Particle Physics "three quarks for Muster Mark" -James Joyce (Finnegan’s Wake) Contents: Particle Accelerators Quantum Electrodynamics and Feynman diagrams.

Slides:



Advertisements
Similar presentations
Garfield Graphics included with kind permission from PAWS Inc. All Rights Reserved. Exchange Particles.
Advertisements

Going Smaller than Atoms AQA Syllabus A A Level Physics – Module 2 © T Harrison. The National School.
Garfield Graphics included with kind permission from PAWS Inc. All Rights Reserved. Strange Particles AS level Notes.
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.
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.
Charged Particles. Nuclear Physics Charged particles can come from nuclear decay. Nuclear physics figures into particle detection. Use terminology from.
University of Birmingham Master class,23rd April 2008 Ravjeet Kour Journey into the heart of matter Introducing Particle Physics.
Chapter 43 Elementary Particles
Modern Physics LECTURE II.
Feynman Diagrams Rosie Cavalier 2012 Edited by Mr Catchpole 2014.
8/5/2002Ulrich Heintz - Quarknet Particle Physics what do we know? Ulrich Heintz Boston University.
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.
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.
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.
Chapters 9, 11, 12 Concepts covered that will also be candidates for exam questions.
Particle Physics Revision The Whole Lot. Announcements Physics revision tonight. Room C56 tomorrow morning. Mock Exams next Wednesday. Potential Divider.
Elementary Particles: Physical Principles Benjamin Schumacher Physics April 2002.
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
Finishing things up. So what’s with that 14 C? Masses of isotopes (not “natural” stuff) truly are multiples of basic hydrogen. Hydrogen is positively.
Jeopardy Jeopardy PHY101 Chapter 12 Review Study of Special Relativity Cheryl Dellai.
Short-Lived Resonance States. Forces and Fields Since 1932, the number of fundamental particles has increased enormously, and the description of these.
Fisica Generale - Alan Giambattista, Betty McCarty Richardson Copyright © 2008 – The McGraw-Hill Companies s.r.l. 1 Chapter 30: Particle Physics Fundamental.
Dr. Bill Pezzaglia Particle Physics Updated: 2010May20 Modern Physics Series 1 ROUGH DRAFT.
Particles and how they interact
© 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 ? ? ?
Subatomic Particles Lesson 10. Objectives describe the modern model of the proton and neutron as being composed of quarks. compare and contrast the up.
The Nucleus Nucleons- the particles inside the nucleus: protons & neutrons Total charge of the nucleus: the # of protons (z) times the elementary charge.
Fundamental principles of particle physics G.Ross, CERN, July08.
Atomic Physics – Part 3 Ongoing Theory Development To accompany Pearson Physics PowerPoint presentation by R. Schultz
Modern Physics. Reinventing Gravity  Einstein’s Theory of Special Relativity  Theorizes the space time fabric.  Describes why matter interacts.  The.
Phys 102 – Lecture 28 Life, the universe, and everything 1.
A photon with a wavelength of 2
Take out hwk & tables. Compare answers to hwk sets.
What makes up the nucleus? Nucleus is positively charged Different atoms have same electrical properties but different masses Isotopes – same atomic number,
Particle Physics Why do we build particle accelerators? The surface is flat Still flat Oh no its not Big balls cannot detect small bumps.
Phy107 Fall From Last Time… Particles are quanta of a quantum field –Often called excitations of the associated field –Particles can appear and.
The Theory of (Almost) Everything Standard Model.
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.
Nuclear Energy and Elementary Particles. Atoms Atoms From the Greek for “indivisible” From the Greek for “indivisible” Were once thought to the elementary.
NUCLEAR ENERGY. The daughter nuclei in the reaction above are highly unstable. They decay by beta emission until they reach stable nuclei.
P ARTICLE P HYSICS A brief intro to the quantum world of particles.
7.3 The Structure of Matter
Units of E are typically eV and units of λ are typically nm Units of E are typically eV and units of λ are typically nm. Using the hc = 1240.
Standard Model for Sub-atomic Particles
The Standard Model of Particle Physics
Lecture 04 - Hadrons Quarks multiplets Hadron decays Resonances
The Standard Model strong nuclear force electromagnetic force
Particle Placemat.
Aim: How can we describe Fundamental Particles?
Elementary particles Spring 2005, Physics /24/2018 Lecture XXV.
The Mysterious Nucleus
Search for Order Ancient Greeks: Aristotle Earth Air Fire Water
Particle Physics what do we know?
The Mysterious Nucleus
Particle Physics Part 1 -James Joyce Contents: Particle Accelerators
Particle physics.
Elementary Particles.
Particle Physics and The Standard Model
ELEMENTARY PARTICLES.
Particle Physics Part 2 -James Joyce Contents: Conservation Laws
Standard Model Review 2019.
PHYS 3446 – Lecture #20 Monday ,April 16, 2012 Dr. Brandt Accelerator
Modern Studies of the Atom
Physics 4 – April 18, 2019 Agenda:
Particle Physics and The Standard Model
Presentation transcript:

Particle Physics "three quarks for Muster Mark" -James Joyce (Finnegan’s Wake) Contents: Particle Accelerators Quantum Electrodynamics and Feynman diagrams The Yukawa Particle Particles and Antiparticles Conservation Laws Types of Particles Strange Things and Quark Theory

Particle Accelerators TOC Basic concept - Vq = 1 / 2 mv 2 Provide energy for nuclear reactions Create particles from energy Proton Source Vacuum Beam Steering (RevereWare) Experiments +150,000 V

Particle Accelerators TOC SLAC - electron accelerator Potential switches 50 GeV - mass?

Particle Accelerators TOC Cyclotrons - In a magnetic field to curve path Potential switches Mass dilates as v->c Synchrotrons - Fermilab(1.0 km), CERN (8.5 km)

8.5 km in diameter

Quantum Electrodynamics TOC Coulomb’s law - Force fields Richard Feynman - EM forces are mediated by photons: Richard Feynman Feynman Diagram Virtual photons:  E  t > h / 2  (Exist for so short a time - never detected)

The Yukawa Particle TOC Photons mediate the EM force Yukawa proposes a particle to mediate strong nuclear force Hideki Yukawa He names it the meson - (between electron and proton)  E  t =  E( d / c ) = h / 2   E = hc / 2  d = 130 MeV

The Yukawa Particle TOC Hideki Yukawa Muon discovered in cosmic radiation m = 106 MeV - doesn’t interact The pi meson (pion) is discovered in 1947 in cosmic rays (3 charge states):  MeV/c 2  o MeV/c 2  MeV/c 2 p + p --> p + p +  o p + p --> p + n +  + (conservation of charge)

The Four Forces of Nature TOC Type Strong Nuclear Electromagnetic Weak Nuclear Gravitational Relative Strength Field Particle Gluons (mesons) Photon W + and Z o Graviton?

Particles and Antiparticles TOC NameParticleAntiparticle Electrone - e + p Protonpp Pion  +  - Some particles have no antiparticle + and - are electron charges When particle meets antiparticle - annihilation (rest mass + E k turns to energy or other particles)

Selected list (there are hundreds of hadrons) Self as antiparticle + and - are electron charges….

Conservation Laws - Baryon Number TOC Conservation of charge Conservation of mass/energy Conservation of nucleon.... In general, baryon number is conserved:

Conservation Laws - Baryon Number TOC In general, baryon number is conserved: This reaction can never happen: p + n -> p + p + p (Antiparticles have B = -1) Baryon numbers: 

Conservation Laws - Baryon Number TOC Heavy baryons decay to lighter ones Proton is lightest - must be stable

Whiteboards: Conservation of Baryon Number 11 | 2 | 3 | 4234 TOC

W 0 What is the total Baryon number of p + n + n +  = 0

What is the total Baryon number of  + +  + +  o +  = -1 W

yes Can this reaction occur? p + p --->  - +  = W

no Can this reaction occur? p + n --->  o +   W

no Can this reaction occur?  o + n --->  o +  + B: = C: != W

Conservation Laws - Lepton Number TOC Lepton number is conserved too L e - Electron/electron neutrino L  - Muon/muon neutrino L  - Tau/Tau neutrino Remember - anti particles have negative lepton numbers Neutrinos are believed to have mass

Conservation Laws - Lepton Number TOC Co Ni +  - + e 13 7 N 13 6 C +  + + e Beta Decay: Emission of an electron neutrino allowed L e to be conserved: L e L  L  Electrone-+100 Neutrino (e) e +100 Muon  Neutrino (  )  0+10 Tau  Neutrino (  )  00+1

Whiteboards: Conservation of Lepton Number 11 | 2 | 3 | 4 | TOC

W dog biscuit Does this decay occur?  - ---> e - + e Charge is conserved L e : 0 = L  : 1  L  is not conserved L e L  L  Electrone-+100 Neutrino (e) e +100 Muon  Neutrino (  )  0+10 Tau  Neutrino (  )  00+1

yo mama Does this decay occur?  - ---> e - + e +  Charge is conserved L e : 0 = L  : 1 = Yes it occurs W L e L  L  Electrone-+100 Neutrino (e) e +100 Muon  Neutrino (  )  0+10 Tau  Neutrino (  )  00+1

the red Does this decay occur?  - ---> e + e +  Charge is Not conserved L e : 0 = L  : 1 = Does not occur W L e L  L  Electrone-+100 Neutrino (e) e +100 Muon  Neutrino (  )  0+10 Tau  Neutrino (  )  00+1

 What is the missing decay product?  - --->  - +  + ??? W L e L  L  Electrone-+100 Neutrino (e) e +100 Muon  Neutrino (  )  0+10 Tau  Neutrino (  )  00+1 Q: -1= ? EL#: 0 = ? ML#: 0= ? TL#: 1 = ?

e+ What is the missing decay product?  + ---> ?? +  + e Q: +1=? EL#: 0 = ? ML#: -1= ? TL#: 0 =? W L e L  L  Electrone-+100 Neutrino (e) e +100 Muon  Neutrino (  )  0+10 Tau  Neutrino (  )  00+1

 What is the missing decay product?  + --->  + + ?? +  W L e L  L  Electrone-+100 Neutrino (e) e +100 Muon  Neutrino (  )  0+10 Tau  Neutrino (  )  00+1 Q: +1=+1 +? +0 EL#: 0 = 0 + ? +0 ML#: 0= -1 + ? +0 TL#: -1 =0 + ? +-1

-- What is the missing particle? ?? ---> e- + e +  W L e L  L  Electrone-+100 Neutrino (e) e +100 Muon  Neutrino (  )  0+10 Tau  Neutrino (  )  00+1 Q: ?= EL#: ? = ML#: ?= TL#: ? =

Types of Particles TOC Gauge Bosons - carry the electro-weak force Leptons - interact via weak and EM (charged) force Hadrons - interact via strong nuclear force Mesons - B = 0 Baryons - B = 1, (-1)…

Quark Theory TOC 1960s - Only 4 Leptons, but Hundreds of Hadrons Leptons seemed elementary/small (< m) Not all Hadrons could be elementary Murray Gell-Mann suggests that Hadrons are made from quarks.quarks "three quarks for Muster Mark" -James Joyce (Finnegan’s Wake)

Quark Theory TOC Murray Gell-Mann suggests that Hadrons are made from quarks.quarks

Quark Theory TOC Proton: +1 charge, B = 1 Neutron: 0 charge, B = 1 Pion + : +1 charge, B = 0 Pion-: -1 charge, B = 0 Kaon-: -1 charge, B = 0 Try making other Hadrons yourself

Truly Fundamental particles TOC Generally accepted fundamental particles Three generations Top quark = 200 GeV/c 2