1 PHYS 3446 Wednesday, Nov. 13, 2013 Dr. Jae Yu 1. Elementary Particle Properties Quantum Numbers Strangeness Isospin Gell-Mann-Nishijima Relations Production.

Slides:



Advertisements
Similar presentations
Quarks come in six different types, with six antipartners. On the A-level syllabus, you need to know about three: up, and down (which make up everyday.
Advertisements

Garfield Graphics included with kind permission from PAWS Inc. All Rights Reserved. Strange Particles AS level Notes.
Properties and Decays of Heavy Flavor S-Wave Hadrons Rohit Dhir Department of Physics, Yonsei University, Seoul Dated:11 th June, 2012.
The Standard Model and Beyond [Secs 17.1 Dunlap].
Particle Reactions and Decays - I [Secs 16.1, 16.2 Dunlap]
FLAVOURS 50 Years After SU(3) Discovery Djordje Šijački.
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.
P461 - particles II1 Lepton and Baryon Conservation Strong and EM conserve particle type. Weak can change but always lepton->lepton or quark->quark So.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 3-Feb pm Physics LRA Dr Matt Burleigh Intro lecture 7-Feb-05.
P461 - particles I1 all fundamental with no underlying structure Leptons+quarks spin ½ while photon, W, Z, gluons spin 1 No QM theory for gravity Higher.
UNIT 2: OUTLINE SYLLABUS: 1st Lecture Introduction Hadrons and Leptons Spin & Anti-Particles The conservation laws: Lepton Number Baryon number Strangeness.
8:00am 9:00 10:00 11:00 12:00pm 1:00 2:00 3:00 4:00 5:00 6:00 7:00 Monday Tuesday Wednesday Thursday Friday Apr 25??? Make up schedule April 11 catch a.
Nucleon Scattering d dd dd dd dd dd d | I,I 3  | 1, 1  | 1,  1  | 1 0  If the strong interaction is I 3 -invariant These.
Modern Physics LECTURE II.
Eightfold Way (old model)
Elementary particles atom Hadrons Leptons Baryons Mesons Nucleons
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Nuclear Force Spin dependent  difference in neutron scattering cross.
Particle Physics Intro. What’s Stuff Made Of…Really? All particles can be grouped into two categories: Fermions and Bosons Things to know about Fermions:
Particles energy states
Wednesday, Mar. 23, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #14 Wednesday, Mar. 23, 2005 Dr. Jae Yu Elementary Particle Properties Forces.
P Spring 2003 L6Richard Kass Parity Let us examine the parity operator (P) and its eigenvalues. The parity operator acting on a wavefunction is defined.
The Particle Zoo. Too Many Particles Far from just finding Protons Neutrons Electrons Neutrinos and their antiparticles, during the 20 th century many.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 26-Jan pm LRB Intro lecture 28-Jan pm LRBProblem solving.
1.7 THE EIGHTFOLD WAY ( ). The Mendeleev of elementary particle physics was Murray Gell-Mann, who introduced the so- called Eightfold Way.
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.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 26-Jan pm LRB Intro lecture 28-Jan pm LRBProblem solving.
Monday, Nov. 20, 2006PHYS 3446, Fall 2006 Jae Yu 1 PHYS 3446 – Lecture #20 Monday, Nov. 20, 2006 Dr. Jae Yu 1. Parity Properties of Parity Determination.
PARTICLE PHYSICS Particles and Interactions. Classifying Particles Most particles fall broadly into two types which can then be broken down further The.
1 FK7003 Lecture 6 ● Isospin ● SU(2) and SU(3) ● Parity.
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.
Lecture 12: The neutron 14/10/ Particle Data Group entry: slightly heavier than the proton by 1.29 MeV (otherwise very similar) electrically.
The Four Fundamental Forces 1.Gravity 2.Weak Force 3.Electromagnetic force 4.Strong Force Weaker Stronger All other forces you know about can be attributed.
The Nucleus Nucleons- the particles inside the nucleus: protons & neutrons Total charge of the nucleus: the # of protons (z) times the elementary charge.
What IS Fundamental???  Many new particles were discovered with the advent of particle accelerators …are they ALL fundamental??? Baryons: particles with.
Quarks and Leptons Announcements 1.Recitation this week in lab. BRING QUESTIONS ! 2.See my by Wed. if you have any grading issues with your exam. 3.Reading.
12004, TorinoAram Kotzinian Neutrino Scattering Neutrino interactions Neutrino-electron scattering Neutrino-nucleon quasi-elastic scattering Neutrino-nucleon.
Multiplet Structure - Isospin and Hypercharges. As far as strong interactions are concerned, the neutron and the proton are the two states of equal mass.
[Secs 16.1 Dunlap] Conservation Laws - II [Secs 2.2, 2.3, 16.4, 16.5 Dunlap]
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.
M. Cobal, PIF 2003 Weak Interactions Take place between all the quarks and leptons (each of them has a weak charge) Usually swamped by the much stronger.
Wednesday, Jan. 15, 2003PHYS 5396, Spring 2003 Jae Yu 1 PHYS 5396 – Lecture #2 Wednesday, Jan. 15, 2003 Dr. Jae Yu 1.What is a neutrino? 2.History of neutrinos.
The Particle Zoo Particle Physics Lesson 6. What are the charges? γ (photon) γ (photon) p (proton) p (proton) n (neutron) n (neutron) ν (neutrino) ν (neutrino)
What makes up the nucleus? Nucleus is positively charged Different atoms have same electrical properties but different masses Isotopes – same atomic number,
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Electromagnetic moments Electromagnetic interaction  information about.
Monday, Feb. 7, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #6 Monday, Feb. 7, 2005 Dr. Jae Yu 1.Nature of the Nuclear Force Short Range Nature.
Nuclear Physics, JU, Second Semester,
Particle Physics "three quarks for Muster Mark" -James Joyce (Finnegan’s Wake) Contents: Particle Accelerators Quantum Electrodynamics and Feynman diagrams.
M. Cobal, PIF 2006/7 Quarks. Quarks are s = ½ fermions, subject to all kind of interactions. They have fractional electric charges Quarks and their bound.
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.
P ARTICLE P HYSICS A brief intro to the quantum world of particles.
Lecture 04 - Hadrons Quarks multiplets Hadron decays Resonances
Unit 7.3 Review.
The Standard Model strong nuclear force electromagnetic force
Aim: How can we describe Fundamental Particles?
Quarks Throughout the 1950 – 1960s, a huge variety of additional particles was found in scattering experiments. This was referred to as the “particle zoo”.
PHYS 663 Advanced Particles Physics
Elementary Particles.
ELEMENTARY PARTICLES.
Do Now An electron in a hydrogen atoms drops from n=5 to n=4 energy level. What is the energy of the photon in eV? What is the frequency of the emitted.
PHYS 3446 – Lecture #20 Elementary Particle Properties
PHYS 3446 – Lecture #20 Monday ,April 16, 2012 Dr. Brandt Accelerator
PHYS 3446 – Lecture #21 Quantum Numbers Symmetries
PHYS 3446 – Lecture #14 Elementary Particle Properties
Physics 4 – April 18, 2019 Agenda:
Presentation transcript:

1 PHYS 3446 Wednesday, Nov. 13, 2013 Dr. Jae Yu 1. Elementary Particle Properties Quantum Numbers Strangeness Isospin Gell-Mann-Nishijima Relations Production and Decay of Resonances Wednesday, Nov. 13, 2013

Announcements Dr. Farbin will be at UTA between 11am – 4pm Friday for research discussions –Please send an ahead with an estimated time for your to stop by Wednesday, Nov. 13,

3 Baryon Number –An additive and conserved quantum number, Baryon number (B), assigned to baryons –All baryons have B=1; How about anti-baryons? –Anti-baryons have B=-1; How about leptons and mesons? –Photons, leptons and mesons have B=0 Lepton Number –Quantum number assigned to leptons –All leptons carry L =1 (particles) or L =-1 (antiparticles) –Photons or hadrons carry L =0 –Total lepton number must be conserved –Lepton numbers by species must be conserved Quantum Numbers Wednesday, Nov. 13, 2013

4 From cosmic ray shower observations –K-mesons and  Λ0 Λ0 baryons are produced strongly w/ large x-sec But their lifetime is typical of weak interactions (~ sec) Are produced in pairs – a K w/ a  or a K w/ a Λ0Λ0 –Gave an indication of a new quantum number Strangeness Wednesday, Nov. 13, 2013

Kaon Properties and Quark Compositions Wednesday, Nov. 13,

6 From cosmic ray shower observations –K-mesons and  Λ0 Λ0 baryons are produced strongly w/ large x-sec But their lifetime is typical of weak interactions (~ sec) Are produced in pairs – a K w/ a  or a K w/ a Λ0Λ0 –Gave an indication of a new quantum number Consider the reaction –K0 –K0 and Λ0 Λ0 subsequently decay – and Observations on Λ0Λ0 – Always produced w/ K0 K0 never w/ just a 00 – Produced w/ K+ K+ but not w/ K-K- Strangeness Wednesday, Nov. 13, 2013

Λ properties and quark compositions Wednesday, Nov. 13,

8 Consider reactions and –With the subsequent decays and Observations from ++ – + + is always produced w/ a K+ K+ never w/ just a ++ – + + is also produced w/ a K0 K0 but w/ an additional + + for charge conservation Observations from  –   is always produced w/ a K+ K+ never w/ K-K- Thus, –Observed: –Not observed: Strangeness Wednesday, Nov. 13, 2013

 Properties and Quark Compositions Wednesday, Nov. 13,

10 – Λ0 Λ0 at v~0.1c decays in about 0.3cm Lifetime of Λ0 Λ0 baryon is The short lifetime of these strange particles indicate a weak decay Further observation of cross section measurements –The cross section for reactions and w/ 1GeV/c pion momenta are ~ 1mb Whereas the total pion-proton scattering cross section is ~ 30mb The interactions are strong interactions Strangeness Wednesday, Nov. 13, 2013

11 The strangeness quantum number –Murray Gell-Mann and Abraham Pais proposed a new additive quantum number that are carried by these particles – Conserved in strong interactions –Violated in weak decays –S=0 for all ordinary mesons and baryons as well as photons and leptons –For any strong associated-production reaction w/ the initial state S=0, the total strangeness of particles in the final state should add up to 0. Strangeness Wednesday, Nov. 13, 2013

12 Based on experimental observations of reactions and w/ an arbitrary choice of S(K 0 )=1, we obtain –S(K + )=S(K 0 )=1 and  K  )=   )=-1 –S( Λ 0 )=S    S(  0 )=S(  - )=-1 –Does this work for the following reactions? – – For strong production reactions and – cascade particles if Strangeness Wednesday, Nov. 13, 2013

Ξ properties and quark compositions Wednesday, Nov. 13,

14 Let’s look at the reactions again –This is a strong interaction Strangeness must be conserved S:  +1 How about the decays of the final state particles? – and –These decays are weak interactions so S is not conserved –S:  and +1  A not-really-elegant solution – – only conserved in Strong and EM interactions  Unique strangeness quantum numbers cannot be assigned to leptons Leads into the necessity of strange quarks More on Strangeness Wednesday, Nov. 13, 2013

15 Strong force does not depend on the charge of the particle –Nuclear properties of protons and neutrons are very similar –From the studies of mirror nuclei, the strengths of p-p, p-n and n-n strong interactions are essentially the same –If corrected by EM interactions, the x-sec between n-n and p-p are the same Since strong force is much stronger than any other forces, we could imagine a new quantum number that applies to all particles –Protons and neutrons are two orthogonal mass eigenstates of the same particle like spin up and down states Isospin Quantum Number Wednesday, Nov. 13, 2013

16 Protons and neutrons are degenerate in mass because of some symmetry of the strong force –Isospin symmetry  Under the strong force these two particles appear identical –Presence of Electromagnetic or Weak forces breaks this symmetry, distinguishing p from n Isospin works just like spins –Protons and neutrons have isospin ½  Isospin doublet –Three pions,  +, - - and  0, have almost the same masses –X-sec by these particles are almost the same after correcting for EM effects –Strong force does not distinguish these particles  Isospin triplet Isospin Quantum Number Wednesday, Nov. 13, 2013

17 This QN is found to be conserved in strong interactions But not conserved in EM or Weak interactions Third component of the isospin QN is assigned to be positive for the particles with larger electric charge Isospin is not a space-time symmetry Cannot be assigned uniquely to leptons and photons since they are not involved in strong interactions –There is something called weak-isospin for weak interactions Isospin Quantum Number Wednesday, Nov. 13, 2013

18 Strangeness assignment is based on Gell-Mann- Nishijima relation –Electric charge of a hadron can be related to its other quantum numbers –Where Q: hadron electric charge I 3 : third component of isospin Y=B+S, strong hypercharge –Quantum numbers of several long lived particles follow this rule Gell-Mann-Nishijima Relation Wednesday, Nov. 13, 2013

19 With the discovery of new flavor quantum numbers, charm and bottom, this relationship was modified to include these new additions (Y=B+S+C+B) –Since the charge and the isospin are conserved in strong interactions, the strong hypercharge, Y, is also conserved in strong interactions This relationship holds in all strong interactions Gell-Mann-Nishijima Relation Wednesday, Nov. 13, 2013

20 Quantum numbers for a few hadrons Wednesday, Nov. 13, 2013

21 The QN we learned are conserved in strong interactions are but many of them are violated in EM or weak interactions Three types of weak interactions –Hadronic decays: Only hadrons in the final state –Semi-leptonic decays: both hadrons and leptons are present –Leptonic decays: only leptons are present Violation of Quantum Numbers Wednesday, Nov. 13, 2013

22 QN Λ 0  -- p I3I3 0½ S 00 These decays follow selection rules: | Δ I 3 |=1/2 and | Δ S|=1 Hadronic Weak Decays QN  +  00 p I3I3 10½ S00 QN  0  ++ -- I3I3 - ½1 S100 QN  -  Λ0Λ0 -- I3I3 - ½0 S-20 ΔΔ 1/

Wednesday, Nov. 13, QNnn p e - +  e I3I3 -1/21/2 S00 These decays follow selection rules: | Δ I 3 |=1 and | Δ S|=0 or | Δ I 3 |= ½ and | Δ S|=1 Semi-leptonic Weak Decays QN  -     I3I3 S0 QN  +  00     I3I3 ½0 S10 QN  -  n e - +  e I3I3 -1/2 S0 ΔΔ /2 1 1

24 Hadronic weak-decays –Selection rules are | Δ I 3 |=1/2 and | Δ S|=1 –| Δ I 3 |=3/2 and | Δ S|=2 exists but heavily suppressed Semi-leptonic weak-decays –Type 1: Strangeness conserving Selection rules are: | Δ S|=0, | Δ I 3 |=1 and | Δ I |=1 –Type 2: Strangeness non-conserving Selection rules are: | Δ S|=1, | Δ I 3 |= ½ and | Δ I |= ½ or 3/2 Δ I =3/2 and | Δ S|=1 exist but heavily suppressed Summary of Weak Decays Wednesday, Nov. 13, 2013

25 EM Processes QN  0   I3I3 0 S0 QN  0   I3I3 0 S0 QN  0  ΛΛ  I3I3 00 S ΔΔ Strangeness is conserved but the total isospin is not –Selection rules are: | Δ S|=0, | Δ I 3 |=0 and Δ I = 1or 0 Wednesday, Nov. 13, 2013

26 Baryon Number –An additive and conserved quantum number, Baryon number (B) –This number is conserved in general but not absolute Lepton Number –Quantum number assigned to leptons –Lepton numbers by species and the total lepton numbers must be conserved Strangeness Numbers –Conserved in strong interactions –But violated in weak interactions Isospin Quantum Numbers –Conserved in strong interactions –But violated in weak and EM interactions Quantum Numbers Wednesday, Nov. 13, 2013