SlideShare ist ein Scribd-Unternehmen logo
1 von 23
ELEMENTARY   PARTICLESPresented  by Mr. S.N. Saravanamoorthy, Assistant Professor of Physics, DevangaArts College (Autonomous), Aruppukottai – 626 101.
1. Introduction 2. Classification 3. Particles & Antiparticles 4. Particles instability 5. Conservation laws
INTRODUCTION *  By the year 1932, only three elementary particles namely electron,      proton and photon were known. * The discovery of Neutron by Chadwick in 1932 raised their number to      four. * These elementary particles are the building blocks of matter & they      have characteristic properties such as rest mass, electric charge &      intrinsic angular momentum.  * The elementary particles discovered so far, form a long list of      around 200. These particles are elementary in the sense that they      are structureless, i.e., they cannot be explained as a system of      other elementary particles.
Elementary particle Baryons                   Leptons                            Mesons                 Antiparticles              Electron       Photon        Neutron              Muon                                                                                                              kaon                                                                                              Pion                       Eta Nucleons                Hyperons Proton                           Lambda, Sigma, Omega Neutron
BARYONS (Or) heavy particles * Protons & particles  heavier than proton form this group. * Proton and neutron are called nucleons and the rest mass      are called hyperons. * Every baryons has an antiparticle. * If a number, called the baryon number +1 is assigned to     baryons and a number -1 is assigned to antibaryons, then     in any closed system interaction or decay, the  baryon     number does not change. This is the law of conservation      of baryons.
HYPERONS * Time decay of the order of 10−10 seconds * Mass value intermediate between neutron & deuteron * Their decay time is very much greater than the time     of their formation (10−3 sec). * K mesons – Strange Particles (Gellmann & Nishijima) * Four types – Lambda, Sigma, Xi, Omega
Leptons *It contains electron, photon, neutrino & muon. * All these elementary particles have masses smaller    than that of a pion. ELECTRON * First discovered particle * negative charge & stable particle * An electrostatic field exists between two electrons
PHOTON * no charge & no rest mass * It has energy given by Plank’s equation E=hν * It has an equivalent mass given by Einstein’s equation    E=mc2. NEUTRINO * 1956 – Beta ray spectra in radioactivity * no charge & rest mass is zero * It travels with the speed of light * It exists in two form, one associated with electron & the other with the muon
Muon * It is similar to the electron except that its mass is     about 200 times that of the electron. * It decays very quickly with a half life of 2.2μs into    one electron and two neutrinos.  * It is negatively charged and has a spin of ½.  * It was first discovered during the study of cosmic rays.
MESONS * Masses are between those of leptons & baryons. * They are unstable. * They decay into lighter mesons or leptons. * They have either positive, negative at zero charge. * The mesons include the pion, kaon and eta particles.
Positive Pimeson (Pion) ,[object Object]
positively charged particle & life time - 10−8 secNeutral Pion ,[object Object]
Mass is equal to 264 times the mass of the electronCharged Kaon: +ve charge & a mass of about one-half of                              proton. Neutral kaon: No charge & Its life is of the order of 10−9 sec
PARTICLES & ANTI-PARTICLES Electron – Positron * Same mass & the same spin but opposite charge *They annihilate each other with the emission of photons * The existence of an antiparticle for the electron was    actually predicted by Dirac, because of a symmetry of     the equations of the relativistic quantum theory of the      electron. ,[object Object],[object Object]
Neutron and Antineutron
Neutrino and Antineutrino It has Charge Zero, spin ½, zero rest mass and magnetic moment smaller than 10−8 Bohr magneton or nearly zero. Finite energy, momentum and travels with the speed of light. It does not cause ionization on passing through matter. The spin of the neutrino is opposite in direction to the direction of its motion. (neutrino spins – counterclockwise) The spin of the antineutrino is in the same direction as its direction of motion. (It spins clockwise) The neutrino moves through space in the manner of a left-handed screw, while the antineutrino does so in the manner of a right-handed screw.  Continue…
Neutrino possesses a “left-handed” helicity ; the antineutrino possesses a “right-handed” helicity. Neutrino’s emitted in Beta decay have a negative helicity.  They are longitudinally polarized with their spin axes antiparallel to their direction of travel.     H = + 1 for ν- ; H = - for ν Because of its lack of charge and magnetic moment, a neutrino has essentially no interaction with matter, except that which leads to inverse beta decay. This interaction is extremely weak. (σ≈10- 20  barn) Matter is almost totally transparent to neutrinos.
Conservation Laws Conservation of parity Charge conjugation symmetry Time reversal symmetry Combined Inversion of CPT
Conservation of Parity Parity relates to the symmetry of the wave function that represents the system. If the wave function is unchanged then the system has a parity of +1. If changed, then the system has parity of -1. During a reaction in which parity is conserved, the total parity number does not change. Prior to 1956 it was believed that all reactions in nature obeyed the law of conservation of parity. Yang and Lee pointed out that in reactions involving the weak interaction, parity was not conserved. Indeed parity conservation is found to hold true only in the strong and em interactions.
Charge conjugate symmetry It is the act of symmetry operation in which every particle in a system is replaced by its antiparticle. If the anti-system or antimatter counterpart exhibits the same physical phenomena, then charge parity (C) is conserved. In fact C is not conserved in the weak interaction.
Time reversal symmetry Time parity T describes the behaviour of a wave function when t is replaced by –t.  The symmetry operation that corresponds to the conservation of time parity is time reversal. The direction of  time is not significant, so that the reverse of any process that can occur is also a process that can occur. Prior to 1964, time parity T was considered to be conserved in every interaction. One form of Kokaon can decay in to π+, π−, which violates the conservation of T.  The symmetry of phenomena under time reversal does not seem to be universal.

Weitere ähnliche Inhalte

Was ist angesagt?

nuclear physics,unit 6
nuclear physics,unit 6nuclear physics,unit 6
nuclear physics,unit 6
Kumar
 
Rutherford scattering show
Rutherford scattering showRutherford scattering show
Rutherford scattering show
Khemendra shukla
 

Was ist angesagt? (20)

12.2
12.212.2
12.2
 
Quantum theory
Quantum theoryQuantum theory
Quantum theory
 
Pauli exclusion principle
Pauli exclusion principlePauli exclusion principle
Pauli exclusion principle
 
Nuclear rections ppt
Nuclear rections pptNuclear rections ppt
Nuclear rections ppt
 
Band theory of solid
Band theory of solidBand theory of solid
Band theory of solid
 
Quarks
QuarksQuarks
Quarks
 
Photoelectric effect ppt
Photoelectric effect pptPhotoelectric effect ppt
Photoelectric effect ppt
 
Wave particle duality
Wave particle dualityWave particle duality
Wave particle duality
 
nuclear physics,unit 6
nuclear physics,unit 6nuclear physics,unit 6
nuclear physics,unit 6
 
Elementary particles
Elementary particlesElementary particles
Elementary particles
 
Energy bands and gaps in semiconductor
Energy bands and gaps in semiconductorEnergy bands and gaps in semiconductor
Energy bands and gaps in semiconductor
 
Gamow theory of alpha decay by prerna
Gamow theory of alpha decay by prernaGamow theory of alpha decay by prerna
Gamow theory of alpha decay by prerna
 
statistic mechanics
statistic mechanicsstatistic mechanics
statistic mechanics
 
Rutherford scattering show
Rutherford scattering showRutherford scattering show
Rutherford scattering show
 
Origin of quantum mechanics
Origin of quantum mechanicsOrigin of quantum mechanics
Origin of quantum mechanics
 
History of Quantum Mechanics
History of Quantum MechanicsHistory of Quantum Mechanics
History of Quantum Mechanics
 
nuclear fission and fusion
nuclear fission and fusionnuclear fission and fusion
nuclear fission and fusion
 
Energy band and energy gap by Pratimesh pathak
Energy band and energy gap by Pratimesh pathakEnergy band and energy gap by Pratimesh pathak
Energy band and energy gap by Pratimesh pathak
 
Quantum theory ppt
Quantum theory ppt Quantum theory ppt
Quantum theory ppt
 
State and explain Alpha , Beta and Gamma decay
State and explain Alpha , Beta and Gamma decayState and explain Alpha , Beta and Gamma decay
State and explain Alpha , Beta and Gamma decay
 

Ähnlich wie Elementary particles

Elementary particles
Elementary particlesElementary particles
Elementary particles
SNS
 
Topic 7.3 - The structure of matter.pptx
Topic 7.3 - The structure of matter.pptxTopic 7.3 - The structure of matter.pptx
Topic 7.3 - The structure of matter.pptx
HashemYamani
 
BE UNIT-1 basic electronics unit one.pptx
BE UNIT-1 basic electronics unit one.pptxBE UNIT-1 basic electronics unit one.pptx
BE UNIT-1 basic electronics unit one.pptx
harisbs369
 
Education.27.11 with a big boy toyzz.pdf
Education.27.11 with a big boy toyzz.pdfEducation.27.11 with a big boy toyzz.pdf
Education.27.11 with a big boy toyzz.pdf
israksiam311
 
Radioactivity
RadioactivityRadioactivity
Radioactivity
wilsone
 

Ähnlich wie Elementary particles (20)

Elementary particles
Elementary particlesElementary particles
Elementary particles
 
elementaryparticles-101223114011-phpapp02.pptx
elementaryparticles-101223114011-phpapp02.pptxelementaryparticles-101223114011-phpapp02.pptx
elementaryparticles-101223114011-phpapp02.pptx
 
Classification of particles
Classification of particlesClassification of particles
Classification of particles
 
Unit2 Presentation
Unit2 PresentationUnit2 Presentation
Unit2 Presentation
 
Atomic structore
Atomic structoreAtomic structore
Atomic structore
 
Atom inside out
Atom inside outAtom inside out
Atom inside out
 
physics project.pptx
physics project.pptxphysics project.pptx
physics project.pptx
 
Quantum Numbers - Mass, Charge, Spin
Quantum Numbers - Mass, Charge, SpinQuantum Numbers - Mass, Charge, Spin
Quantum Numbers - Mass, Charge, Spin
 
Topic 7.3 - The structure of matter.pptx
Topic 7.3 - The structure of matter.pptxTopic 7.3 - The structure of matter.pptx
Topic 7.3 - The structure of matter.pptx
 
BE UNIT-1 basic electronics unit one.pptx
BE UNIT-1 basic electronics unit one.pptxBE UNIT-1 basic electronics unit one.pptx
BE UNIT-1 basic electronics unit one.pptx
 
Structure of atom by pratiksha
Structure of atom by pratikshaStructure of atom by pratiksha
Structure of atom by pratiksha
 
Shubham kumar{11th a}
Shubham kumar{11th a}Shubham kumar{11th a}
Shubham kumar{11th a}
 
Martin Lindsey MSIMatter Presentation
Martin Lindsey MSIMatter PresentationMartin Lindsey MSIMatter Presentation
Martin Lindsey MSIMatter Presentation
 
Structure of atomic
Structure of atomicStructure of atomic
Structure of atomic
 
Chemical bonding and aromaticity
Chemical bonding and aromaticityChemical bonding and aromaticity
Chemical bonding and aromaticity
 
The atom and rutherford experiment
The atom and rutherford experimentThe atom and rutherford experiment
The atom and rutherford experiment
 
Education.27.11 with a big boy toyzz.pdf
Education.27.11 with a big boy toyzz.pdfEducation.27.11 with a big boy toyzz.pdf
Education.27.11 with a big boy toyzz.pdf
 
Automic Structure
Automic Structure Automic Structure
Automic Structure
 
Radioactivity
RadioactivityRadioactivity
Radioactivity
 
Atomic and nuclear physics
Atomic and nuclear physicsAtomic and nuclear physics
Atomic and nuclear physics
 

Mehr von SNS (6)

Growth and spectroscopic studies on vitamin 'C' crystal
Growth and spectroscopic studies on vitamin 'C' crystalGrowth and spectroscopic studies on vitamin 'C' crystal
Growth and spectroscopic studies on vitamin 'C' crystal
 
GATE - Physics - 2006
GATE - Physics - 2006GATE - Physics - 2006
GATE - Physics - 2006
 
GATE - Physics - 2005
GATE - Physics - 2005GATE - Physics - 2005
GATE - Physics - 2005
 
Materials science
Materials scienceMaterials science
Materials science
 
Matter
MatterMatter
Matter
 
Monkey
MonkeyMonkey
Monkey
 

Kürzlich hochgeladen

Making and Justifying Mathematical Decisions.pdf
Making and Justifying Mathematical Decisions.pdfMaking and Justifying Mathematical Decisions.pdf
Making and Justifying Mathematical Decisions.pdf
Chris Hunter
 
1029-Danh muc Sach Giao Khoa khoi 6.pdf
1029-Danh muc Sach Giao Khoa khoi  6.pdf1029-Danh muc Sach Giao Khoa khoi  6.pdf
1029-Danh muc Sach Giao Khoa khoi 6.pdf
QucHHunhnh
 
An Overview of Mutual Funds Bcom Project.pdf
An Overview of Mutual Funds Bcom Project.pdfAn Overview of Mutual Funds Bcom Project.pdf
An Overview of Mutual Funds Bcom Project.pdf
SanaAli374401
 
Seal of Good Local Governance (SGLG) 2024Final.pptx
Seal of Good Local Governance (SGLG) 2024Final.pptxSeal of Good Local Governance (SGLG) 2024Final.pptx
Seal of Good Local Governance (SGLG) 2024Final.pptx
negromaestrong
 
Gardella_PRCampaignConclusion Pitch Letter
Gardella_PRCampaignConclusion Pitch LetterGardella_PRCampaignConclusion Pitch Letter
Gardella_PRCampaignConclusion Pitch Letter
MateoGardella
 

Kürzlich hochgeladen (20)

INDIA QUIZ 2024 RLAC DELHI UNIVERSITY.pptx
INDIA QUIZ 2024 RLAC DELHI UNIVERSITY.pptxINDIA QUIZ 2024 RLAC DELHI UNIVERSITY.pptx
INDIA QUIZ 2024 RLAC DELHI UNIVERSITY.pptx
 
This PowerPoint helps students to consider the concept of infinity.
This PowerPoint helps students to consider the concept of infinity.This PowerPoint helps students to consider the concept of infinity.
This PowerPoint helps students to consider the concept of infinity.
 
PROCESS RECORDING FORMAT.docx
PROCESS      RECORDING        FORMAT.docxPROCESS      RECORDING        FORMAT.docx
PROCESS RECORDING FORMAT.docx
 
Making and Justifying Mathematical Decisions.pdf
Making and Justifying Mathematical Decisions.pdfMaking and Justifying Mathematical Decisions.pdf
Making and Justifying Mathematical Decisions.pdf
 
Advance Mobile Application Development class 07
Advance Mobile Application Development class 07Advance Mobile Application Development class 07
Advance Mobile Application Development class 07
 
1029-Danh muc Sach Giao Khoa khoi 6.pdf
1029-Danh muc Sach Giao Khoa khoi  6.pdf1029-Danh muc Sach Giao Khoa khoi  6.pdf
1029-Danh muc Sach Giao Khoa khoi 6.pdf
 
Class 11th Physics NEET formula sheet pdf
Class 11th Physics NEET formula sheet pdfClass 11th Physics NEET formula sheet pdf
Class 11th Physics NEET formula sheet pdf
 
An Overview of Mutual Funds Bcom Project.pdf
An Overview of Mutual Funds Bcom Project.pdfAn Overview of Mutual Funds Bcom Project.pdf
An Overview of Mutual Funds Bcom Project.pdf
 
Seal of Good Local Governance (SGLG) 2024Final.pptx
Seal of Good Local Governance (SGLG) 2024Final.pptxSeal of Good Local Governance (SGLG) 2024Final.pptx
Seal of Good Local Governance (SGLG) 2024Final.pptx
 
Sports & Fitness Value Added Course FY..
Sports & Fitness Value Added Course FY..Sports & Fitness Value Added Course FY..
Sports & Fitness Value Added Course FY..
 
Introduction to Nonprofit Accounting: The Basics
Introduction to Nonprofit Accounting: The BasicsIntroduction to Nonprofit Accounting: The Basics
Introduction to Nonprofit Accounting: The Basics
 
Application orientated numerical on hev.ppt
Application orientated numerical on hev.pptApplication orientated numerical on hev.ppt
Application orientated numerical on hev.ppt
 
Measures of Dispersion and Variability: Range, QD, AD and SD
Measures of Dispersion and Variability: Range, QD, AD and SDMeasures of Dispersion and Variability: Range, QD, AD and SD
Measures of Dispersion and Variability: Range, QD, AD and SD
 
Mixin Classes in Odoo 17 How to Extend Models Using Mixin Classes
Mixin Classes in Odoo 17  How to Extend Models Using Mixin ClassesMixin Classes in Odoo 17  How to Extend Models Using Mixin Classes
Mixin Classes in Odoo 17 How to Extend Models Using Mixin Classes
 
Mattingly "AI & Prompt Design: Structured Data, Assistants, & RAG"
Mattingly "AI & Prompt Design: Structured Data, Assistants, & RAG"Mattingly "AI & Prompt Design: Structured Data, Assistants, & RAG"
Mattingly "AI & Prompt Design: Structured Data, Assistants, & RAG"
 
Accessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impactAccessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impact
 
Paris 2024 Olympic Geographies - an activity
Paris 2024 Olympic Geographies - an activityParis 2024 Olympic Geographies - an activity
Paris 2024 Olympic Geographies - an activity
 
Gardella_PRCampaignConclusion Pitch Letter
Gardella_PRCampaignConclusion Pitch LetterGardella_PRCampaignConclusion Pitch Letter
Gardella_PRCampaignConclusion Pitch Letter
 
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
 
Z Score,T Score, Percential Rank and Box Plot Graph
Z Score,T Score, Percential Rank and Box Plot GraphZ Score,T Score, Percential Rank and Box Plot Graph
Z Score,T Score, Percential Rank and Box Plot Graph
 

Elementary particles

  • 1. ELEMENTARY PARTICLESPresented by Mr. S.N. Saravanamoorthy, Assistant Professor of Physics, DevangaArts College (Autonomous), Aruppukottai – 626 101.
  • 2. 1. Introduction 2. Classification 3. Particles & Antiparticles 4. Particles instability 5. Conservation laws
  • 3. INTRODUCTION * By the year 1932, only three elementary particles namely electron, proton and photon were known. * The discovery of Neutron by Chadwick in 1932 raised their number to four. * These elementary particles are the building blocks of matter & they have characteristic properties such as rest mass, electric charge & intrinsic angular momentum. * The elementary particles discovered so far, form a long list of around 200. These particles are elementary in the sense that they are structureless, i.e., they cannot be explained as a system of other elementary particles.
  • 4. Elementary particle Baryons Leptons Mesons Antiparticles Electron Photon Neutron Muon kaon Pion Eta Nucleons Hyperons Proton Lambda, Sigma, Omega Neutron
  • 5.
  • 6.
  • 7. BARYONS (Or) heavy particles * Protons & particles heavier than proton form this group. * Proton and neutron are called nucleons and the rest mass are called hyperons. * Every baryons has an antiparticle. * If a number, called the baryon number +1 is assigned to baryons and a number -1 is assigned to antibaryons, then in any closed system interaction or decay, the baryon number does not change. This is the law of conservation of baryons.
  • 8. HYPERONS * Time decay of the order of 10−10 seconds * Mass value intermediate between neutron & deuteron * Their decay time is very much greater than the time of their formation (10−3 sec). * K mesons – Strange Particles (Gellmann & Nishijima) * Four types – Lambda, Sigma, Xi, Omega
  • 9. Leptons *It contains electron, photon, neutrino & muon. * All these elementary particles have masses smaller than that of a pion. ELECTRON * First discovered particle * negative charge & stable particle * An electrostatic field exists between two electrons
  • 10. PHOTON * no charge & no rest mass * It has energy given by Plank’s equation E=hν * It has an equivalent mass given by Einstein’s equation E=mc2. NEUTRINO * 1956 – Beta ray spectra in radioactivity * no charge & rest mass is zero * It travels with the speed of light * It exists in two form, one associated with electron & the other with the muon
  • 11. Muon * It is similar to the electron except that its mass is about 200 times that of the electron. * It decays very quickly with a half life of 2.2μs into one electron and two neutrinos. * It is negatively charged and has a spin of ½. * It was first discovered during the study of cosmic rays.
  • 12. MESONS * Masses are between those of leptons & baryons. * They are unstable. * They decay into lighter mesons or leptons. * They have either positive, negative at zero charge. * The mesons include the pion, kaon and eta particles.
  • 13.
  • 14.
  • 15. Mass is equal to 264 times the mass of the electronCharged Kaon: +ve charge & a mass of about one-half of proton. Neutral kaon: No charge & Its life is of the order of 10−9 sec
  • 16.
  • 18. Neutrino and Antineutrino It has Charge Zero, spin ½, zero rest mass and magnetic moment smaller than 10−8 Bohr magneton or nearly zero. Finite energy, momentum and travels with the speed of light. It does not cause ionization on passing through matter. The spin of the neutrino is opposite in direction to the direction of its motion. (neutrino spins – counterclockwise) The spin of the antineutrino is in the same direction as its direction of motion. (It spins clockwise) The neutrino moves through space in the manner of a left-handed screw, while the antineutrino does so in the manner of a right-handed screw. Continue…
  • 19. Neutrino possesses a “left-handed” helicity ; the antineutrino possesses a “right-handed” helicity. Neutrino’s emitted in Beta decay have a negative helicity. They are longitudinally polarized with their spin axes antiparallel to their direction of travel. H = + 1 for ν- ; H = - for ν Because of its lack of charge and magnetic moment, a neutrino has essentially no interaction with matter, except that which leads to inverse beta decay. This interaction is extremely weak. (σ≈10- 20 barn) Matter is almost totally transparent to neutrinos.
  • 20. Conservation Laws Conservation of parity Charge conjugation symmetry Time reversal symmetry Combined Inversion of CPT
  • 21. Conservation of Parity Parity relates to the symmetry of the wave function that represents the system. If the wave function is unchanged then the system has a parity of +1. If changed, then the system has parity of -1. During a reaction in which parity is conserved, the total parity number does not change. Prior to 1956 it was believed that all reactions in nature obeyed the law of conservation of parity. Yang and Lee pointed out that in reactions involving the weak interaction, parity was not conserved. Indeed parity conservation is found to hold true only in the strong and em interactions.
  • 22. Charge conjugate symmetry It is the act of symmetry operation in which every particle in a system is replaced by its antiparticle. If the anti-system or antimatter counterpart exhibits the same physical phenomena, then charge parity (C) is conserved. In fact C is not conserved in the weak interaction.
  • 23. Time reversal symmetry Time parity T describes the behaviour of a wave function when t is replaced by –t. The symmetry operation that corresponds to the conservation of time parity is time reversal. The direction of time is not significant, so that the reverse of any process that can occur is also a process that can occur. Prior to 1964, time parity T was considered to be conserved in every interaction. One form of Kokaon can decay in to π+, π−, which violates the conservation of T. The symmetry of phenomena under time reversal does not seem to be universal.
  • 24. Combined Inversion of CPT The combined symmetry operation in which the antimatter mirror-image of a system is run in reverse allows a test of CPT invariance. The conservation of CPT means that for every process there is an antimatter mirror-image counterpart that takes place in reverse. This particular symmetry seems to hold for all interactions, even though its component symmetries sometimes fail individually.