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1.1b Particles & Radiation Quarks & Leptons Breithaupt pages 18 to 27 April 8 th , 2010

1.1b Particles & Radiation Quarks & Leptons

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1.1b Particles & Radiation Quarks & Leptons. Breithaupt pages 18 to 27. April 8 th , 2010. AQA AS Specification. Cosmic rays and particle generation. Cosmic rays consist of high energy protons and nuclei emitted from stars including the Sun. - PowerPoint PPT Presentation

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Page 1: 1.1b Particles & Radiation Quarks & Leptons

1.1b Particles & Radiation Quarks & Leptons

Breithaupt pages 18 to 27

April 8th, 2010

Page 2: 1.1b Particles & Radiation Quarks & Leptons

AQA AS SpecificationLessons Topics

1 & 2 Classification of particlesHadrons: baryons (proton, neutron) and antibaryons (antiproton and antineutron) and mesons (pion, kaon).Hadrons are subject to the strong nuclear force.Candidates should know that the proton is the only stable baryon into which other baryons eventually decay; in particular, the decay of the neutron should be known.Leptons: electron, muon, neutrino (electron and muon types).Leptons are subject to the weak interaction.Candidates will be expected to know baryon numbers for the hadrons. Lepton numbers for the leptons will be given in the data booklet.

3 to 5 Quarks and antiquarksUp (u), down (d) and strange (s) quarks only.Properties of quarks: charge, baryon number and strangeness.Combinations of quarks and antiquarks required for baryons (proton and neutron only), antibaryons (antiproton and antineutron only) and mesons (pion and kaon) only.Change of quark character in β - and β + decay.Application of the conservation laws for charge, baryon number, lepton number and strangeness to particle interactions. The necessary data will be provided in questions for particles outside those specified.

Page 3: 1.1b Particles & Radiation Quarks & Leptons

Cosmic rays and particle generation

• Cosmic rays consist of high energy protons and nuclei emitted from stars including the Sun.

• The protons strike gas atoms in the upper atmosphere and produce new short lived particles and antiparticles.

• These new particles can be detected at ground level by cloud chambers and other detectors.

• The first new particles to be detected were muons (1937), pions (1947) and kaons (1947).

Page 4: 1.1b Particles & Radiation Quarks & Leptons

AcceleratorsThese enable more controlled conditions than occur with cosmic radiation interactions.

High voltages are used to accelerate charged particles (electrons, positrons, protons and antiprotons) to near light velocities.

The particles are made to collide into a stationary target or head-on with each other.

The energy produced in these collisions can be used to create other particles.

The largest linear accelerator is at Stanford in California which uses a 50 000 million volts (50 GV) to accelerate electrons over a distance of 3km to an energy of 50 GeV.Linear particle accelerator game

The largest circular accelerator is the Large Hadron Collider (LHC) at CERN near Geneva. This uses a circular tube of circumference 27km within which protons and antiprotons are made to make head-on collisions at energies of up to 7000 GeVLHC SimulatorLHC Rap

Page 5: 1.1b Particles & Radiation Quarks & Leptons

Hadrons and leptonsHADRONS are particles that interact through the strong interactionexamples: protons, neutrons, pions and kaons

LEPTONS are particles that do not interact through the strong interactionexamples: electrons, positrons, muons and neutrinos

Leptons interact through the weak interaction.

All charged particles interact through the electromagnetic interaction

Page 6: 1.1b Particles & Radiation Quarks & Leptons

Baryons and mesons

• Baryons are hadrons that are protons or particles that eventually decay into protons.

• The proton is the only stable baryon.

• Neutrons are baryons because they decay into protons with a half-life of 12 minutes. Other baryons have much shorter half-lives.

• Baryons are also called ‘fermions’

• Mesons are hadrons that do not include protons in their decay products.

• All mesons are unstable• Examples of mesons

include pions (π mesons) and kaons (K mesons)

Page 7: 1.1b Particles & Radiation Quarks & Leptons

Pions or π mesonsPions or π mesons can be positively charged (π+), negatively charged (π - ) or uncharged (π0).

They have rest masses between the muon and proton (about 300 x the electron).

They are all very unstable and decay by the weak interaction.• π+ decays into an antimuon and a neutrino• π - decays into an muon and an antineutrino• π0 decays into two high energy photons

Page 8: 1.1b Particles & Radiation Quarks & Leptons

Kaons or K mesonsKaons or K mesons can be positively charged (K+), negatively charged (K- ) or uncharged (K0).

They have rest masses greater than pions but less than a proton (about 1000 x the electron).

They are all unstable and decay by the weak interaction far more slowly than pions.

This relatively slow rate of decay (about 10 - 10 s) was unexpected and led to these particles being called ‘strange’ particles.

Kaons decay into pions, muons and neutrinos.

Page 9: 1.1b Particles & Radiation Quarks & Leptons

Strangeness• This is a property possessed by some hadrons

that has been assigned in order to explain why some particle interactions take place more slowly than others or do not occur at all.

• The K + meson was the first particle with strangeness to be discovered and has been assigned a strangeness number (S) of +1

• Strangeness is a property, like charge, that is reversed in an antiparticle. Therefore the K - meson has strangeness of – 1.

Page 10: 1.1b Particles & Radiation Quarks & Leptons

Baryon number (B)

Conservation of baryon number

In all interactions the total baryon number is conserved.

You are expected to recall baryon numbers in the AS examination!

antibaryons: (e.g. antiproton)

non-baryons (e.g. mesons and leptons)

baryons: (e.g. protons and neutrons) + 1

- 1

0

Page 11: 1.1b Particles & Radiation Quarks & Leptons

Leptons

• Leptons are believed to be fundamental particles. This means that they do not decay into any other particles except leptons.

• There are three families of leptons and antileptons. In order of increasing rest mass:

1. electrons and their neutrinos

2. muons and their neutrinos

3. tauons and their neutrinos

• Only electrons and their neutrinos are stable.

Page 12: 1.1b Particles & Radiation Quarks & Leptons

Muons (μ-)

• These are negatively charged like electrons but about 200 times more massive

• There also exists the positively charged antimuon (μ+)

• Muons are unstable and decay by the weak interaction into electrons and antineutrinos

• Antimuons decay into positrons and neutrinos

• Tauons are heavier versions of muons (about 20 x more massive). You are not expected to know about these in AS physics

Page 13: 1.1b Particles & Radiation Quarks & Leptons

Lepton and antileptons

increasing mass →

leptons

electron e - muon μ - tauon τ -

electron

neutrino νe

muon

neutrino νμ

tauon

neutrino ττ

antileptons

positron e + antimuon μ + antitauon τ +

electron

antineutrino νe

muon

antineutrino νμ

tauon

antineutrino ντ

leptons

electron, e-

electron neutrino, ve

muon, μ-

muon neutrino, vμ

tauon, τ-

tauon neutrino, vτ

anti-leptons

positron, e+

electron

antineutrino, ve

antimuon, μ+

muon

antineutrino, vμ

tauon

antineutrino, vτ

antitauon, τ+

Page 14: 1.1b Particles & Radiation Quarks & Leptons

Lepton number (L)

Conservation of lepton numberIn all interactions the total lepton number is conserved.

Lepton numbers are given in the AS examination

leptons: (electrons, muons and their neutrinos)

+ 1

antileptons: (positrons, antimuons

and their antineutrinos)- 1

non-leptons (e.g. hadrons and photons) 0

leptons: (electrons, muons and their neutrinos)

antileptons: (positrons, antimuons and their antineutrinos)

non-leptons (e.g. hadrons and photons)

+ 1

- 1

0

Page 15: 1.1b Particles & Radiation Quarks & Leptons

Answers:particle matter or

antimatterhadron or

lepton

electromagnetic

interaction ?baryon, meson

or neither

proton matter hadron yes baryon

positron antimatter lepton yes neither

K0 matter hadron no meson

antineutrino antimatter lepton no neither

muon matter lepton yes neither

neutron matter hadron no baryon

hadron yes baryon

antimatter lepton neither

matter no meson

antineutrino neither

matter yes neither

matter hadron no

Complete:

Page 16: 1.1b Particles & Radiation Quarks & Leptons

Particle overview

matter and antimatter

hadrons leptons

baryons mesons

Page 17: 1.1b Particles & Radiation Quarks & Leptons

Interaction conservation rules

All interactions must conserve:

• ENERGY

• CHARGE

• LEPTON NUMBER & TYPE

• BARYON NUMBER

• and with strong interactions only:

STRANGENESS

Page 18: 1.1b Particles & Radiation Quarks & Leptons

Energy and matterAccelerators such as the Large Hadron Collider increase the kinetic energy of particles involved in collisions.

The total energy of the particles before the collision is equal to the rest plus kinetic energies of the particles.

Likewise the total energy of the particles present after the collision.

Using the conservation of energy:

rest energy = total energy + kinetic energy of the products before of the products

The smaller the final kinetic energy the better. This allows more energy to go into particle creation. Head-on collisions such as those with the LHC given the minimum final kinetic energy.

LHC Simulator

Page 19: 1.1b Particles & Radiation Quarks & Leptons

QuestionA proton and an antiproton, both with 1.5 GeV of kinetic energy, make a head-on collision. If the collision only produces K mesons and photons what is the maximum number of K mesons that could be produced? [Take the rest energy of a proton = 938 MeV; K meson = 490 MeV]

Page 20: 1.1b Particles & Radiation Quarks & Leptons

Total energy before collision: = 2 x (rest energy + kinetic energy)= 2 x (938 MeV + 1500 MeV)= 4876 MeVtherefore the number of possible K mesons = 4876 / 490= 9.95but only a whole number of K mesons can be formedtherefore up to 9 K mesons could be formed

The remainder of the energy would emerge in the form of photon and particle kinetic energy.

Page 21: 1.1b Particles & Radiation Quarks & Leptons

Lepton type conservation

The total electron or muon lepton numbers must also be conserved in any interaction.

Example:

The total lepton number on both sides is the same = +1

However, in terms of muons and muon antineutrinos the number changes from +1 to –1

In terms of electrons and electron neutrinos the number changes from 0 to +2

Therefore this interaction is not permitted

Page 22: 1.1b Particles & Radiation Quarks & Leptons

Allowed interactionsBeta-minus decayLepton number before

= 0 Lepton number after

= 0 + 1 – 1 = 0 Muon decayLepton number before = + 1 Lepton number after

= + 1 – 1 + 1 = + 1

n → p + e- + ve

μ- → e- + ve + vμ

Page 23: 1.1b Particles & Radiation Quarks & Leptons

Questions

1. Write an equation for beta-plus decay:

2. Write an equation for μ+ decay:

3. Can the interaction shown below occur?

Yes, lepton numbers: +1 +0 = 0 +1

and it also conserves electron lepton type number

p → n + e+ + ve

μ+ → e+ + ve + vμ

Page 24: 1.1b Particles & Radiation Quarks & Leptons

Sigma particlesThese are all baryons (B= +1) with a strangeness, S of -1.

sigma-plus Σ +

charge = + 1 (equals proton charge)

sigma-zero Σ0 charge = 0

sigma-minus Σ –

charge = - 1(Note: This is NOT the antiparticle of Σ +)

Like all baryons they eventually decay into protons for example: Σ – → n + π - , after which the neutron decays into a proton

Page 25: 1.1b Particles & Radiation Quarks & Leptons

Conservation of strangeness

Strangeness is always conserved in all strong interactions (no leptons involved).

Strangeness is not always conserved in weak interactions.

Strangeness conserved:

S: 0 + 0 → -1 + 1

Page 26: 1.1b Particles & Radiation Quarks & Leptons

Can the following interactions occur ?

π - + n → K - + Σ 0

1.

2.

3.

YES: baryon numbers are: 0 + 1 → 1 + 0

AND strangeness numbers are: 0 + 0 → -1 + 1

NO: baryon numbers are: 0 + 1 ≠ 0 + 0

strangeness numbers are: 0 + 0 ≠ -1 + 0

NO: baryon numbers are: 0 + 1 → 0 + 1

BUT strangeness numbers are: 0 + 0 ≠ -1 + (-1)

Page 27: 1.1b Particles & Radiation Quarks & Leptons

Further interactions to check

4.

YES

5.NO – Charge is not conserved (neither is strangeness)

6.

YESe- + e+ → p + p + ve + ve

Page 28: 1.1b Particles & Radiation Quarks & Leptons

Quarks• Baryons and mesons are not fundamental

particles of matter (unlike leptons) but are composed of smaller particles called quarks.

• Quarks feel the STRONG force (unlike leptons).

• Quarks are never found in isolation but always in pairs or triplets.

Page 29: 1.1b Particles & Radiation Quarks & Leptons

The quark model of hadronsBARYONSConsist of three quarks:

ANTIBARYONSConsist of three antiquarks:

MESONSConsist of a quark-antiquark pair:

q q q

q q q

q q

This is called the ‘Standard Model’.

Page 30: 1.1b Particles & Radiation Quarks & Leptons

Types of quark• There are six types (flavours) of quarks: up (u);

down (d); charm (c); strange (s); top (t) and bottom (b)

• Charm and top quarks are increasingly more massive versions of the up quark.

• Strange and bottom quarks are increasingly more massive versions of the down quark.

• There are also six corresponding antiquarks (anti-up, anti-down etc..).

• Only knowledge of the up, down and strange quarks is required for AS physics.

Page 31: 1.1b Particles & Radiation Quarks & Leptons

Properties of quarkssymbol relative

mass

charge

proton = 1

baryon

number

strangeness

up u 1 + ⅔ + ⅓ 0

down d 2 - ⅓ + ⅓ 0

strange s 40 - ⅓ + ⅓ -1

charm c 600 + ⅔ + ⅓ 0

top t 90 000 + ⅔ + ⅓ 0

bottom b 2000 - ⅓ + ⅓ 0

1

2

40

+ ⅔

- ⅓ + ⅓

+ ⅓

+ ⅓

- ⅓

0

0

- 1

up u

down d

strange s

charm c 600 + ⅔ + ⅓ 0

bottom b 2000 - ⅓ + ⅓ 0

top t 90 000 + ⅔ + ⅓ 0

Antiquarks have the same mass but opposite charge, baryon number and strangeness.

Page 32: 1.1b Particles & Radiation Quarks & Leptons

Protons and neutrons

Protons consist of two up and one down quark (uud)

Charge = + ⅔ + ⅔ - ⅓ = +1

Baryon number = + ⅓ + ⅓ + ⅓ = +1

Neutrons consist of one up and two down quarks (udd)

Charge = + ⅔ - ⅓ - ⅓ = 0

Baryon number = + ⅓ + ⅓ + ⅓ = +1

u

d

u

u

d

d

Page 33: 1.1b Particles & Radiation Quarks & Leptons

Antiprotons and antineutrons

Antiprotons consist of two up antiquarks and one down antiquark (uud)Charge = - ⅔ - ⅔ + ⅓ = -1Baryon number = - ⅓ - ⅓ - ⅓ = -1

Antineutrons consist of one up antiquark and two down antiquarks (udd)Charge = - ⅔ + ⅓ + ⅓ = 0Baryon number = - ⅓ - ⅓ - ⅓ = -1

u u

d

u

d

d

Page 34: 1.1b Particles & Radiation Quarks & Leptons

Sigma particle questionInsert the missing information below:

sigma-plus Σ +

Quarks: uusCharge = + ⅔ + ⅔ - ⅓ = + 1B = + ⅓ + ⅓ + ⅓ = + 1S = 0 + 0 – 1 = – 1 sigma-zero Σ0 Quarks: udsCharge = + ⅔ - ⅓ - ⅓ = 0B = + ⅓ + ⅓ + ⅓ = + 1S = 0 + 0 – 1 = – 1sigma-minus Σ –

Quarks: ddsCharge = - ⅓ - ⅓ - ⅓ = – 1B = + ⅓ + ⅓ + ⅓ = + 1S = 0 + 0 – 1 = – 1

anti-sigma-plus Σ +

Quarks: u u sCharge = - ⅔ - ⅔ + ⅓ = – 1B = - ⅓ - ⅓ - ⅓ = – 1S = 0 + 0 + 1 = + 1 anti-sigma-zero Σ0 Quarks: u d sCharge = - ⅔ + ⅓ + ⅓ = 0B = - ⅓ - ⅓ - ⅓ = – 1S = 0 + 0 + 1 = + 1 anti-sigma-minus Σ –

Quarks: d d sCharge = + ⅓ + ⅓ + ⅓ = + 1B = - ⅓ - ⅓ - ⅓ = – 1S = 0 + 0 + 1 = + 1

Page 35: 1.1b Particles & Radiation Quarks & Leptons

Charged π mesons

These are made up of a quark and an antiquark pair made of up and down quarks and antiquarks

π + = ud

charge = + ⅔ + ⅓ = +1

B = + ⅓ - ⅓ = 0

π - = ud

charge = - ⅔ - ⅓ = -1

B = - ⅓ + ⅓ = 0

Page 36: 1.1b Particles & Radiation Quarks & Leptons

Uncharged π mesonsThese are made up of a quark and an antiquark pair of up, down or strange quarks

π 0 = uucharge = + ⅔ - ⅔ = 0B = + ⅓ - ⅓ = 0S = 0 + 0 = 0

OR π 0 = ddcharge = - ⅓ + ⅓ = 0B = + ⅓ - ⅓ = 0S = 0 + 0 = 0

OR π 0 = sscharge = - ⅓ + ⅓ = 0B = + ⅓ - ⅓ = 0S = -1 + 1 = 0

Page 37: 1.1b Particles & Radiation Quarks & Leptons

K mesonsThese combinations a strange quark along with an up or down quark

normal particles:K+ = us (S = 0 + 1 = +1)

K0 = ds (S = 0 + 1 = +1)

antiparticles:

K- = su (S = - 1 + 0 = - 1)

K0 = sd (S = - 1 + 0 = - 1)

Page 38: 1.1b Particles & Radiation Quarks & Leptons

Meson summary diagram

π –

(du)

π +

(ud)

K +

(us)

K –

(su)

K 0

(ds)

K 0

(sd)

π 0

(uu, dd or ss)

Page 39: 1.1b Particles & Radiation Quarks & Leptons

Answers

name symbol quarks charge B S

proton p u u d + 1 + 1 0

neutron n u d d 0 + 1 0

pion

plusπ + u d + 1 0 0

omega

minusΩ - s s s - 1 + 1 - 3

neutral

lambdaΛ0 u d s 0 + 1 - 1

Complete:

proton

pion plus

neutron

p

n

ud

+ 1

0

0

- 1 + 1

+ 1

+ 1

0

0

- 3

- 1

Page 40: 1.1b Particles & Radiation Quarks & Leptons

Quark interactionsQuarks undergo both strong and weak interactions.

In strong interactions the numbers and types of quark are conserved.

In weak interactions the overall number of quarks can change and individual quarks can change from one type to another.

Page 41: 1.1b Particles & Radiation Quarks & Leptons

Example of a STRONG quark interaction:Quark annihilation

In quark terms the interaction is:

An up quark and an up antiquark annihilate each other in a strong force interaction producing two pions with the release of radiation.

ENERGY: mass-energy is converted into kinetic energy and photonsCHARGE: + 1 – 1 = + 1 – 1 conservedLEPTON NUMBER: strong interaction – no leptons involvedBARYON NUMBER: + 1 – 1 = 0 + 0 conservedSTRANGNESS NUMBER: 0 + 0 = 0 + 0 conservedThis reaction can occur.

u u d + u u d → u d + u d

Page 42: 1.1b Particles & Radiation Quarks & Leptons

Examples of a WEAK quark interaction: 1. Beta-minus decay

With beta-minus decay a neutron (udd) changes into a proton (uud).

This can be represented on a Feynman diagram as a down quark changing into an up quark.

Note: An early version of the text book shows, incorrectly, an electron-neutrino.

d → u + β- + νe

d

uβ-

ve

time

W-

Page 43: 1.1b Particles & Radiation Quarks & Leptons

Examples of a WEAK quark interaction: 2. Beta-plus decay

With beta-plus decay a proton (uud) changes into a neutron (udd).

u → d + β+ + νe

This can be represented on a Feynman diagram as an up quark changing into a down quark.

Note: An early version of the text book shows, incorrectly, an electron-antineutrino.

u

dβ+

ve

time

W+

Page 44: 1.1b Particles & Radiation Quarks & Leptons

Strong or weak interaction ?

Do any of the following occur ?

1) leptons involved

2) total strangeness changes

3) quarks change type

4) W+ or W- exchange particle

NO

YES

STRONG INTERACTION

e.g.: p + p → π + + π -

when a proton undergoes annihilation with an antiproton to produce two pions

WEAK INTERACTIONExample: Beta decay: n → p + e - + νe

Page 45: 1.1b Particles & Radiation Quarks & Leptons

Internet Links• Fifty-Fifty Game on

What particles are positive - by KT - Microsoft WORD

• Hidden Pairs Game on Quark-Lepton Symmetry - by KT - Microsoft WORD

• Sequential Puzzle on Particle Masses order - by KT  - Microsoft WORD .

Page 46: 1.1b Particles & Radiation Quarks & Leptons

Core Notes from Breithaupt pages 18 to 271. What are muons, pions and kaons?

Give their approximate masses and charges.

2. Explain how muons, pions and kaons decay. State what interactions are involved and what is produced.

3. Define what is meant by (a) a hadron; (b) a lepton; (c) a baryon & (d) a meson. Give two examples of each type of particle.

4. How many baryons are stable? Name them.

5. Why is a neutron a baryon?6. What are the two types of neutrinos?7. Explain the lepton rules in (a)

interactions between leptons and hadrons and (b) muon decay

8. Give and explain an example of a non-allowed interaction where lepton number is conserved. (see the ‘weak puzzle’)

9. Copy table 1 on page 25. Define baryons, antibaryons and mesons in terms of quark composition.

10. State the quark compositions of protons, neutrons, antiprotons and the three varieties of pion.

11. Explain beta-minus and beta-plus decay in terms of quark change. Illustrate with Feynman diagrams.

12. Define what is meant by Baryon number. State the baryon numbers of quarks, antiquarks, protons, neutrons, antiprotons and mesons.

13. List the conservation rules that must apply to all interactions. State how strangeness is exceptional.

14. Give and explain an example of an interaction where quarks are annihilated.

Page 47: 1.1b Particles & Radiation Quarks & Leptons

2.1 The Particle Zoo Notes from Breithaupt pages 18 & 19

1. What are muons, pions and kaons? Give their approximate masses and charges.

2. Explain how muons, pions and kaons decay. State what interactions are involved and what is produced.

3. Write a paragraph in each case about (a) the Stanford Linear Accelerator and (b) the LHC at CERN.

4. Try the summary questions on page 19

Page 48: 1.1b Particles & Radiation Quarks & Leptons

2.2 Particle SortingNotes from Breithaupt pages 20 & 21

1. Define what is meant by (a) a hadron; (b) a lepton; (c) a baryon & (d) a meson. Give two examples of each type of particle.

2. How many baryons are stable? Name them.3. Why is a neutron a baryon?

4. Explain how conservation of energy controls which particles are produced in particle collisions.

5. Try the summary questions on page 21

Page 49: 1.1b Particles & Radiation Quarks & Leptons

2.3 Leptons at workNotes from Breithaupt pages 22 & 23

1. What are the two types of neutrinos?2. Explain the lepton rules in (a) interactions

between leptons and hadrons and (b) muon decay

3. Give and explain an example of a non-allowed interaction where lepton number is conserved. (see the ‘weak puzzle’)

4. Try the summary questions on page 23

Page 50: 1.1b Particles & Radiation Quarks & Leptons

2.4 Quarks and antiquarksNotes from Breithaupt pages 24 to 25

1. Copy table 1 on page 25. Define baryons, antibaryons and mesons in terms of quark composition.

2. State the quark compositions of protons, neutrons, antiprotons and the three varieties of pion.

3. Explain beta-minus and beta-plus decay in terms of quark change. Illustrate with Feynman diagrams.

4. Why is it necessary for some particles to be assigned a strangeness number. Show how the strangeness numbers for K-mesons and sigma particles are allocated.

5. Try the summary questions on pages 25

Page 51: 1.1b Particles & Radiation Quarks & Leptons

2.5 Conservation rulesNotes from Breithaupt pages 26 to 27

1. Define what is meant by Baryon number. State the baryon numbers of quarks, antiquarks, protons, neutrons, antiprotons and mesons.

2. List the conservation rules that must apply to all interactions. State how strangeness is exceptional.

3. Give and explain an example of an interaction where quarks are annihilated.

4. Try the summary questions on pages 27