SlideShare une entreprise Scribd logo
1  sur  25
Particles

                             Classification of Particles
                               Hadrons and Quarks
                                      Leptons

Thursday, 08 December 2011
The Stanford linear accelerator
In 1968 the Stanford accelerator shot a beam of 20 GeV electrons on a
   target. The results showed clearly that the electrons were strongly
   scattered by stationary protons and sometimes even bounced
   backward.




                                          q
                                                q

                                          q
The Stanford linear accelerator
Does that remind you of another famous experiment? What can be
  deduced about the internal structure of the proton?
The outcomes of the experiment resemble Rutherford’s experiment that
  led to the discovery of the nucleus.
The proton must be made up of sub-nuclear particles, some of which
  carry negative charge. This provides proof for the existence of quarks.
The Structure of a Proton
These results pointed at a structure of nucleons like the proton as being
  made up of three sub-nuclear particles called Quarks.




                                           q
                                                 q

                                           q
Classifying Particles
All particles can be classified in three main categories:

•   Hadrons  made up of quarks. They are affected by strong forces
•   Leptons  fundamental particles, i.e. they don’t have an internal
    structure. In other words, they are not made up of smaller particles
    and are not affected by strong forces.
•   Quarks  smaller particles that combine to form hadrons. They
    carry fractional charges (fractions of the charge of the electron).


So, what is everything made of?
•   Quarks and Leptons
1st       • up (u)  +2/3
generation   • down (d)  -1/3




       2nd       • charm (c) +2/3
    generation   • strange  -1/3




   3rd       • top (t)  +2/3
generation   • bottom (b)  -1/3
• electron (e-)  -1
   1st
generation   • electron neutrino
               ( e)  0



                 • muon ( -) -1
       2nd
    generation   • muon-neutrino
                   ( ) 0



             • tau ( -)  -1
   3rd
generation   • Tau-neutrino ( )
               0
• Pions:   0=(uu) or dd
                           += (ud)
Meson       (1             -= (ud)
quark + 1 anti-
   quark)         • Kaons: 0 (ds)
                            + (us)
                            - (us)




  Baryons          • Proton (uud) +1
 (3 quarks)        • Neutron (udd) 0
Lego Particles
Up quark (+2/3)        Anti-up quark (+2/3)


Down quark (-1/3)      Anti-Down quark (-
                       1/3)

Strange quark (-1/3)   Anti-Strange quark (-
                       1/3)


Electron (-1)          Positron (+1)
Neutrino (0)           Anti-Neutrino (0)

Muon (-1)              Anti-moun (+1)
Fundamental particles
A proton is made of two Up quarks and one down. Show that the sum of
   the three charges gives +1.
+2/3 + 2/3 – 1/3 = +3/3 = +1
                                        u
                                    d       u


A neutron is made of two down quarks and one up quark. Show the
   neutrality of this distribution.
-1/3 – 1/3 + 2/3 = -2/3 + 2/3 = 0
                                        d
                                    d       u
Lepton Number
All leptons have an additional property called Lepton Number. The
   lepton number is always conserved.


                 Particle               Lepton Number

         All leptons                           +1

         All anti-leptons                       -1

         Hadrons
                                                0
         (baryons and mesons)
-   Decay and lepton number
Explain why both an electron and an anti-neutrino must be formed in a
    - decay.




                   n          p e                      e

• The lepton number must be conserved.
• e- lepton no = +1      +1 – 1 = 0  an electron and an anti-
                            neutrino must be created for lepton
•   e lepton   no = -1      number to be conserved
Properties of quarks
Quarks and anti-quarks have some properties that you might not have
  encountered before:
• Relative Charge  all quarks and anti-quarks carry a charge which is
  a fraction of the charge of the electron, i.e. 1.6 x 10-19 C. In all
  interactions charge must be conserved.
• Baryon Number  all quarks and anti-quarks have a baryon number.
  The baryon number is +1/3 for quarks and -1/3 for all anti-quarks. In
  all interactions baryon number must be conserved.
• Strangeness  all quarks and anti-quarks have strangeness = 0 apart
  from the strange quark (strangeness = -1) and the anti-strange quark
  (strangeness = +1). In all interactions involving the STRONG FORCE
  strangeness must be conserved, but in weak interactions strangeness
  can be conserved, or change by ±1.
Properties of quarks
                                           Baryon
                Name         Symbol Charge        Strangeness
                                           Number
                  up           u     +2/3   +1/3       0
Quarks




                 down          d     -1/3   +1/3       0

                strange        s     -1/3   +1/3       -1
Anti-quarks




                anti-up        u     -2/3   -1/3       0

              anti-down        d     +1/3   -1/3       0

              anti-strange     s     +1/3   -1/3       +1
Mesons and Quarks
A K+ meson is made up of an up quark and an anti-strange quark. Work
   out the relative charge, baryon number and strangeness of this
   particle.
• Charge +2/3 + 1/3 = +3/3 = +1
• Baryon no  +1/3 – 1/3 = 0
• Strangeness  0 + 1 = +1


                                   s
                               u
Mesons and Quarks
A   - meson is made up of an anti-up quark and a down quark. Work out
    the relative charge, baryon number and strangeness of this particle.
• Charge -2/3 - 1/3 = -3/3 = -1
• Baryon no  +1/3 – 1/3 = 0
• Strangeness  0 – 0 = 0



                                    u
                                d
Change of Quarks in                     -   Decay
In a - decay one quark in the neutron changes character (flavour) to
   form a proton. Complete the diagram with the correct quarks in the
   proton.
                   proton
                              After
                    u du
                                    e-    e

                                W



                   u dd      Before
                  neutron
A down quark in the neutron changes into an up quark, emitting an
   electron and an anti-neutrino.
Stable and Unstable Baryons
In a - decay one quark in the neutron changes character (flavour) to
   form a proton. But why does that happen?
• The proton is the only stable Baryon.
• All other Baryons eventually decay into a proton.
• So, it is not surprising that in “nature” the neutron decays into a
  proton releasing an electron and an anti-neutrino.
Change of Quarks in                    +   Decay
In a - decay one quark in the neutron changes character (flavour) to
   form a proton. Complete the diagram with the correct quarks in the
   proton and the neutron.
                 neutron     After
                  u dd
                                  e+      e

                                W



                   u du      Before
                  proton
An up quark in the neutron changes into an down quark, emitting a
  positron and a neutrino.
Conservation Laws
In all particle interactions these conservation laws apply and must be
   fulfilled for the interaction to happen:
• Conservation of Charge  In all interactions charge must be
  conserved. So, Sum of Charges before = Sum of Charges after
• Conservation of Baryon Number  In all interactions baryon
  number must be conserved.
• Conservation of Strangeness  In all interactions involving the
  STRONG FORCE strangeness must be conserved, but in weak
  interactions strangeness can be conserved, or change by ±1.
• Conservation of Lepton Number  In all interactions the lepton
  number must be conserved.
Conservation Laws
Applying the conservation laws, show whether the following
  interactions are possible or not.


 Answer                n       p e        e


 Answer                         e    e

 Answer                n       p e        e


 Answer                    n   e
Answer
                         n         p e    e


This reaction can occur because:
• Charge is conserved  Before: 0        After: +1 – 1 + 0 = 0
• Baryon no is conserved  Before: +1    After: +1 + 0 + 0 = +1
• Lepton no is conserved  Before: 0     After: 0 + 1 - 1 = 0
• Strangeness is conserved  Before: 0   After: 0
Answer
                                   e     e

This reaction can occur because:
• Charge is conserved  Before: 0            After: -1 + 1 = 0
• Baryon no is conserved  Before: 0         After: 0 + 0 = 0
• Lepton no is conserved  Before: 0         After: +1 - 1 = 0
• Strangeness is conserved  Before: 0       After: 0
Answer
                         n      p e         e


This reaction cannot occur because:
• Charge is conserved  Before: 0         After: +1 - 1 + 0 = 0
• Baryon no is conserved  Before: 0      After: 0 + 0 + 0 = 0
• Strangeness is conserved  Before: 0    After: 0
• But, Lepton no is not conserved  Before: 0     After: +1 + 1 = 2
Answer
                           n     e

This reaction cannot occur because:
• Charge is conserved  Before: 0            After: -1 + 2/3 + 1/3 = 0
• But, Baryon not is conserved  Before: 1          After: 0 + 0 = 0
• Strangeness is changed by +1 conserved  Before: 0        After: +1
• But, Lepton no is not conserved  Before: 0       After: +1 + 0 = +1

Contenu connexe

Tendances

Particle physics - Standard Model
Particle physics - Standard ModelParticle physics - Standard Model
Particle physics - Standard Model
David Young
 
Standard Model in Particle Physics, Physical Science Lesson PowerPoint
Standard Model in Particle Physics, Physical Science Lesson PowerPointStandard Model in Particle Physics, Physical Science Lesson PowerPoint
Standard Model in Particle Physics, Physical Science Lesson PowerPoint
www.sciencepowerpoint.com
 
photo electric effect slides
photo electric effect slidesphoto electric effect slides
photo electric effect slides
Mian Ullah
 

Tendances (20)

Mesons
Mesons Mesons
Mesons
 
Quark model 4-20 Aug 2018.pptx
Quark model  4-20 Aug 2018.pptxQuark model  4-20 Aug 2018.pptx
Quark model 4-20 Aug 2018.pptx
 
12.2
12.212.2
12.2
 
The Nuclear Shell Model
The Nuclear Shell ModelThe Nuclear Shell Model
The Nuclear Shell Model
 
Particle physics - Standard Model
Particle physics - Standard ModelParticle physics - Standard Model
Particle physics - Standard Model
 
Introduction to particle physics
Introduction to particle physicsIntroduction to particle physics
Introduction to particle physics
 
Nuclear physics
Nuclear physicsNuclear physics
Nuclear physics
 
Classification of nuclei and properties of nucleus
Classification  of nuclei and properties of nucleusClassification  of nuclei and properties of nucleus
Classification of nuclei and properties of nucleus
 
Standard Model in Particle Physics, Physical Science Lesson PowerPoint
Standard Model in Particle Physics, Physical Science Lesson PowerPointStandard Model in Particle Physics, Physical Science Lesson PowerPoint
Standard Model in Particle Physics, Physical Science Lesson PowerPoint
 
photo electric effect slides
photo electric effect slidesphoto electric effect slides
photo electric effect slides
 
Elementary particles
Elementary particlesElementary particles
Elementary particles
 
Applications of schrodinger equation
Applications of schrodinger equationApplications of schrodinger equation
Applications of schrodinger equation
 
Classical Mechanics-MSc
Classical Mechanics-MScClassical Mechanics-MSc
Classical Mechanics-MSc
 
Nuclear chemistry and radioactivity
Nuclear chemistry and radioactivityNuclear chemistry and radioactivity
Nuclear chemistry and radioactivity
 
Fundamental forces in nature
Fundamental forces in natureFundamental forces in nature
Fundamental forces in nature
 
heisenberg uncertainty principle
heisenberg uncertainty principleheisenberg uncertainty principle
heisenberg uncertainty principle
 
Nuclear force
Nuclear forceNuclear force
Nuclear force
 
nuclear shell model.pptx
nuclear shell model.pptxnuclear shell model.pptx
nuclear shell model.pptx
 
History of Quantum Mechanics
History of Quantum MechanicsHistory of Quantum Mechanics
History of Quantum Mechanics
 
Nuclear physics
Nuclear physicsNuclear physics
Nuclear physics
 

En vedette

Inside the Atom, Quarks, Leptons, Force Carrier Particles Physical Science Le...
Inside the Atom, Quarks, Leptons, Force Carrier Particles Physical Science Le...Inside the Atom, Quarks, Leptons, Force Carrier Particles Physical Science Le...
Inside the Atom, Quarks, Leptons, Force Carrier Particles Physical Science Le...
www.sciencepowerpoint.com
 
Quarks
QuarksQuarks
Quarks
Astrid
 
Quarkspresentation
QuarkspresentationQuarkspresentation
Quarkspresentation
zeewillew
 
Ch 18 Electric Fields
Ch 18 Electric FieldsCh 18 Electric Fields
Ch 18 Electric Fields
Scott Thomas
 
How Does Lightning Work?
How Does Lightning Work?How Does Lightning Work?
How Does Lightning Work?
erowell
 

En vedette (20)

Feynman diagrams
Feynman diagramsFeynman diagrams
Feynman diagrams
 
Inside the Atom, Quarks, Leptons, Force Carrier Particles Physical Science Le...
Inside the Atom, Quarks, Leptons, Force Carrier Particles Physical Science Le...Inside the Atom, Quarks, Leptons, Force Carrier Particles Physical Science Le...
Inside the Atom, Quarks, Leptons, Force Carrier Particles Physical Science Le...
 
Elementary particles and their properties
Elementary particles and their propertiesElementary particles and their properties
Elementary particles and their properties
 
Big Fast Data in High-Energy Particle Physics
Big Fast Data in High-Energy Particle PhysicsBig Fast Data in High-Energy Particle Physics
Big Fast Data in High-Energy Particle Physics
 
Summer '16 Lightning Update for ISVs (June 30, 2016)
Summer '16 Lightning Update for ISVs (June 30, 2016)Summer '16 Lightning Update for ISVs (June 30, 2016)
Summer '16 Lightning Update for ISVs (June 30, 2016)
 
Feynman Rules
Feynman RulesFeynman Rules
Feynman Rules
 
Quarks
QuarksQuarks
Quarks
 
Quarkspresentation
QuarkspresentationQuarkspresentation
Quarkspresentation
 
Matter and antimatter
Matter and antimatterMatter and antimatter
Matter and antimatter
 
Quarks
QuarksQuarks
Quarks
 
Quarks
QuarksQuarks
Quarks
 
Mass and energy
Mass and energyMass and energy
Mass and energy
 
The atom and rutherford experiment
The atom and rutherford experimentThe atom and rutherford experiment
The atom and rutherford experiment
 
Quarks
QuarksQuarks
Quarks
 
Photon and energy levels
Photon and energy levelsPhoton and energy levels
Photon and energy levels
 
Ch 18 Electric Fields
Ch 18 Electric FieldsCh 18 Electric Fields
Ch 18 Electric Fields
 
How Does Lightning Work?
How Does Lightning Work?How Does Lightning Work?
How Does Lightning Work?
 
Photoelectric effect
Photoelectric effectPhotoelectric effect
Photoelectric effect
 
Phenomenon of lightning
Phenomenon of lightningPhenomenon of lightning
Phenomenon of lightning
 
presentation of lightning
presentation of lightningpresentation of lightning
presentation of lightning
 

Similaire à Classifying particles

Radioactivity + isotopes lect.1,2,
Radioactivity + isotopes lect.1,2,Radioactivity + isotopes lect.1,2,
Radioactivity + isotopes lect.1,2,
kamal2200
 
Facultyetsuedublantonlecture3radiationppt3714
Facultyetsuedublantonlecture3radiationppt3714Facultyetsuedublantonlecture3radiationppt3714
Facultyetsuedublantonlecture3radiationppt3714
Michel Tamira
 
Radioactivity
RadioactivityRadioactivity
Radioactivity
wilsone
 
Physics fs2009
Physics fs2009Physics fs2009
Physics fs2009
bjmeef
 
introduction-to-radioactivity
 introduction-to-radioactivity introduction-to-radioactivity
introduction-to-radioactivity
Michel Tamira
 
Radioactivity
RadioactivityRadioactivity
Radioactivity
E H Annex
 
Radiation section 2
Radiation section 2Radiation section 2
Radiation section 2
jmocherman
 

Similaire à Classifying particles (20)

AS PARTICLE PHYSICS MODULE
AS PARTICLE PHYSICS MODULEAS PARTICLE PHYSICS MODULE
AS PARTICLE PHYSICS MODULE
 
11 Nuclear
11 Nuclear11 Nuclear
11 Nuclear
 
Radioactivity + isotopes lect.1,2,
Radioactivity + isotopes lect.1,2,Radioactivity + isotopes lect.1,2,
Radioactivity + isotopes lect.1,2,
 
Chapter 21 Lecture- Nuclear Chemistry
Chapter 21 Lecture- Nuclear ChemistryChapter 21 Lecture- Nuclear Chemistry
Chapter 21 Lecture- Nuclear Chemistry
 
Animatter Explained
Animatter ExplainedAnimatter Explained
Animatter Explained
 
Facultyetsuedublantonlecture3radiationppt3714
Facultyetsuedublantonlecture3radiationppt3714Facultyetsuedublantonlecture3radiationppt3714
Facultyetsuedublantonlecture3radiationppt3714
 
Radioactivity.pdf
Radioactivity.pdfRadioactivity.pdf
Radioactivity.pdf
 
Nuclear Decay
Nuclear DecayNuclear Decay
Nuclear Decay
 
Nuclear Decay
Nuclear  DecayNuclear  Decay
Nuclear Decay
 
Radioactive decay
Radioactive decayRadioactive decay
Radioactive decay
 
Quantum numbers
Quantum numbersQuantum numbers
Quantum numbers
 
from web, will read for later, and delete thereafter
from web, will read for later, and delete thereafterfrom web, will read for later, and delete thereafter
from web, will read for later, and delete thereafter
 
Radioactivity & waste
Radioactivity & wasteRadioactivity & waste
Radioactivity & waste
 
2k19–Nuclear Physics–02.pdf
2k19–Nuclear Physics–02.pdf2k19–Nuclear Physics–02.pdf
2k19–Nuclear Physics–02.pdf
 
Nuclear Basics Summer 2010
Nuclear Basics Summer 2010Nuclear Basics Summer 2010
Nuclear Basics Summer 2010
 
Radioactivity
RadioactivityRadioactivity
Radioactivity
 
Physics fs2009
Physics fs2009Physics fs2009
Physics fs2009
 
introduction-to-radioactivity
 introduction-to-radioactivity introduction-to-radioactivity
introduction-to-radioactivity
 
Radioactivity
RadioactivityRadioactivity
Radioactivity
 
Radiation section 2
Radiation section 2Radiation section 2
Radiation section 2
 

Dernier

+971581248768>> SAFE AND ORIGINAL ABORTION PILLS FOR SALE IN DUBAI AND ABUDHA...
+971581248768>> SAFE AND ORIGINAL ABORTION PILLS FOR SALE IN DUBAI AND ABUDHA...+971581248768>> SAFE AND ORIGINAL ABORTION PILLS FOR SALE IN DUBAI AND ABUDHA...
+971581248768>> SAFE AND ORIGINAL ABORTION PILLS FOR SALE IN DUBAI AND ABUDHA...
?#DUbAI#??##{{(☎️+971_581248768%)**%*]'#abortion pills for sale in dubai@
 

Dernier (20)

HTML Injection Attacks: Impact and Mitigation Strategies
HTML Injection Attacks: Impact and Mitigation StrategiesHTML Injection Attacks: Impact and Mitigation Strategies
HTML Injection Attacks: Impact and Mitigation Strategies
 
presentation ICT roal in 21st century education
presentation ICT roal in 21st century educationpresentation ICT roal in 21st century education
presentation ICT roal in 21st century education
 
2024: Domino Containers - The Next Step. News from the Domino Container commu...
2024: Domino Containers - The Next Step. News from the Domino Container commu...2024: Domino Containers - The Next Step. News from the Domino Container commu...
2024: Domino Containers - The Next Step. News from the Domino Container commu...
 
+971581248768>> SAFE AND ORIGINAL ABORTION PILLS FOR SALE IN DUBAI AND ABUDHA...
+971581248768>> SAFE AND ORIGINAL ABORTION PILLS FOR SALE IN DUBAI AND ABUDHA...+971581248768>> SAFE AND ORIGINAL ABORTION PILLS FOR SALE IN DUBAI AND ABUDHA...
+971581248768>> SAFE AND ORIGINAL ABORTION PILLS FOR SALE IN DUBAI AND ABUDHA...
 
Polkadot JAM Slides - Token2049 - By Dr. Gavin Wood
Polkadot JAM Slides - Token2049 - By Dr. Gavin WoodPolkadot JAM Slides - Token2049 - By Dr. Gavin Wood
Polkadot JAM Slides - Token2049 - By Dr. Gavin Wood
 
Strategies for Unlocking Knowledge Management in Microsoft 365 in the Copilot...
Strategies for Unlocking Knowledge Management in Microsoft 365 in the Copilot...Strategies for Unlocking Knowledge Management in Microsoft 365 in the Copilot...
Strategies for Unlocking Knowledge Management in Microsoft 365 in the Copilot...
 
Connector Corner: Accelerate revenue generation using UiPath API-centric busi...
Connector Corner: Accelerate revenue generation using UiPath API-centric busi...Connector Corner: Accelerate revenue generation using UiPath API-centric busi...
Connector Corner: Accelerate revenue generation using UiPath API-centric busi...
 
Strategies for Landing an Oracle DBA Job as a Fresher
Strategies for Landing an Oracle DBA Job as a FresherStrategies for Landing an Oracle DBA Job as a Fresher
Strategies for Landing an Oracle DBA Job as a Fresher
 
Boost PC performance: How more available memory can improve productivity
Boost PC performance: How more available memory can improve productivityBoost PC performance: How more available memory can improve productivity
Boost PC performance: How more available memory can improve productivity
 
Exploring the Future Potential of AI-Enabled Smartphone Processors
Exploring the Future Potential of AI-Enabled Smartphone ProcessorsExploring the Future Potential of AI-Enabled Smartphone Processors
Exploring the Future Potential of AI-Enabled Smartphone Processors
 
Top 5 Benefits OF Using Muvi Live Paywall For Live Streams
Top 5 Benefits OF Using Muvi Live Paywall For Live StreamsTop 5 Benefits OF Using Muvi Live Paywall For Live Streams
Top 5 Benefits OF Using Muvi Live Paywall For Live Streams
 
Manulife - Insurer Innovation Award 2024
Manulife - Insurer Innovation Award 2024Manulife - Insurer Innovation Award 2024
Manulife - Insurer Innovation Award 2024
 
Boost Fertility New Invention Ups Success Rates.pdf
Boost Fertility New Invention Ups Success Rates.pdfBoost Fertility New Invention Ups Success Rates.pdf
Boost Fertility New Invention Ups Success Rates.pdf
 
TrustArc Webinar - Stay Ahead of US State Data Privacy Law Developments
TrustArc Webinar - Stay Ahead of US State Data Privacy Law DevelopmentsTrustArc Webinar - Stay Ahead of US State Data Privacy Law Developments
TrustArc Webinar - Stay Ahead of US State Data Privacy Law Developments
 
Real Time Object Detection Using Open CV
Real Time Object Detection Using Open CVReal Time Object Detection Using Open CV
Real Time Object Detection Using Open CV
 
MINDCTI Revenue Release Quarter One 2024
MINDCTI Revenue Release Quarter One 2024MINDCTI Revenue Release Quarter One 2024
MINDCTI Revenue Release Quarter One 2024
 
From Event to Action: Accelerate Your Decision Making with Real-Time Automation
From Event to Action: Accelerate Your Decision Making with Real-Time AutomationFrom Event to Action: Accelerate Your Decision Making with Real-Time Automation
From Event to Action: Accelerate Your Decision Making with Real-Time Automation
 
TrustArc Webinar - Unlock the Power of AI-Driven Data Discovery
TrustArc Webinar - Unlock the Power of AI-Driven Data DiscoveryTrustArc Webinar - Unlock the Power of AI-Driven Data Discovery
TrustArc Webinar - Unlock the Power of AI-Driven Data Discovery
 
Apidays New York 2024 - The value of a flexible API Management solution for O...
Apidays New York 2024 - The value of a flexible API Management solution for O...Apidays New York 2024 - The value of a flexible API Management solution for O...
Apidays New York 2024 - The value of a flexible API Management solution for O...
 
Apidays New York 2024 - Scaling API-first by Ian Reasor and Radu Cotescu, Adobe
Apidays New York 2024 - Scaling API-first by Ian Reasor and Radu Cotescu, AdobeApidays New York 2024 - Scaling API-first by Ian Reasor and Radu Cotescu, Adobe
Apidays New York 2024 - Scaling API-first by Ian Reasor and Radu Cotescu, Adobe
 

Classifying particles

  • 1. Particles Classification of Particles Hadrons and Quarks Leptons Thursday, 08 December 2011
  • 2. The Stanford linear accelerator In 1968 the Stanford accelerator shot a beam of 20 GeV electrons on a target. The results showed clearly that the electrons were strongly scattered by stationary protons and sometimes even bounced backward. q q q
  • 3. The Stanford linear accelerator Does that remind you of another famous experiment? What can be deduced about the internal structure of the proton? The outcomes of the experiment resemble Rutherford’s experiment that led to the discovery of the nucleus. The proton must be made up of sub-nuclear particles, some of which carry negative charge. This provides proof for the existence of quarks.
  • 4. The Structure of a Proton These results pointed at a structure of nucleons like the proton as being made up of three sub-nuclear particles called Quarks. q q q
  • 5. Classifying Particles All particles can be classified in three main categories: • Hadrons  made up of quarks. They are affected by strong forces • Leptons  fundamental particles, i.e. they don’t have an internal structure. In other words, they are not made up of smaller particles and are not affected by strong forces. • Quarks  smaller particles that combine to form hadrons. They carry fractional charges (fractions of the charge of the electron). So, what is everything made of? • Quarks and Leptons
  • 6. 1st • up (u)  +2/3 generation • down (d)  -1/3 2nd • charm (c) +2/3 generation • strange  -1/3 3rd • top (t)  +2/3 generation • bottom (b)  -1/3
  • 7. • electron (e-)  -1 1st generation • electron neutrino ( e)  0 • muon ( -) -1 2nd generation • muon-neutrino ( ) 0 • tau ( -)  -1 3rd generation • Tau-neutrino ( ) 0
  • 8. • Pions: 0=(uu) or dd += (ud) Meson (1 -= (ud) quark + 1 anti- quark) • Kaons: 0 (ds) + (us) - (us) Baryons • Proton (uud) +1 (3 quarks) • Neutron (udd) 0
  • 9. Lego Particles Up quark (+2/3) Anti-up quark (+2/3) Down quark (-1/3) Anti-Down quark (- 1/3) Strange quark (-1/3) Anti-Strange quark (- 1/3) Electron (-1) Positron (+1) Neutrino (0) Anti-Neutrino (0) Muon (-1) Anti-moun (+1)
  • 10. Fundamental particles A proton is made of two Up quarks and one down. Show that the sum of the three charges gives +1. +2/3 + 2/3 – 1/3 = +3/3 = +1 u d u A neutron is made of two down quarks and one up quark. Show the neutrality of this distribution. -1/3 – 1/3 + 2/3 = -2/3 + 2/3 = 0 d d u
  • 11. Lepton Number All leptons have an additional property called Lepton Number. The lepton number is always conserved. Particle Lepton Number All leptons +1 All anti-leptons -1 Hadrons 0 (baryons and mesons)
  • 12. - Decay and lepton number Explain why both an electron and an anti-neutrino must be formed in a - decay. n p e e • The lepton number must be conserved. • e- lepton no = +1 +1 – 1 = 0  an electron and an anti- neutrino must be created for lepton • e lepton no = -1 number to be conserved
  • 13. Properties of quarks Quarks and anti-quarks have some properties that you might not have encountered before: • Relative Charge  all quarks and anti-quarks carry a charge which is a fraction of the charge of the electron, i.e. 1.6 x 10-19 C. In all interactions charge must be conserved. • Baryon Number  all quarks and anti-quarks have a baryon number. The baryon number is +1/3 for quarks and -1/3 for all anti-quarks. In all interactions baryon number must be conserved. • Strangeness  all quarks and anti-quarks have strangeness = 0 apart from the strange quark (strangeness = -1) and the anti-strange quark (strangeness = +1). In all interactions involving the STRONG FORCE strangeness must be conserved, but in weak interactions strangeness can be conserved, or change by ±1.
  • 14. Properties of quarks Baryon Name Symbol Charge Strangeness Number up u +2/3 +1/3 0 Quarks down d -1/3 +1/3 0 strange s -1/3 +1/3 -1 Anti-quarks anti-up u -2/3 -1/3 0 anti-down d +1/3 -1/3 0 anti-strange s +1/3 -1/3 +1
  • 15. Mesons and Quarks A K+ meson is made up of an up quark and an anti-strange quark. Work out the relative charge, baryon number and strangeness of this particle. • Charge +2/3 + 1/3 = +3/3 = +1 • Baryon no  +1/3 – 1/3 = 0 • Strangeness  0 + 1 = +1 s u
  • 16. Mesons and Quarks A - meson is made up of an anti-up quark and a down quark. Work out the relative charge, baryon number and strangeness of this particle. • Charge -2/3 - 1/3 = -3/3 = -1 • Baryon no  +1/3 – 1/3 = 0 • Strangeness  0 – 0 = 0 u d
  • 17. Change of Quarks in - Decay In a - decay one quark in the neutron changes character (flavour) to form a proton. Complete the diagram with the correct quarks in the proton. proton After u du e- e W u dd Before neutron A down quark in the neutron changes into an up quark, emitting an electron and an anti-neutrino.
  • 18. Stable and Unstable Baryons In a - decay one quark in the neutron changes character (flavour) to form a proton. But why does that happen? • The proton is the only stable Baryon. • All other Baryons eventually decay into a proton. • So, it is not surprising that in “nature” the neutron decays into a proton releasing an electron and an anti-neutrino.
  • 19. Change of Quarks in + Decay In a - decay one quark in the neutron changes character (flavour) to form a proton. Complete the diagram with the correct quarks in the proton and the neutron. neutron After u dd e+ e W u du Before proton An up quark in the neutron changes into an down quark, emitting a positron and a neutrino.
  • 20. Conservation Laws In all particle interactions these conservation laws apply and must be fulfilled for the interaction to happen: • Conservation of Charge  In all interactions charge must be conserved. So, Sum of Charges before = Sum of Charges after • Conservation of Baryon Number  In all interactions baryon number must be conserved. • Conservation of Strangeness  In all interactions involving the STRONG FORCE strangeness must be conserved, but in weak interactions strangeness can be conserved, or change by ±1. • Conservation of Lepton Number  In all interactions the lepton number must be conserved.
  • 21. Conservation Laws Applying the conservation laws, show whether the following interactions are possible or not. Answer n p e e Answer e e Answer n p e e Answer n e
  • 22. Answer n p e e This reaction can occur because: • Charge is conserved  Before: 0 After: +1 – 1 + 0 = 0 • Baryon no is conserved  Before: +1 After: +1 + 0 + 0 = +1 • Lepton no is conserved  Before: 0 After: 0 + 1 - 1 = 0 • Strangeness is conserved  Before: 0 After: 0
  • 23. Answer e e This reaction can occur because: • Charge is conserved  Before: 0 After: -1 + 1 = 0 • Baryon no is conserved  Before: 0 After: 0 + 0 = 0 • Lepton no is conserved  Before: 0 After: +1 - 1 = 0 • Strangeness is conserved  Before: 0 After: 0
  • 24. Answer n p e e This reaction cannot occur because: • Charge is conserved  Before: 0 After: +1 - 1 + 0 = 0 • Baryon no is conserved  Before: 0 After: 0 + 0 + 0 = 0 • Strangeness is conserved  Before: 0 After: 0 • But, Lepton no is not conserved  Before: 0 After: +1 + 1 = 2
  • 25. Answer n e This reaction cannot occur because: • Charge is conserved  Before: 0 After: -1 + 2/3 + 1/3 = 0 • But, Baryon not is conserved  Before: 1 After: 0 + 0 = 0 • Strangeness is changed by +1 conserved  Before: 0 After: +1 • But, Lepton no is not conserved  Before: 0 After: +1 + 0 = +1