The Zoo of Subatomic Particles

Slides:



Advertisements
Similar presentations
Nuclear Physics UConn Mentor Connection Mariel Tader.
Advertisements

Varan Satchithanandan Mentor: Dr. Richard Jones.  explains what the world is and what holds it together  consists of:  6 quarks  6 leptons  force.
Nuclear Physics Part 1: The Standard Model
Leptons: There are 6 leptons (and their corresponding anti-leptons). One 1st generation lepton is the electron previously discussed. The electron.
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 III1 EM Decay of Hadrons If a photon is involved in a decay (either final state or virtual) then the decay is at least partially electromagnetic.
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.
Modern Physics LECTURE II.
8/5/2002Ulrich Heintz - Quarknet Particle Physics what do we know? Ulrich Heintz Boston University.
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.
The Standard Model An Introduction to Particle Physics
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.
THE STANDARD MODEL  What’s fundamental  What’s in a name.
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)
My Chapter 30 Lecture.
ParticleZoo. The Standard Model The body of currently accepted views of structure and interactions of subatomic particles. Interaction Coupling Charge.
Elementary Particles: Physical Principles Benjamin Schumacher Physics April 2002.
From Luigi DiLella, Summer Student Program
Fisica Generale - Alan Giambattista, Betty McCarty Richardson Copyright © 2008 – The McGraw-Hill Companies s.r.l. 1 Chapter 30: Particle Physics Fundamental.
1 FK7003 Lecture 6 ● Isospin ● SU(2) and SU(3) ● Parity.
Properties conserved in Strong and EM interactions
Dr. Bill Pezzaglia Particle Physics Updated: 2010May20 Modern Physics Series 1 ROUGH DRAFT.
Aim: How can we explain the four fundamental forces and the standard model? Do Now: List all the subatomic particles that you can think of.
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.
ParticleZoo. September 01 W. Udo Schröder: History NS 2 Nucleons Are Not Elementary Particles! p e-e- e-e- hadron jet Scatter high-energy electrons off.
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.
Quarknet Syracuse Summer Institute Strong and EM forces 1.
© John Parkinson 1 e+e+ e-e- ANNIHILATION © John Parkinson 2 Atom 1x m n n n n Nucleus 1x m U Quarks 1x m U D ? ? ?
The Nucleus Nucleons- the particles inside the nucleus: protons & neutrons Total charge of the nucleus: the # of protons (z) times the elementary charge.
Modern Physics. Reinventing Gravity  Einstein’s Theory of Special Relativity  Theorizes the space time fabric.  Describes why matter interacts.  The.
Introduction to CERN Activities
STANDARD MODEL class of “High Energy Physics Phenomenology” Mikhail Yurov Kyungpook National University November 15 th.
Lecture 2: The First Second Baryogenisis: origin of neutrons and protons Hot Big Bang Expanding and cooling “Pair Soup” free particle + anti-particle pairs.
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.
PARTICLE PHYSICS Summary Alpha Scattering & Electron Diffraction.
1 The Standard Model of Particle Physics Owen Long U. C. Riverside March 1, 2014.
What is the Standard Model of Particle Physics ???? 1. A theory of three of the four known fundamental interactions and the elementary particles that.
More on the Standard Model Particles from quarks Particle interactions Particle decays More conservation laws Quark confinement Spin.
Phy107 Fall From Last Time… Particles are quanta of a quantum field –Often called excitations of the associated field –Particles can appear and.
Particle Physics "three quarks for Muster Mark" -James Joyce (Finnegan’s Wake) Contents: Particle Accelerators Quantum Electrodynamics and Feynman diagrams.
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.
AS Particles Re-cap The stuff what you needs to know…
 All elementary particles in physics are classified as either fermions or bosons. Quantum physics demonstrates the particles may have an intrinsic non-zero.
The Standard Model of Particle Physics
The Standard Model An Introduction to 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?
Quarks Throughout the 1950 – 1960s, a huge variety of additional particles was found in scattering experiments. This was referred to as the “particle zoo”.
Advanced Topics Nuclear Physics ElementaryParticles General Relativity
Standard Model of Particles
Particle Physics what do we know?
Section IX - Quark Model of Hadrons
PHYS 663 Advanced Particles Physics
Particle physics.
ELEMENTARY PARTICLES.
The Color Charge & Bag Model
The Standard Model By: Dorca Lee.
Introduction to Particle Physics
PHYS 3446 – Lecture #23 Standard Model Wednesday, Apr 25, 2012
Physics 4 – April 18, 2019 Agenda:
Particle Physics and The Standard Model
Presentation transcript:

The Zoo of Subatomic Particles ParticleZoo The Zoo of Subatomic Particles The Standard Model of Quarks and Leptons

Nucleons Are Not Elementary Particles! Scatter high-energy electrons off protons. If there is no internal structure of e- or p, then well-defined “elastic” e- energy for each angle. See structure!! p e- hadron jet excited states of the proton Each line in the energy spectrum of scattered electrons corresponds to a different energy state of the proton. Bartel etal. PL28B, 148 (1968) scatter probability energy of scattered electron ground state of the proton elastic x1/8.5

The Quark Model The quark model represents a relatively simple picture of the internal structure of subatomic particles and makes predictions of their production and decay. It uses a minimum of adjusted quark parameters and has great predictive power, e.g., for the composite-particle masses, magnetic moments, and lifetimes. There are no contradictions to this model known so far, (but many questions remain).

Internal Nucleonic Structure p e- The proton has internal structure, so-called quarks (u,u,d). Quarks combine to nucleon states of different excitations. Proton is the (u,u,d) ground state N D S=½ S=3/2 1200 MeV N: one doublet with a splitting of only Dm = 1.3 MeV D: one quadruplet with a splitting of only Dm = 8 MeV 938 MeV p S=0 Mesons 135 MeV

The Quark-Lepton Model of Matter Explains the consistency of the known particles in all of their states. 3 families of quarks (3 “colors” each) and associated leptons. All are spin-1/2 particles, quarks have non-integer charges Mesons (q, q-bar) q-bar:anti-quark Nucleons (q,q,q)

1 2 3 4 Spin ½ ½ 3/2 0 1 Leptons Baryons Mesons Hadrons m t X S L N W X*Y* D hK p K*w r 8 10 J/Y Y' Y'’ Mass (GeV/c2) n, e Particle Spectrum Simplified scheme of stable or unstable subatomic particles. Families have different interactions, Leptons: weak+elm, Hadrons: weak+elm+strong Each particle also has an anti-particle, with inverse quantum numbers. “strange”

Quark Quantum Numbers All: spin=1/2, baryon number B=1/3 Q/e M/GeVc-2 Flavor Q/e M/GeVc-2 T T3 S C B* Top u +2/3 0.005 ½ d -1/3 0.009 - ½ s 0.175 -1 c 1.5 1 b 4.9 t 162 T,T3: isospin; S: strangeness; C: charm; B*: bottom qu.#, Top: top qu.#

Structure of Composite Particles There are only 3-quark (q,q,q)  Baryons and quark-antiquark configurations. No free quarks or higher quark multiplicities. _d _u _s u d s quarks antiquarks s= 1/2 Baryon Octet s= 0 Meson Nonet _s d _u s u _d T3 d u s d n p S- S0 L0 S+ X- X0 p- K0 K+ K- _K0 p0 h h’ p+ S

Baryon Decuplet s = 3/2 d u s D- D0 D+ D++ S*- S*0 S*+ X*- X*0 W- S T3

Meson Wave Functions Examples to interpret the graphic shorthand in these figures: Meson spins are integer, vector sum of half-integer quark and anti-quark spins, and their integer orbital angular momentum l. In ground state, mostly l =0.

Baryon Wave Functions Examples to interpret the graphic shorthand: These Baryon and Meson wave functions are schematic, do not have proper (anti-)symmetry property required by Pauli Principle: The total particle wave function must be antisymmetric under quark exchange (quarks are fermions)

Pauli Principle and Color Coordinate Quarks are Fermions  no two same quarks can be in the same state d D- u D++ s3,T3 have both 3 identical fermions (same quarks) with same spins (S=3/2) and isospin (T3=+3/2) states Violates Pauli Principle !? Conclusion: There must be an additional quantum number (degree of freedom), “color”. Need 3 colors and their anti-colors Color and complementary color (anti-color) add up to color-less (white) d _d d quarks anti-d quarks

Color Wave Function d _d d quarks anti-d quarks D++ : Flavor and spin configurations symmetric, spatial configuration symmetric (no orbital angular momentum, l =0)  color configuration must be antisymmetric. All colors are present with equal weights. All physical particles are “white.” Necessity of color rules out combinations such as There are no free quarks  Confinement

Gluons Bound quark systems (physical particles) by q-q interactions. Field quanta: 8 Gluons (not actually pions!) Spin and parity 1- like a photon. Gluons carry color and the corresponding anticolor. Color can be transferred but particle remains colorless. _q qc’ q qc gluon emission q-qbar creation self coupling changes color of the color charges Usual conservation laws apply to reactions between quarks.

Gluon Exchange Gluons are exchanged back and forth between q-q, time u _d r b g _r _b _g p+ _ r,b _ b,g u r b g _ b,g _ r,g d p Gluons are exchanged back and forth between q-q, changing q colors and momenta dynamically r, g, and b are visited with equal probability

Baryon Production with Strong Interactions Typically: Energetic projectile hits nucleon/nucleus, new particles are produced. Rules for strong interactions: Energy, momentum, s, charge, baryon numbers, etc., conserved q existing in system are rearranged, no flavor is changed q-q-bar pairs can be produced u d _d s _s time  u p S+ p+ K+ annihilation creation d, d-bar s, s-bar

Baryon Resonances Typically: Energetic projectile hits nucleon/nucleus, intermediate particle is produced and decays into other particles. u u d _ d u time  p p+ D++ produced as short-lived intermediate state, t = 0.5·10-23s corresp. width of state: G = ħ/t = 120 MeV This happens with high probability when a nucleon of 300 MeV/c, or a relative energy of 1232 MeV penetrates into the medium of a nucleus.  Resonance u u u D++

Confinement and Strings Why are there no free quarks? Earlier: symmetry arguments. Property of gluon interaction between color charges (“string-like character). Q: Can one dissociate a qq pair? energy in strings proportional to length 0.9GeV/fm field lines: color strings successive q/q-bar creation, always in pairs!

Leptons Leptons have their own quantum number, L, which is conserved. It seems likely, but is not yet known, whether electronic, muonic and tau lepton numbers are independently conserved in reactions and decays.

Quantum numbers are additive. Conservation Laws Quantum numbers are additive. Anti-quarks have all signs of quark quantum numbers reversed, except spin and isospin. Derived quantities: In a reaction/transmutation, decay, the following quantities are conserved (before=after): The total energy, momentum, angular momentum (spin), The total charge, baryon number, lepton number

Conservation Laws in Decays A  B + C possible, if mAc2 ≥ mBc2 + mCc2 Otherwise, balance must be supplied as kinetic energy. Example: Conservation of charge, baryon number, lepton number in neutron decay.

Weak Interactions Weak bosons can change quark flavor 10-5 weaker than strong interaction, small probabilities for reaction/decays. Mediated by heavy (mass ~100GeV) intermediate bosons W± ,Z0. Weak bosons can change quark flavor d u u Z0 W+ W- u s u up-down strange-non-strange no flavor change conversion conversion carries +e carries –e carries no charge

Decays of W± and Z0 Bosons Hadronic decays to quark pair are dominant (>90%), leptonic decays are weak. All possible couplings:

Examples of Weak Decays Can you predict, which (if any) weak boson effects the change? p _ne p ne e- n m- ? ? ? time n p n nm e- n-decay? neutrino scattering neutrino-induced off protons? reaction off e-?

Examples of Weak Decays Answer: Yes, all processes are possible. These are the bosons, p _ne ne e- p n m- W- Z0 W+ time n p n nm e- n-decay neutrino scattering neutrino-induced off protons reaction off e- Method: Balance conserved quantities at the vortex, where boson originates. Remember W± carries away charge ±|e|. Balance conserved quantities at lepton vortex.

Particle Production In electron-positron collisions, particle-anti-particle pairs can be created out of collision energy, either via electromagnetic or weak interaction. probability  collision energy (GeV) anti-fermion fermion m- m+ m- m+ Z0 g Z0 e- e- e+ e- e+ e+ electromagnetic weak example

The Standard Model Interactions The body of currently accepted views of structure and interactions of subatomic particles. Interactions Interaction Coupling Charge Field Boson Mass/GeVc-2 Jp strong color gluons (8) 1- elmgn electric (e) photon (g) weak W+, W-, Z0 100 1 Weak interactions violate certain symmetries (parity, helicity) see later Particles Fermions Family Q/e Color Spin Weak Isospin Quarks u c t d s b +2/3 -1/3 r, b, g ½ Leptons ne nm nt e m t -1 none

The Standard Model ct’d Combine weak and elm interactions “electro-weak” Type of isospin-symmetry: same particles carry weak and elm charge. Vqq r 1 fm Force range Electromagnetic: ∞ Weak: 10-3fm Strong qq force increases with distance 2mqc2 There are no free quarks. All free physical particles are colorless.

The End