Dirac Equation. H. A. Tanaka The Dirac Equation H. A. Tanaka Relativistic Wave Equations: In non-relativistic quantum mechanics, we have the Schrödinger Equation: H = i t H = p2 2m 2 = i 2m 2 p t i Inspired by this, Klein and Gordon

More information

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

Lecture 7 From Dirac equation to Feynman diagramms. SS2011: Introduction to Nuclear and Particle Physics, Part 2 2 Lecture 7 From Dirac equation to Feynman diagramms SS2011: Introduction to Nuclear and Particle Physics, Part 2 2 1 Dirac equation* The Dirac equation - the wave-equation for free relativistic fermions

More information

Particle Notes. Ryan D. Reece

Particle Notes. Ryan D. Reece Particle Notes Ryan D. Reece July 9, 2007 Chapter 1 Preliminaries 1.1 Overview of Special Relativity 1.1.1 Lorentz Boosts Searches in the later part 19th century for the coordinate transformation that

More information

129 Lecture Notes More on Dirac Equation

129 Lecture Notes More on Dirac Equation 19 Lecture Notes More on Dirac Equation 1 Ultra-relativistic Limit We have solved the Diraction in the Lecture Notes on Relativistic Quantum Mechanics, and saw that the upper lower two components are large

More information

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 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 ( ) ( ) P47 For a Lorentz boost along the x-axis, Lecture 9/ (February 9/4, 4) DIRAC EQUATION(III) i ψ ωσ ψ ω exp α ψ ( x) ( x ) exp ( x) (65) where tanh ω β, cosh ω γ, sinh ω βγ β imilarly, for a rotation around

More information

G : Quantum Mechanics II

G : Quantum Mechanics II G5.666: Quantum Mechanics II Notes for Lecture 5 I. REPRESENTING STATES IN THE FULL HILBERT SPACE Given a representation of the states that span the spin Hilbert space, we now need to consider the problem

More information

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

Lecture 4 - Relativistic wave equations. Relativistic wave equations must satisfy several general postulates. These are; Lecture 4 - Relativistic wave equations Postulates Relativistic wave equations must satisfy several general postulates. These are;. The equation is developed for a field amplitude function, ψ 2. The normal

More information

QFT. Unit 1: Relativistic Quantum Mechanics

QFT. Unit 1: Relativistic Quantum Mechanics QFT Unit 1: Relativistic Quantum Mechanics What s QFT? Relativity deals with things that are fast Quantum mechanics deals with things that are small QFT deals with things that are both small and fast What

More information

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

Lecture 10. The Dirac equation. WS2010/11: Introduction to Nuclear and Particle Physics Lecture 10 The Dirac equation WS2010/11: Introduction to Nuclear and Particle Physics The Dirac equation The Dirac equation is a relativistic quantum mechanical wave equation formulated by British physicist

More information

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

The Dirac Field. Physics , Quantum Field Theory. October Michael Dine Department of Physics University of California, Santa Cruz Michael Dine Department of Physics University of California, Santa Cruz October 2013 Lorentz Transformation Properties of the Dirac Field First, rotations. In ordinary quantum mechanics, ψ σ i ψ (1) is

More information

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

Physics 214 UCSD/225a UCSB Lecture 11 Finish Halzen & Martin Chapter 4 Physics 24 UCSD/225a UCSB Lecture Finish Halzen Martin Chapter 4 origin of the propagator Halzen Martin Chapter 5 Continue Review of Dirac Equation Halzen Martin Chapter 6 start with it if time permits

More information

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

Extending the 4 4 Darbyshire Operator Using n-dimensional Dirac Matrices International Journal of Applied Mathematics and Theoretical Physics 2015; 1(3): 19-23 Published online February 19, 2016 (http://www.sciencepublishinggroup.com/j/ijamtp) doi: 10.11648/j.ijamtp.20150103.11

More information

Units and dimensions

Units and dimensions Particles and Fields Particles and Antiparticles Bosons and Fermions Interactions and cross sections The Standard Model Beyond the Standard Model Neutrinos and their oscillations Particle Hierarchy Everyday

More information

2.4 Parity transformation

2.4 Parity transformation 2.4 Parity transformation An extremely simple group is one that has only two elements: {e, P }. Obviously, P 1 = P, so P 2 = e, with e represented by the unit n n matrix in an n- dimensional representation.

More information

7 Quantized Free Dirac Fields

7 Quantized Free Dirac Fields 7 Quantized Free Dirac Fields 7.1 The Dirac Equation and Quantum Field Theory The Dirac equation is a relativistic wave equation which describes the quantum dynamics of spinors. We will see in this section

More information

ΑΒΓΔΕΖΗΘΙΚΛΜΝΞΟΠΡΣΤΥΦΧΨΩ αβγδεζηθικλμνξοπρςστυφχψω +<=>± ħ

ΑΒΓΔΕΖΗΘΙΚΛΜΝΞΟΠΡΣΤΥΦΧΨΩ αβγδεζηθικλμνξοπρςστυφχψω +<=>± ħ CHAPTER 1. SECOND QUANTIZATION In Chapter 1, F&W explain the basic theory: Review of Section 1: H = ij c i < i T j > c j + ij kl c i c j < ij V kl > c l c k for fermions / for bosons [ c i, c j ] = [ c

More information

11 Spinor solutions and CPT

11 Spinor solutions and CPT 11 Spinor solutions and CPT 184 In the previous chapter, we cataloged the irreducible representations of the Lorentz group O(1, 3. We found that in addition to the obvious tensor representations, φ, A

More information

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

Parity P : x x, t t, (1.116a) Time reversal T : x x, t t. (1.116b) 4 Version of February 4, 005 CHAPTER. DIRAC EQUATION (0, 0) is a scalar. (/, 0) is a left-handed spinor. (0, /) is a right-handed spinor. (/, /) is a vector. Before discussing spinors in detail, let us

More information

Introduction to Modern Quantum Field Theory

Introduction to Modern Quantum Field Theory Department of Mathematics University of Texas at Arlington Arlington, TX USA Febuary, 2016 Recall Einstein s famous equation, E 2 = (Mc 2 ) 2 + (c p) 2, where c is the speed of light, M is the classical

More information

Quantum Electrodynamics Test

Quantum Electrodynamics Test MSc in Quantum Fields and Fundamental Forces Quantum Electrodynamics Test Monday, 11th January 2010 Please answer all three questions. All questions are worth 20 marks. Use a separate booklet for each

More information

Geometry and Physics. Amer Iqbal. March 4, 2010

Geometry and Physics. Amer Iqbal. March 4, 2010 March 4, 2010 Many uses of Mathematics in Physics The language of the physical world is mathematics. Quantitative understanding of the world around us requires the precise language of mathematics. Symmetries

More information

129 Lecture Notes Relativistic Quantum Mechanics

129 Lecture Notes Relativistic Quantum Mechanics 19 Lecture Notes Relativistic Quantum Mechanics 1 Need for Relativistic Quantum Mechanics The interaction of matter and radiation field based on the Hamitonian H = p e c A m Ze r + d x 1 8π E + B. 1 Coulomb

More information

4. The Standard Model

4. The Standard Model 4. The Standard Model Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 4. The Standard Model 1 In this section... Standard Model particle content Klein-Gordon equation Antimatter Interaction

More information

The Dirac Equation. Topic 3 Spinors, Fermion Fields, Dirac Fields Lecture 13

The Dirac Equation. Topic 3 Spinors, Fermion Fields, Dirac Fields Lecture 13 The Dirac Equation Dirac s discovery of a relativistic wave equation for the electron was published in 1928 soon after the concept of intrisic spin angular momentum was proposed by Goudsmit and Uhlenbeck

More information

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

MSci EXAMINATION. Date: XX th May, Time: 14:30-17:00 MSci EXAMINATION PHY-415 (MSci 4242 Relativistic Waves and Quantum Fields Time Allowed: 2 hours 30 minutes Date: XX th May, 2010 Time: 14:30-17:00 Instructions: Answer THREE QUESTIONS only. Each question

More information

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

As usual, these notes are intended for use by class participants only, and are not for circulation. Week 6: Lectures 11, 12 As usual, these notes are intended for use by class participants only, and are not for circulation Week 6: Lectures, The Dirac equation and algebra March 5, 0 The Lagrange density for the Dirac equation

More information

Particle Physics I Lecture Exam Question Sheet

Particle Physics I Lecture Exam Question Sheet Particle Physics I Lecture Exam Question Sheet Five out of these 16 questions will be given to you at the beginning of the exam. (1) (a) Which are the different fundamental interactions that exist in Nature?

More information

Paris Samuel Miles-Brenden. June 23, 2017

Paris Samuel Miles-Brenden. June 23, 2017 Symmetry of Covariance & Exchange: Particle, Field Theory & The Two Body Equation Paris Samuel Miles-Brenden June 23, 2017 Introduction The interior and effective representational algebra of the raising

More information

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

You may not start to read the questions printed on the subsequent pages until instructed to do so by the Invigilator. MATHEMATICAL TRIPOS Part III Monday 7 June, 004 1.30 to 4.30 PAPER 48 THE STANDARD MODEL Attempt THREE questions. There are four questions in total. The questions carry equal weight. You may not start

More information

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

PRINCIPLES OF PHYSICS. \Hp. Ni Jun TSINGHUA. Physics. From Quantum Field Theory. to Classical Mechanics. World Scientific. Vol.2. Report and Review in LONDON BEIJING HONG TSINGHUA Report and Review in Physics Vol2 PRINCIPLES OF PHYSICS From Quantum Field Theory to Classical Mechanics Ni Jun Tsinghua University, China NEW JERSEY \Hp SINGAPORE World Scientific

More information

The Klein-Gordon equation

The Klein-Gordon equation Lecture 8 The Klein-Gordon equation WS2010/11: Introduction to Nuclear and Particle Physics The bosons in field theory Bosons with spin 0 scalar (or pseudo-scalar) meson fields canonical field quantization

More information

Lecture notes for FYS610 Many particle Quantum Mechanics

Lecture notes for FYS610 Many particle Quantum Mechanics UNIVERSITETET I STAVANGER Institutt for matematikk og naturvitenskap Lecture notes for FYS610 Many particle Quantum Mechanics Note 20, 19.4 2017 Additions and comments to Quantum Field Theory and the Standard

More information

d 3 r d 3 vf( r, v) = N (2) = CV C = n where n N/V is the total number of molecules per unit volume. Hence e βmv2 /2 d 3 rd 3 v (5)

d 3 r d 3 vf( r, v) = N (2) = CV C = n where n N/V is the total number of molecules per unit volume. Hence e βmv2 /2 d 3 rd 3 v (5) LECTURE 12 Maxwell Velocity Distribution Suppose we have a dilute gas of molecules, each with mass m. If the gas is dilute enough, we can ignore the interactions between the molecules and the energy will

More information

Relativistic Quantum Mechanics

Relativistic Quantum Mechanics Physics 342 Lecture 34 Relativistic Quantum Mechanics Lecture 34 Physics 342 Quantum Mechanics I Wednesday, April 30th, 2008 We know that the Schrödinger equation logically replaces Newton s second law

More information

PHY 396 K. Solutions for homework set #9.

PHY 396 K. Solutions for homework set #9. PHY 396 K. Solutions for homework set #9. Problem 2(a): The γ 0 matrix commutes with itself but anticommutes with the space-indexed γ 1,2,3. At the same time, the parity reflects the space coordinates

More information

Dr Victoria Martin, Spring Semester 2013

Dr Victoria Martin, Spring Semester 2013 Particle Physics Dr Victoria Martin, Spring Semester 2013 Lecture 3: Feynman Diagrams, Decays and Scattering Feynman Diagrams continued Decays, Scattering and Fermi s Golden Rule Anti-matter? 1 Notation

More information

Relativistic quantum mechanics

Relativistic quantum mechanics Chapter 6 Relativistic quantum mechanics The Schrödinger equation for a free particle in the coordinate representation, i Ψ t = 2 2m 2 Ψ, is manifestly not Lorentz constant since time and space derivatives

More information

Tutorial 5 Clifford Algebra and so(n)

Tutorial 5 Clifford Algebra and so(n) Tutorial 5 Clifford Algebra and so(n) 1 Definition of Clifford Algebra A set of N Hermitian matrices γ 1, γ,..., γ N obeying the anti-commutator γ i, γ j } = δ ij I (1) is the basis for an algebra called

More information

Maxwell s equations. electric field charge density. current density

Maxwell s equations. electric field charge density. current density Maxwell s equations based on S-54 Our next task is to find a quantum field theory description of spin-1 particles, e.g. photons. Classical electrodynamics is governed by Maxwell s equations: electric field

More information

Relativistic Waves and Quantum Fields

Relativistic Waves and Quantum Fields Relativistic Waves and Quantum Fields (SPA7018U & SPA7018P) Gabriele Travaglini December 10, 2014 1 Lorentz group Lectures 1 3. Galileo s principle of Relativity. Einstein s principle. Events. Invariant

More information

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

THE DIRAC EQUATION (A REVIEW) We will try to find the relativistic wave equation for a particle. THE DIRAC EQUATION (A REVIEW) We will try to find the relativistic wave equation for a particle. First, we introduce four dimensional notation for a vector by writing x µ = (x, x 1, x 2, x 3 ) = (ct, x,

More information

Quantum Physics II (8.05) Fall 2002 Assignment 12 and Study Aid

Quantum Physics II (8.05) Fall 2002 Assignment 12 and Study Aid Quantum Physics II (8.05) Fall 2002 Assignment 12 and Study Aid Announcement This handout includes 9 problems. The first 5 are the problem set due. The last 4 cover material from the final few lectures

More information

Introduction to particle physics Lecture 2

Introduction to particle physics Lecture 2 Introduction to particle physics Lecture 2 Frank Krauss IPPP Durham U Durham, Epiphany term 2009 Outline 1 Quantum field theory Relativistic quantum mechanics Merging special relativity and quantum mechanics

More information

Introduction to Quantum Mechanics PVK - Solutions. Nicolas Lanzetti

Introduction to Quantum Mechanics PVK - Solutions. Nicolas Lanzetti Introduction to Quantum Mechanics PVK - Solutions Nicolas Lanzetti lnicolas@student.ethz.ch 1 Contents 1 The Wave Function and the Schrödinger Equation 3 1.1 Quick Checks......................................

More information

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

L = e i `J` i `K` D (1/2,0) (, )=e z /2 (10.253) 44 Group Theory The matrix D (/,) that represents the Lorentz transformation (.4) L = e i `J` i `K` (.5) is D (/,) (, )=exp( i / /). (.5) And so the generic D (/,) matrix is D (/,) (, )=e z / (.53) with

More information

Lecture 11 Spin, orbital, and total angular momentum Mechanics. 1 Very brief background. 2 General properties of angular momentum operators

Lecture 11 Spin, orbital, and total angular momentum Mechanics. 1 Very brief background. 2 General properties of angular momentum operators Lecture Spin, orbital, and total angular momentum 70.00 Mechanics Very brief background MATH-GA In 9, a famous experiment conducted by Otto Stern and Walther Gerlach, involving particles subject to a nonuniform

More information

lattice QCD and the hadron spectrum Jozef Dudek ODU/JLab

lattice QCD and the hadron spectrum Jozef Dudek ODU/JLab lattice QCD and the hadron spectrum Jozef Dudek ODU/JLab a black box? QCD lattice QCD observables (scattering amplitudes?) in these lectures, hope to give you a look inside the box 2 these lectures how

More information

β matrices defined above in terms of these Pauli matrices as

β matrices defined above in terms of these Pauli matrices as The Pauli Hamiltonian First let s define a set of x matrices called the Pauli spin matrices; i σ ; ; x σ y σ i z And note for future reference that σ x σ y σ z σ σ x + σ y + σ z 3 3 We can rewrite α &

More information

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

Chapter 17 The bilinear covariant fields of the Dirac electron. from my book: Understanding Relativistic Quantum Field Theory. Chapter 17 The bilinear covariant fields of the Dirac electron from my book: Understanding Relativistic Quantum Field Theory Hans de Vries November 10, 008 Chapter Contents 17 The bilinear covariant fields

More information

1.7 Plane-wave Solutions of the Dirac Equation

1.7 Plane-wave Solutions of the Dirac Equation 0 Version of February 7, 005 CHAPTER. DIRAC EQUATION It is evident that W µ is translationally invariant, [P µ, W ν ] 0. W is a Lorentz scalar, [J µν, W ], as you will explicitly show in homework. Here

More information

be stationary under variations in A, we obtain Maxwell s equations in the form ν J ν = 0. (7.5)

be stationary under variations in A, we obtain Maxwell s equations in the form ν J ν = 0. (7.5) Chapter 7 A Synopsis of QED We will here sketch the outlines of quantum electrodynamics, the theory of electrons and photons, and indicate how a calculation of an important physical quantity can be carried

More information

Particle Physics WS 2012/13 ( )

Particle Physics WS 2012/13 ( ) Particle Physics WS /3 (3..) Stephanie Hansmann-Menzemer Physikalisches Institut, INF 6, 3. How to describe a free particle? i> initial state x (t,x) V(x) f> final state. Non-relativistic particles Schrödinger

More information

Relativistic quantum mechanics

Relativistic quantum mechanics Free-electron solution of Quantum mechanics 2 - Lecture 11 UJJS, Dept. of Physics, Osijek January 15, 2013 Free-electron solution of 1 2 3 Free-electron solution of 4 5 Contents Free-electron solution

More information

THEORY AND PRACTICES FOR ENERGY EDUCATION, TRAINING, REGULATION AND STANDARDS Basic Laws and Principles of Quantum Electromagnetism C.N.

THEORY AND PRACTICES FOR ENERGY EDUCATION, TRAINING, REGULATION AND STANDARDS Basic Laws and Principles of Quantum Electromagnetism C.N. BASIC LAWS AND PRINCIPLES OF QUANTUM ELECTROMAGNETISM C. N. Booth Department of Physics and Astronomy, University of Sheffield, UK Keywords: antiparticle, boson, Dirac equation, fermion, Feynman diagram,

More information

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

DISCRETE SYMMETRIES IN NUCLEAR AND PARTICLE PHYSICS. Parity PHYS NUCLEAR AND PARTICLE PHYSICS PHYS 30121 NUCLEAR AND PARTICLE PHYSICS DISCRETE SYMMETRIES IN NUCLEAR AND PARTICLE PHYSICS Discrete symmetries are ones that do not depend on any continuous parameter. The classic example is reflection

More information

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

msqm 2011/8/14 21:35 page 189 #197 msqm 2011/8/14 21:35 page 189 #197 Bibliography Dirac, P. A. M., The Principles of Quantum Mechanics, 4th Edition, (Oxford University Press, London, 1958). Feynman, R. P. and A. P. Hibbs, Quantum Mechanics

More information

Physics 582, Problem Set 1 Solutions

Physics 582, Problem Set 1 Solutions Physics 582, Problem Set 1 Solutions TAs: Hart Goldman and Ramanjit Sohal Fall 2018 1. THE DIRAC EQUATION [20 PTS] Consider a four-component fermion Ψ(x) in 3+1D, L[ Ψ, Ψ] = Ψ(i/ m)ψ, (1.1) where we use

More information

Path Integral for Spin

Path Integral for Spin Path Integral for Spin Altland-Simons have a good discussion in 3.3 Applications of the Feynman Path Integral to the quantization of spin, which is defined by the commutation relations [Ŝj, Ŝk = iɛ jk

More information

The quantum state as a vector

The quantum state as a vector The quantum state as a vector February 6, 27 Wave mechanics In our review of the development of wave mechanics, we have established several basic properties of the quantum description of nature:. A particle

More information

Physics 221B Spring 2018 Notes 47 Solutions of the Dirac Equation and Their Properties

Physics 221B Spring 2018 Notes 47 Solutions of the Dirac Equation and Their Properties Copyright c 218 by Robert G. Littlejohn Physics 221B Spring 218 Notes 47 Solutions of the Dirac Equation and Their Properties 1. Introduction In Notes 44 we introduced the Dirac equation in much the same

More information

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

Physics 217 FINAL EXAM SOLUTIONS Fall u(p,λ) by any method of your choosing. Physics 27 FINAL EXAM SOLUTIONS Fall 206. The helicity spinor u(p, λ satisfies u(p,λu(p,λ = 2m. ( In parts (a and (b, you may assume that m 0. (a Evaluate u(p,λ by any method of your choosing. Using the

More information

LS coupling. 2 2 n + H s o + H h f + H B. (1) 2m

LS coupling. 2 2 n + H s o + H h f + H B. (1) 2m LS coupling 1 The big picture We start from the Hamiltonian of an atomic system: H = [ ] 2 2 n Ze2 1 + 1 e 2 1 + H s o + H h f + H B. (1) 2m n e 4πɛ 0 r n 2 4πɛ 0 r nm n,m Here n runs pver the electrons,

More information

Introduction to Neutrino Physics. TRAN Minh Tâm

Introduction to Neutrino Physics. TRAN Minh Tâm Introduction to Neutrino Physics TRAN Minh Tâm LPHE/IPEP/SB/EPFL This first lecture is a phenomenological introduction to the following lessons which will go into details of the most recent experimental

More information

Disclaimer. [disclaimer]

Disclaimer. [disclaimer] Disclaimer This is a problem set (as turned in) for the module physics755. This problem set is not reviewed by a tutor. This is just what I have turned in. All problem sets for this module can be found

More information

Lecture #13 1. Incorporating a vector potential into the Hamiltonian 2. Spin postulates 3. Description of spin states 4. Identical particles in

Lecture #13 1. Incorporating a vector potential into the Hamiltonian 2. Spin postulates 3. Description of spin states 4. Identical particles in Lecture #3. Incorporating a vector potential into the Hamiltonian. Spin postulates 3. Description of spin states 4. Identical particles in classical and QM 5. Exchange degeneracy - the fundamental problem

More information

Quantum Field Theory I Examination questions will be composed from those below and from questions in the textbook and previous exams

Quantum Field Theory I Examination questions will be composed from those below and from questions in the textbook and previous exams Quantum Field Theory I Examination questions will be composed from those below and from questions in the textbook and previous exams III. Quantization of constrained systems and Maxwell s theory 1. The

More information

Weak interactions, parity, helicity

Weak interactions, parity, helicity Lecture 10 Weak interactions, parity, helicity SS2011: Introduction to Nuclear and Particle Physics, Part 2 2 1 Weak decay of particles The weak interaction is also responsible for the β + -decay of atomic

More information

What s up with those Feynman diagrams? an Introduction to Quantum Field Theories

What s up with those Feynman diagrams? an Introduction to Quantum Field Theories What s up with those Feynman diagrams? an Introduction to Quantum Field Theories Martin Nagel University of Colorado February 3, 2010 Martin Nagel (CU Boulder) Quantum Field Theories February 3, 2010 1

More information

Semi-Classical Theory of Radiative Transitions

Semi-Classical Theory of Radiative Transitions Semi-Classical Theory of Radiative Transitions Massimo Ricotti ricotti@astro.umd.edu University of Maryland Semi-Classical Theory of Radiative Transitions p.1/13 Atomic Structure (recap) Time-dependent

More information

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

Lorentz-covariant spectrum of single-particle states and their field theory Physics 230A, Spring 2007, Hitoshi Murayama Lorentz-covariant spectrum of single-particle states and their field theory Physics 30A, Spring 007, Hitoshi Murayama 1 Poincaré Symmetry In order to understand the number of degrees of freedom we need

More information

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

Particle Physics Dr M.A. Thomson Part II, Lent Term 2004 HANDOUT V Particle Physics Dr M.A. Thomson (ifl μ @ μ m)ψ = Part II, Lent Term 24 HANDOUT V Dr M.A. Thomson Lent 24 2 Spin, Helicity and the Dirac Equation Upto this point we have taken a hands-off approach to spin.

More information

E = φ 1 A The dynamics of a particle with mass m and charge q is determined by the Hamiltonian

E = φ 1 A The dynamics of a particle with mass m and charge q is determined by the Hamiltonian Lecture 9 Relevant sections in text: 2.6 Charged particle in an electromagnetic field We now turn to another extremely important example of quantum dynamics. Let us describe a non-relativistic particle

More information

DERIVATION OF DIRAC S EQUATION FROM THE EVANS WAVE EQUATION. Alpha Institute for Advanced Study

DERIVATION OF DIRAC S EQUATION FROM THE EVANS WAVE EQUATION. Alpha Institute for Advanced Study DERIVATION OF DIRAC S EQUATION FROM THE EVANS WAVE EQUATION M. W. Evans Alpha Institute for Advanced Study E-mail: emyrone@aol.com Received 27 August 2003; revised 25 October 2003 The Evans wave equation

More information

1. Estimate the lifetime of an excited state of hydrogen. Give your answer in terms of fundamental constants.

1. Estimate the lifetime of an excited state of hydrogen. Give your answer in terms of fundamental constants. Sample final questions.. Estimate the lifetime of an excited state of hydrogen. Give your answer in terms of fundamental constants. 2. A one-dimensional harmonic oscillator, originally in the ground state,

More information

Elementary Par,cles Rohlf Ch , p474 et seq.

Elementary Par,cles Rohlf Ch , p474 et seq. Elementary Par,cles Rohlf Ch. 17-18, p474 et seq. The Schroedinger equa,on is non- rela,vis,c. Rela,vis,c wave equa,on (Klein- Gordon eq.) Rela,vis,c equa,on connec,ng the energy and momentum of a free

More information

where P a is a projector to the eigenspace of A corresponding to a. 4. Time evolution of states is governed by the Schrödinger equation

where P a is a projector to the eigenspace of A corresponding to a. 4. Time evolution of states is governed by the Schrödinger equation 1 Content of the course Quantum Field Theory by M. Srednicki, Part 1. Combining QM and relativity We are going to keep all axioms of QM: 1. states are vectors (or rather rays) in Hilbert space.. observables

More information

Maxwell s equations. based on S-54. electric field charge density. current density

Maxwell s equations. based on S-54. electric field charge density. current density Maxwell s equations based on S-54 Our next task is to find a quantum field theory description of spin-1 particles, e.g. photons. Classical electrodynamics is governed by Maxwell s equations: electric field

More information

lattice QCD and the hadron spectrum Jozef Dudek ODU/JLab

lattice QCD and the hadron spectrum Jozef Dudek ODU/JLab lattice QCD and the hadron spectrum Jozef Dudek ODU/JLab the light meson spectrum relatively simple models of hadrons: bound states of constituent quarks and antiquarks the quark model empirical meson

More information

Quantization of the Spins

Quantization of the Spins Chapter 5 Quantization of the Spins As pointed out already in chapter 3, the external degrees of freedom, position and momentum, of an ensemble of identical atoms is described by the Scödinger field operator.

More information

Fermi Fields without Tears

Fermi Fields without Tears Fermi Fields without Tears Peter Cahill and Kevin Cahill cahill@unm.edu http://dna.phys.unm.edu/ Abstract One can construct Majorana and Dirac fields from fields that are only slightly more complicated

More information

Chapter 10 Operators of the scalar Klein Gordon field. from my book: Understanding Relativistic Quantum Field Theory.

Chapter 10 Operators of the scalar Klein Gordon field. from my book: Understanding Relativistic Quantum Field Theory. Chapter 10 Operators of the scalar Klein Gordon field from my book: Understanding Relativistic Quantum Field Theory Hans de Vries November 11, 2008 2 Chapter Contents 10 Operators of the scalar Klein Gordon

More information

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

Outline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification Weak Interactions Outline Charged Leptonic Weak Interaction Decay of the Muon Decay of the Neutron Decay of the Pion Charged Weak Interactions of Quarks Cabibbo-GIM Mechanism Cabibbo-Kobayashi-Maskawa

More information

Rotations in Quantum Mechanics

Rotations in Quantum Mechanics Rotations in Quantum Mechanics We have seen that physical transformations are represented in quantum mechanics by unitary operators acting on the Hilbert space. In this section, we ll think about the specific

More information

Chapter 3: Relativistic Wave Equation

Chapter 3: Relativistic Wave Equation Chapter 3: Relativistic Wave Equation Klein-Gordon Equation Dirac s Equation Free-electron Solutions of the Timeindependent Dirac Equation Hydrogen Solutions of the Timeindependent Dirac Equation (Angular

More information

1 The postulates of quantum mechanics

1 The postulates of quantum mechanics 1 The postulates of quantum mechanics The postulates of quantum mechanics were derived after a long process of trial and error. These postulates provide a connection between the physical world and the

More information

Loop corrections in Yukawa theory based on S-51

Loop corrections in Yukawa theory based on S-51 Loop corrections in Yukawa theory based on S-51 Similarly, the exact Dirac propagator can be written as: Let s consider the theory of a pseudoscalar field and a Dirac field: the only couplings allowed

More information

Relativistic Electron Theory The Dirac Equation Mathematical Physics Project

Relativistic Electron Theory The Dirac Equation Mathematical Physics Project Relativistic Electron Theory The Dirac Equation Mathematical Physics Project Karolos POTAMIANOS Université Libre de Bruxelles Abstract This document is about relativistic quantum mechanics and more precisely

More information

Particle Physics 2018 Final Exam (Answers with Words Only)

Particle Physics 2018 Final Exam (Answers with Words Only) Particle Physics 2018 Final Exam (Answers with Words Only) This was a hard course that likely covered a lot of new and complex ideas. If you are feeling as if you could not possibly recount all of the

More information

Quantum Physics II (8.05) Fall 2002 Outline

Quantum Physics II (8.05) Fall 2002 Outline Quantum Physics II (8.05) Fall 2002 Outline 1. General structure of quantum mechanics. 8.04 was based primarily on wave mechanics. We review that foundation with the intent to build a more formal basis

More information

ψ(t) = U(t) ψ(0). (6.1.1)

ψ(t) = U(t) ψ(0). (6.1.1) Chapter 6 Symmetries 6.1 Quantum dynamics The state, or ket, vector ψ of a physical system completely characterizes the system at a given instant. The corresponding bra vector ψ is the Hermitian conjugate

More information