1 FK7003 Lecture 6 ● Isospin ● SU(2) and SU(3) ● Parity.

Slides:



Advertisements
Similar presentations
: The mirror did not seem to be operating properly: A guide to CP violation C hris P arkes 12/01/2006.
Advertisements

The Standard Model and Beyond [Secs 17.1 Dunlap].
Originally form Brian Meadows, U. Cincinnati Bound States.
Symmetries and conservation laws:
Shu-Yu Ho Date : 2010/9/20 QFT study group
1 FK7003 Lecture 8 ● CP -violation ● T -violation ● CPT invariance.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE  5-Feb pm Physics LRA Dr M Burleigh Intro lecture  9-Feb-04.
Symmetries By Dong Xue Physics & Astronomy University of South Carolina.
UNIT 2: OUTLINE SYLLABUS: 1st Lecture Introduction Hadrons and Leptons Spin & Anti-Particles The conservation laws: Lepton Number Baryon number Strangeness.
P461 - decays II1 Parity Violation in Beta Decays The Parity operator is the mirror image and is NOT conserved in Weak decays (is conserved in EM and strong)
Modern Physics LECTURE II.
Eightfold Way (old model)
Quark Soup Elementary Particles?? (circa 1960)   (pions),  K , , etc proton neutron        c,  b, Etc www-pnp.physics.ox.ac.uk/~huffman/
Symmetries and conservation laws
Quantum Electrodynamics Dirac Equation : spin 1/2.
Elementary particles atom Hadrons Leptons Baryons Mesons Nucleons
J.5.1State what is meant by deep inelastic scattering. J.5.2Analyze the results of deep inelastic scattering. J.5.3Describe what is meant by asymptotic.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 26-Jan pm LRB Intro lecture 28-Jan pm LRBProblem solving.
Lecture 5 – Symmetries and Isospin
Particle Physics J4 Leptons and the standard model.
10 lectures. classical physics: a physical system is given by the functions of the coordinates and of the associated momenta – 2.
Electroweak Theory Mr. Gabriel Pendas Dr. Susan Blessing.
ParticleZoo. The Standard Model The body of currently accepted views of structure and interactions of subatomic particles. Interaction Coupling Charge.
Symmetry and conservation Laws Submitted: Pro. Cho By Adil Khan.
Physics for Scientists and Engineers, 6e Chapter 46 - Particle Physics and Cosmology.
Elementary Particles: Physical Principles Benjamin Schumacher Physics April 2002.
1 Conservation Kihyeon Cho April 5, 2011 HEP. What is the world made of? What holds the world together? Where did we come from? the smallest things in.
From Luigi DiLella, Summer Student Program
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 26-Jan pm LRB Intro lecture 28-Jan pm LRBProblem solving.
Mesons and Glueballs September 23, 2009 By Hanna Renkema.
PARTICLE PHYSICS Particles and Interactions. Classifying Particles Most particles fall broadly into two types which can then be broken down further The.
Eightfold Way (old model)
P Spring 2003 L5 Isospin Richard Kass
Properties conserved in Strong and EM interactions
Dr. Bill Pezzaglia Particle Physics Updated: 2010May20 Modern Physics Series 1 ROUGH DRAFT.
WHAT IS THE DIFFERENCE BETWEEN A LEFT AND A RIGHT HABD? RH IS BIGGER THAN LH ???
[Secs 16.1 Dunlap] Conservation Laws - II [Secs 2.2, 2.3, 16.4, 16.5 Dunlap]
Lecture 2: The First Second Baryogenisis: origin of neutrons and protons Hot Big Bang Expanding and cooling “Pair Soup” free particle + anti-particle pairs.
Kihyeon Cho Kyungpook National University
Wednesday, Apr. 13, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #19 Wednesday, Apr. 13, 2005 Dr. Jae Yu Parity Determination of Parity Parity.

The Zoo of Subatomic Particles
Monday, Apr. 4, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #16 Monday, Apr. 4, 2005 Dr. Jae Yu Symmetries Why do we care about the symmetry?
Lecture 7: Symmetries II Charge Conjugation Time Reversal CPT Theorem Baryon & Lepton Number Strangeness Applying Conservation Laws Section 4.6, Section.
P Spring 2002 L4Richard Kass Conservation Laws When something doesn’t happen there is usually a reason! Read: M&S Chapters 2, 4, and 5.1, That something.
J.4.1State the three-family structure of quarks and leptons in the standard model. J.4.2State the lepton number of the leptons in each family. J.4.3Solve.
U(1) Define a property characterized by a single value. Define a property characterized by a single value. E.G. Objects color E.G. Objects color Change.
Monday, Apr. 11, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #18 Monday, Apr. 11, 2005 Dr. Jae Yu Symmetries Local gauge symmetry Gauge fields.
10/29/2007Julia VelkovskaPHY 340a Lecture 4: Last time we talked about deep- inelastic scattering and the evidence of quarks Next time we will talk about.
Symmetries in particle physics Symmetries: Spins and their addition The eightfold way revisited Discrete symmetries: Charge conjugation, parity and time.
The quark model FK7003.
Lecture 7 Parity Charge conjugation G-parity CP FK7003.
The Standard Model of Particle Physics
Announcements Please fill out ECAFE online evaluations !!!
The Standard Model.
Countries that signed the nuclear arms treaty with Iran
Handout 9 : The Weak Interaction and V-A
Lecture 04 - Hadrons Quarks multiplets Hadron decays Resonances
Developments of the quark model
Unit 7.3 Review.
The Standard Model strong nuclear force electromagnetic force
Aim: How can we describe Fundamental Particles?
Matter vs. Antimatter The Question of Symmetry
Quarks Throughout the 1950 – 1960s, a huge variety of additional particles was found in scattering experiments. This was referred to as the “particle zoo”.
Quantum numbers.
Advanced Topics Nuclear Physics ElementaryParticles General Relativity
Standard Model of Particles
The symmetry of interactions
Section IX - Quark Model of Hadrons
The Standard Model By: Dorca Lee.
Presentation transcript:

1 FK7003 Lecture 6 ● Isospin ● SU(2) and SU(3) ● Parity

2 FK7003 Reminder about isospin (1) ● We’re dealing with the strong force. ● The theory of the strong force works extremely well (can’t be proven wrong) for interactions at high energies (>> 1 GeV).  Forthcoming lectures ● At low energies we can’t do much.  We can’t calculate all hadron masses from first principles.  We can’t calculate all reaction rates from first principles. ● We use symmetry (isospin) as an experimentally established fact to guide us and help us ”feel our way” wrt strong force observables

3 FK7003 Reminder (2) – conservation of isospin

4 FK7003 Reminder (3): invariance to a rotation in isospin space

5 FK7003 Quarks and isospin

6 FK7003 Isospin of antiquarks (not for lecture or exam)

7 FK7003 Isospin with quarks - continued    I3I3 I3I3 Not used by nature

8 FK7003 Question ● Write down a particle decay which does not conserve isospin.

9 FK7003 Isospin and group theory

10 FK7003 Conservation of isospin ● Conserved for strong processes. ● Violated for weak and electromagnetic processes. ● Can think about as: photon, W,Z, and the leptons have zero isospin:

11 FK7003 Why does isospin work ?

12 FK7003 ● Strange, charm and bottom quarks also form hadrons. ● Large mass differences between the quarks. ● What kind of symmetry can we obtain here. Quark Q (e) Mass (GeV) BSCBT u- up2/ /30000 d- down-1/ /30000 s- strange-1/30.151/3000 c- charm2/31.21/30100 b- bottom-1/34.21/3000 t-top2/31711/30001  4 GeV  1 GeV 0.1 GeV  2 MeV The other quarks

13 FK7003 From SU(2) to SU(3)    I3I3 I3I3 ½-½ +1 Meson nonet (spin 0)

14 FK7003 Identifying the states SU(3) is an approximate symmetry. Particles within multiplet have large mass differences. Due to quark mass differences! Strong force is not invariant to SU(3) flavour transformations. Useful to catalogue the states and their quark composition. (6.20) (6.14) (6.21)

15 FK7003 SU(3) Flavour – mesons of spin 1 (vector) (6.22)

16 FK7003 Question 1. What is the strangeness of the   meson ? 2. Give evidence that the   meson is more likely to consist of ss than uu.

17 FK7003 Higher mass meson multiplets Spectroscopic notation – explored further in lectures on bound states.

18 FK7003 Baryons Spin ½ Spin 3/2 Historically, these arrangements of hadrons was termed ” the eight-fold way ” by Murray Gell-Mann after the octet arrangement above. This work allowed the understanding of hadron masses and properties in terms of quarks and was the first evidence for quarks. Like all good theories it gave a prediction which experimentalists could verify.

19 FK7003 Baryon decuplet – something missing? 1964 One particle was missing to make up the baryon decuplet. ?

20 FK7003 Discovery of the  

21 FK7003 Summary of isospin, SU(2) and SU(3) ● Isospin is a good symmetry of the strong force  Hadron masses, reaction/decay rates respect isospin symmetry  The strong force is invariant to SU(2) isospin transformations.  This is due to the small u,d mass difference ● The other quarks are much heavier than u,d and show large mass differences.  SU(3) flavour symmetry is useful for enumerating and ordering the different hadrons and understanding their quark composition.  The strong force is not invariant to SU(3) flavour transformations since the quark masses are so different.

22 FK7003 Parity ● The laws of physics are invariant to, eg a shifted co-ordinate system ( x’ x+a ) or rotated co-ordinate system. ● What happens if we make a parity transformation: invert the co-ordinate system ( x,y,z) (-x,-y,-z) ? ● Parity is a discrete symmetry offering two possible states

23 FK7003 ● Invert the spatial co-ordinate system  Parity transformation (P)  Change handedness of co-ordinate system (eg right to left) ● By 1956 parity invariance had been shown for the strong and electromagnetic forces. ● A test for the weak force was needed.. Parity

24 FK7003 Parity A reflection in the x-z plane followed by a rotation about the y-axis is equivalent to a parity transformation. To test parity invariance: study a reaction and ask if the mirror reflection of that process has the same probability of occuring (no need to consider further rotation since rotation invariance is implied by angular momentum conservation).

25 FK7003 Parity violation – Wu’s experiment Study the   decay of Co-60 At a low temperature 0.01K, the spins can be polarised parallel to an external magnetic field. The electrons are dominantly emitted in the direction opposite to the spin In the ”mirror” image, the electron is dominantly emitted in the opposite parallel to the spin. Parity is violated in weak decays ! A symmetry which is violated means that some quantity is not being conserved

26 FK7003 Helicity A particle possesses helicity – Arbitary z -axis for spin angular momentum – select direction of motion Helicity is not a useful quantity for most particles since it isn’t a Lorentz invariant Can be defined for luminal particles eg a massless neutrino (6.23)

27 FK7003 Muon measured and found to be right-handed  Neutrino oscillations imply that they have a tiny mass ( <2 eV). Maybe its better to say that most neutrinos are left-handed and most anti-neutrinos are right-handed. Certainly, it’s a good approximation since left-handed neutrino and right-handed antineutrino are just about impossible to observe in laboratory experiments. s

28 FK7003 What parity did to the neutrinos in Wu’s experiment Parity transformation means moving from a right-handed to a left-handed co-ordinate system Wu’s experiment is  - decay A ”mirror reflection” of the right-handed anti- neutrino is a left-handed anti-neutrino. We don’t observe the ”reflected” process. ss Change handedness

29 FK7003 Parity ● Parity is a symmetry respected by the electromagnetic and strong forces ● Parity is violated by the weak force.

30 FK7003 Summary ● Isospin and flavour symmetries ● Parity – space inversion ● Weak interactions are not invariant to parity