Properties conserved in Strong and EM interactions

Slides:



Advertisements
Similar presentations
Radius of Observable Universe and Expansion Rate vs time, k = 0  = 0 Radiation dominated R = 3 x cm R = 10 cm R. =10 18 c c.
Advertisements

The Standard Model and Beyond [Secs 17.1 Dunlap].
Brian Meadows, U. Cincinnati Discrete Symmetries Noether’s theorem – (para-phrased) “A symmetry in an interaction Lagrangian corresponds to a conserved.
Symmetries and conservation laws:
Shu-Yu Ho Date : 2010/9/20 QFT study group
1 FK7003 Lecture 8 ● CP -violation ● T -violation ● CPT invariance.
Charge conservation: is the principle that electric charge can neither be created nor destroyed. The quantity of electric charge, the amount of positive.
Symmetries By Dong Xue Physics & Astronomy University of South Carolina.
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.
Modern Physics LECTURE II.
Eightfold Way (old model)
Feynman Diagrams.
Quantum Electrodynamics Dirac Equation : spin 1/2.
Elementary particles atom Hadrons Leptons Baryons Mesons Nucleons
Particle Physics J1 Particles and Interactions. Particle Physics Description and classification State what is meant by an elementary particle (no internal.
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:
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.
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.
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.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 26-Jan pm LRB Intro lecture 28-Jan pm LRBProblem solving.
BY: BRETT SLAJUS Particle Physics. Standard Model of Elementary Particles Three Generations of Matter (Fermions)
Lecture 5 – Symmetries and Isospin
Particle Physics J4 Leptons and the standard model.
ParticleZoo. The Standard Model The body of currently accepted views of structure and interactions of subatomic particles. Interaction Coupling Charge.
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.
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.
1 FK7003 Lecture 6 ● Isospin ● SU(2) and SU(3) ● Parity.
P Spring 2003 L5 Isospin Richard Kass
Dr. Bill Pezzaglia Particle Physics Updated: 2010May20 Modern Physics Series 1 ROUGH DRAFT.
M. Cobal, PIF 2003 Resonances - If cross section for muon pairs is plotted one find the 1/s dependence -In the hadronic final state this trend is broken.
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.
Subatomic Particles Lesson 10. Objectives describe the modern model of the proton and neutron as being composed of quarks. compare and contrast the up.
Classification of the Elementary Particles
The Nucleus Nucleons- the particles inside the nucleus: protons & neutrons Total charge of the nucleus: the # of protons (z) times the elementary charge.
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]
Lecture 2: The First Second Baryogenisis: origin of neutrons and protons Hot Big Bang Expanding and cooling “Pair Soup” free particle + anti-particle pairs.
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.
What is the Standard Model of Particle Physics ???? 1. A theory of three of the four known fundamental interactions and the elementary particles that.
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Electromagnetic moments Electromagnetic interaction  information about.
1 PHYS 3446 Wednesday, Nov. 13, 2013 Dr. Jae Yu 1. Elementary Particle Properties Quantum Numbers Strangeness Isospin Gell-Mann-Nishijima Relations Production.
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.
Nuclear Physics, JU, Second Semester,
Physics 222 UCSD/225b UCSB Lecture 12 Chapter 15: The Standard Model of EWK Interactions A large part of today’s lecture is review of what we have already.
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.
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.
Feynman Diagrams Topic 7.3.
NUCLEAR ENERGY. The daughter nuclei in the reaction above are highly unstable. They decay by beta emission until they reach stable nuclei.
 All elementary particles in physics are classified as either fermions or bosons. Quantum physics demonstrates the particles may have an intrinsic non-zero.
Lecture 7 Parity Charge conjugation G-parity CP FK7003.
The Standard Model of Particle Physics
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?
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
PHYS 663 Advanced Particles Physics
PHYS 3446 – Lecture #20 Elementary Particle Properties
PHYS 3446 – Lecture #21 Quantum Numbers Symmetries
Presentation transcript:

Properties conserved in Strong and EM interactions Grass 20090817 http://www.physnet.org/modules/pdf_modules.html

Outline Multiplets Strangeness Charge Conjugation (C) Parity (P) Time Reversal (T) T Inv. and Weak Decays: CPT Inv. Isospin Concept Isospin Calculation Isospin Conservation Application

Multiplets Hadrons can be arranged in small groups with all members of the group having nearly the same mass. The members of a group are called by the same name (pions, kaons, nucleons, antikaons, etc). The groups are called multiplets and the number of particles in a group is called the multiplicity of that group. B=Baryon number S=Strangeness Y=Hypercharge =Twice of Qave S=Y-B This formula must be altered for particles that have Charm.

Note K- is antiparticle of K+. But Σ- not antiparticle of Σ+ . How about π? Why they can stay in same multiplet?

Reminder Universal conservation conservation of energy conservation of baryon number conservation of lepton number conservation of charge conservation of momentum

Strangeness Decay time Strong ~10-23 sec EM ~ 10-21 sec Weak ~ 10-10 sec Nine example for weak decay which violate the conservation of strangeness

Charge Conjugation (C) Charge Conjugation (C) is the operation of changing a particle into its antiparticle. The strong and EM interactions are said to be invariant under charge conjugation. If, in the first interaction, A is scattered through a certain angle with a certain probability, then, in the second interaction, A is scattered through the same angle with the same probability provided, of course, the experimental conditions (initial energy, momentum, and spin) are the same.

C Non-Invariance : Weak The electron from μ- the tend to leave the decay site preferentially in the direction opposite to the spin direction of the μ- while the positrons from μ+ tend to leave preferentially in the same direction as the spin of the μ+. The decay is not invariant under charge conjugation.

Parity (P) The P Operator (P), works on x, p, L, S. P reverses the components of all true vectors. For example, the parity operation on radius and momentum vectors produces: Note that angular momentum is the product of two vectors so it does not get reversed by the parity operator: Spin is a form of angular momentum so it too does not change sign under the P.

Inv. Under P : Strong & EM, not Weak. Inv. case: if A + B → C + D, and P(A) = A’; P(B) = B’; P(C) = C’ then A’ + B’ → C’ + D’ Non-Inv. case: Non-Inv. case: neutrino itself P( )= Not found exists

CP Invariance Neutrino itself http://universe-review.ca/I15-25-CPviolation1.jpg

CP Violation K0 can transform into their antiparticles (in which each quark is replaced with the other's antiquark) and vice versa, but such transformation does not occur with exactly the same probability in both directions

Time Reversal (T) The T makes time run backwards. This reverses both momentum and spin and changes ingoing particles to outgoing and outgoing to incoming.

CPT Invariance Many physicists believe that all interactions must be CPT invariant. If this is true and it is also true that CP is violated in weak interactions, then T must also be violated in just the right way to make weak interactions CPT invariant.

Isospin Concept Multiplet Splitting and Charge. Examples of Hadron multiplets are: a doublet of nucleons and a triplet of pions. The members of a multiplet have the same strangeness, hypercharge, spin, baryon number, electron family number, and muon family number, but differ in charge and differ slightly in mass (about 5MeV differences in mass). It is believed that if electromagnetic interactions were turned off, the members of a multiplet would be identical. This hypothesis is born out by the study of nucleon-nucleon scattering where neutron-neutron scattering can be deduced from proton-proton scattering by “turning off the proton's charge" in the scattering equations. The algebra of isospin is exactly the same as for spin, which accounts for its name. It should be emphasized at the outset, however, that isospin is not spin. Spin exists in real space but isospin exists only in an abstract mathematical isospin space.

Isospin Calculations Each multiplet is assigned a isospin number I. Positive integer or half an odd positive integer. Isospin may be considered to be a vector with magnitude (I(I + 1))1/2 (compare with the spin vector of magnitude ћ (s(s + 1))1/2 .) To emphasize that isospin is not a vector in coordinate space, we will not call the axes x, y, z but rather 1, 2, 3. The 3 component, I3, may take on any one of the values I, I-1, I-2, …, -I in a fashion similar to the values of the z component of angular momentum. Each of these values corresponds to a different member of the multiplet with I3. I3 = I assigned to the particle with the most positive charge and I3= -I assigned to the particle with the most negative charge.

Isospin Calculations If a particle is in a state with definite I3 , the uncertainty principle prohibits it from having definite values of I1 or I2 so we ignore those components. Multiplicity. If the isospin of a multiplet is I, there are 2I + 1 particles in the multiplet. This result follows from counting the possible values of I3. Thus singlets have I = 0, doublets have I = 1/2, and triplets have I = 1. Later we shall run into a quartet (I = 3/2). Note that an antiparticle has the same value of I as the corresponding particle but its I3 has the opposite sign.

Isospin Calculations The magnitude of the total isospin is (I(I + 1))1/2 where I is a positive integer or half an odd positive integer and, for a given collection of particles, the maximum value I can have is the sum of the individual particle's I's: The value of I3 for a collection of particles is the sum of the individual particle's I3's: I must be greater than or equal to | I3 |. Thus I can have any one of the values Imax, Imax-1, Imax-2, …, | I3 |. For example if one considers π+p scattering: Iπ+ =1; Ip =1/2; Imax =3/2; I3π+ =1; I3p =1/2; I3 =3/2; so I=3/2 For π-p scattering: Iπ- =1; Ip =1/2; Imax =3/2; I3π- =-1; I3p =1/2; I3 =-1/2; so I=3/2 or 1/2

Isospin Conservation Relationship: Q, S, B, I3; Y, I3. Note that the signs of S, B, I3, and q are opposite for a particle and its antiparticle. Both I and I3 are conserved during strong interactions and decays. Since q, S, and B are conserved there, the conservation of I3 is not a new conservation law. For weak interactions neither S, I3, nor I need be conserved although q and B are universally conserved. For electromagnetic interactions, I need not be conserved.

Deducing Interactions from Decay Products If particles appear for which isospin is not defined (γ, leptons), then the interaction is not strong. If neutrinos appear, then the interaction must be weak. If photons appear, the interaction must be include electromagnetic. It is sometimes impossible to distinguish between weak and electromagnetic interactions on the basis of product particles alone. In particular, when C, P, or T violation occurs, the products may not show the violation (neutrinos, of course, do). What you are really doing is finding the dominant part of the interaction for the determination of lifetime.

More Example K+,Λ0,Ξ0,Ω- only decay by weak K+ is the lightest strange particle and a combination of the energy and strangeness conservation laws forces its decay to be weak. The Λ0 is the lightest strange baryon and conservation of energy, strangeness, and baryon number precludes its decay via the strong or electromagnetic interactions. The Ξ0, if it decayed strongly or electromagnetically, must decay to particles with a net strangeness of -2. Clearly, ΣΣ, ΛΛ, ΛΣ, ΣK meet energy conservation requirements. Two K's have less total mass and conserve strangeness and charge. However the products must include a baryon and all baryon have too much mass to join the kaons as decay products. The Ξ0, must decay weakly. In fact, the most probable decay is The Ω- also decays weakly can be predicted by invoking conservation of strangeness, energy and baryon number.

More Example As an example, consider the strong or electromagnetic decay of the Σ+. To conserve strangeness, which strong and electromagnetic decays require, the Σ+ must decay either to a Λ0 or a kaon, the only strange particles with less mass. Consider first the decay to a Λ0 . The other decay products must have net strangeness 0, total mass less than 73.8 MeV, and charge +1. These conditions can be met only if a positron appears among the products. Other products must have net charge 0, and electron family number +1. Only the electron's neutrino will do. Since a neutrino is required, parity invariance is violated and the decay cannot be strong or electromagnetic. Now consider the possibility of decay to a K0. Strangeness is conserved. Other products must have net charge +1, mass less than 695.6 MeV, and strangeness 0. In addition, at least one baryon must be involved. There is no baryon with mass less than 695.6 eV. Thus this decay cannot occur via the strong or electromagnetic interactions. The decay most often observed is

More Example S 1 -1 I ½ I3 -½ 3/2 or ½ This interaction conserves charge and baryon number. It can conserve angular momentum, energy, and momentum. It conserves strangeness. We conclude that isotopic spin could be conserved. So, barring violation of C, P, or T, the interaction is strong. S 1 -1 I ½ I3 -½ 3/2 or ½

Special case : sigma decay Σ0→Λ0+γ The decay of the Σ0. The products must include a single baryon (conservation of energy prohibits 2 baryons and an antibaryon). If the decay is to be strong the product particles must have strangeness =-1. This requirement leads to the conclusion that one of the products is either Λ0 or one of the anti-kaons. A kaon and any baryon together are too massive so the decay must be to a Λ0. Any other particles that could be produced must have total mass less than 76.9 MeV: i.e., photons, electrons, or neutrinos. We have determined that the decay products of Σ0 must be the Λ0 plus photons or leptons. Can this decay take place via the strong interaction? The Σ0 has isotopic spin 1 while the Λ0 has isotopic spin 0. All the other possible products (leptons and photons) have isotopic spin 0. We conclude that the decay cannot take place via the strong interaction. However all the conservation laws for the electromagnetic interaction do hold in fact the decay does not violate any conservation law we have discussed except isospin. The decay takes place via the electromagnetic interaction.

End

http://www.physnet.org/modules/pdf_modules.html