Quantum numbers.

Slides:



Advertisements
Similar presentations
3224 Nuclear and Particle Physics Ruben Saakyan UCL
Advertisements

Properties and Decays of Heavy Flavor S-Wave Hadrons Rohit Dhir Department of Physics, Yonsei University, Seoul Dated:11 th June, 2012.
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:
Why we believe there’s a strong force. Why Colour? –Why not something with no inappropriate mental imagery Probing the Colour Force –The study of simple.
Symmetries By Dong Xue Physics & Astronomy University of South Carolina.
PH 301 Dr. Cecilia Vogel Lecture 19. Review Outline  conservation laws  hadrons, baryons, mesons  flavor and color  quarks and leptons  matter and.
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.
C4 Lecture 3 - Jim Libby1 Lecture 3 summary Frames of reference Invariance under transformations Rotation of a H wave function: d -functions Example: e.
Spin and addition of angular momentum
Nuclear de-excitation Outline of approach… Source of radiation Propagation of radiation field Detection of radiation ?? nucleus.
Particle Physics J1 Particles and Interactions. Particle Physics Description and classification State what is meant by an elementary particle (no internal.
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.
Chapter 41 Atomic Structure
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.
Lecture 10: Inelastic Scattering from the Proton 7/10/2003
Physics for Scientists and Engineers, 6e Chapter 46 - Particle Physics and Cosmology.
Elementary Particles: Physical Principles Benjamin Schumacher Physics April 2002.
From Luigi DiLella, Summer Student Program
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.
P Spring 2003 L9Richard Kass Inelastic ep Scattering and Quarks Elastic vs Inelastic electron-proton scattering: In the previous lecture we saw that.
Spin Electronic charge in motion - A current loop behaves as a magnetic dipole and has a magnetic moment. - Note the current direction is opposite to the.
6.852: Distributed Algorithms Spring, 2008 April 1, 2008 Class 14 – Part 2 Applications of Distributed Algorithms to Diverse Fields.
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
Properties conserved in Strong and EM interactions
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.
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.

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.
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.
Lecture 4 – Quantum Electrodynamics (QED)
 All elementary particles in physics are classified as either fermions or bosons. Quantum physics demonstrates the particles may have an intrinsic non-zero.
PHYS 3446 – Lecture #10 Nuclear Radiation Energy Deposition in Media
Lecture 7 Parity Charge conjugation G-parity CP FK7003.
Handout 3 : Interaction by Particle Exchange and QED
Chapter V Interacting Fields Lecture 1 Books Recommended:
Chapter 41 Atomic Structure
Countries that signed the nuclear arms treaty with Iran
Handout 9 : The Weak Interaction and V-A
The Standard Model strong nuclear force electromagnetic force
Section VI - Weak Interactions
Spin and Magnetic Moments
Chapter 4 Quantum Mechanics in 3D.
Announcements Exam Details: Today: Problems 6.6, 6.7
Advanced Topics Nuclear Physics ElementaryParticles General Relativity
Chapter 9 Spin.
Standard Model of Particles
Spin and Magnetic Moments (skip sect. 10-3)
Quantum Two.
Section IX - Quark Model of Hadrons
Elementary Particles.
Chapter 41 Atomic Structure
Section VII - QCD.
PHYS 3446 – Lecture #10 Nuclear Radiation Energy Deposition in Media
PHYS 3446 – Lecture #20 Elementary Particle Properties
Handout 4 : Electron-Positron Annihilation
LECTURE 15.
PHYS 3446 – Lecture #20 Monday ,April 16, 2012 Dr. Brandt Accelerator
PHYS 3446 – Lecture #23 Standard Model Wednesday, Apr 25, 2012
Physics 3313 – Review 2 Wednesday May 5, 2010 Dr. Andrew Brandt
PHYS 3446 – Lecture #14 Elementary Particle Properties
The Quantum-Mechanical Hydrogen Atom
PHYS 3446 – Review Review Note Test deferred until Weds.
Particle Physics and The Standard Model
Presentation transcript:

Quantum numbers

Electric charge Q

Barion Number B

Lepton Number

Barion-lepton conservation Gauge invariance  conservation law (i.e. charge) In field theories with local gauge simmetry: absolutely conserved quantity implies long-range field (i.e Em field) coupled to the charge If baryon number were absolutely conserved (from local gauge simmetry), a long-range field coupled to it should exist. No evidence for such a field! However: charge conservation lepton conservation baryon conservation

Highest limits are on the lepton and baryon nr conservation, even if not protected by any gauge principle Other reasons for baryon non-conservation: huge baryon-antibaryon asimmetry in the Universe (NB today  1079!) For practical purposes, we will assume that baryon and lepton nr are conserved, even if there is no deep theoretical reasons to suppose this conservation rule as absolute. While total lepton number seems to be conserved, weak transition between leptons of different flavours (e.g.: ne  nm ) can be possible (see: experiments on neutrino oscillations)

Spin S W. Pauli introduced for the 1st time a fourth quantic number - the spin - to completely describe the electron state inside the atomic orbitals No physics meaning was assigned to the spin until 1927, when the experiment of Phipps ad Taylor associated to the spin a magnetic moment of the electron. The electron spin can assume only two values: +1/2 and –1/2: it is an intrinsic attribute of the electron and it appears only in a relativistic scenario Later, it was possible to attribute the spin to other particles (m, p e n) by applying the law of the angular momentum conservation or the principle of the detailed balance

Spin and cross sections Suppose the initial-state particles are unpolarised. Total number of final spin substates available is: gf = (2sc+1)(2sd+1) Total number of initial spin substates: gi = (2sa+1)(2sb+1) One has to average the transition probability over all possible initial states, all equally probable, and sum over all final states  Multiply by factor gf /gi All the so-called crossed reactions are allowed as well, and described by the same matrix-elements (but different kinematic constraints)

Good quantum numbers: if associated with a conserved observables (= operators commute with the Hamiltonian) Spin: one of the quantum numbers which characterise any particle (elementary or composite) Spin Sp of the particle, is the total angular momentum J of its costituents in their centre-of-mass-frame Quarks are spin-1/2 particles  the spin quantum number Sp = J can be integer or half integer The spin projection on the z-axis – Jz- can assume any of 2J+ 1 values, from –J to J, with steps of 1, depending on the particle’s spin orientation

Illustration of possible Jz values for Spin-1/2 and Spin-1 particles It is assumed that L and S are “good” quantum numbers with J = Sp Jz depends instead on the spin orientation Using “good”quantum numbers, one can refer to a particle using the spectroscopic notation (2S+1)LJ Following chemistry traditions, instead of numerical values of L = 0,1,2,3.....letters S,P,D,F are used

In this notation, the lowest-lying (L=0) bound state of two particles of spin-1/2 will be 1S0 or 3S1 - For mesons with L >= 1, possible states are: - Baryons are bound states of 3 quarks  two orbital angular momenta connected to the relative motions of quarks - total orbital angular momentum is L = L12+L3 - spin of a baryon is S = S1+S2+S3  S = 1/2 or S = 3/2

Internal orbital angular momenta of a 3-quarks state Possible baryon states:

Parity P

The intrinsic parities of e- and e+ are related, namely: Pe+Pe- = -1 This is true for all fermions (spin-1/2 particles): Pf+ Pf- = -1 Experimentally this can be confirmed by studying the reaction: e+e- gg where initial state has zero orbital momentum and parity of Pe+Pe If the final state has relative orbital angular momentum lg, its parity is: Pg2(-1)lg Since Pg2=1, from the parity conservation law: Pe+Pe- = (-1)lg Experimental measurement of lg confirm this result

Consequently, parities of anti-leptons have opposite sign - However, it is impossible to determine Pe- or Pe+,since these particles are created or destroyed in pairs Conventionally, defined parities of leptons are: Pe- = Pm- = Pt- = 1 Consequently, parities of anti-leptons have opposite sign Since quarks and anti-quarks are also created only in pairs, their parities are also defined by convention: Pu = Pd = Ps = Pc = Pb = Pt = 1 With parities of antiquarks being –1 For a meson parity is calculated as: For L=0 that means P = -1, confirmed by observations.

For a baryon B=(abc), parity is given as: and for antibaryon as for leptons For the low-lying baryons, the formula predicts positive parities (confirmed by experiments). Parity of the photons can be deduced from classical field theory, considering Poisson’s equ. Under a parity transformation, charge density changes as and changes its sign  to keep the equation invariant, E must transform as: The em field is described by the vector and scalar potential:

- For photon, only the vector part correspond to the wavefunction: Under the parity transformation, And therefore: It can be concluded for the photon parity that: Strange particles are created in association, not singly as pions Only the parity of the LK pair, relative to the nucleon can be measured (found to be odd) By convention: PL = +1, and PK = -1