3.2.1 - Particles

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Specific Charge

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43 Terms

1

Specific Charge

The ratio of the charge of a particle to its mass measured in C/kg.

Specific Charge = Charge / Mass

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2

What is the Strong Nuclear Force?

The strong nuclear force holds protons and neutrons together to overcome electrostatic forces of repulsion between protons to keep the nucleus together (stable).

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3

Strong Nuclear Force - range

0 - 0.5 fm = repulsive

0.5 - 3 fm = attractive

3 fm = no effect

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4

What is a femtometer?

1 fm = 1 x 10^-15 m

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5

Alpha decay

When the nucleus of an atom emits an alpha particle (2 protons and 2 neutrons)

<p>When the nucleus of an atom emits an alpha particle (2 protons and 2 neutrons)</p>
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Beta (minus) decay

When a neutron in the atom converts into a proton - during which a beta particle (an electron) and an electron anti-neutrino are emitted from the nucleus.

<p>When a neutron in the atom converts into a proton - during which a beta particle (an electron) and an electron anti-neutrino are emitted from the nucleus.</p>
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7

Why were neutrinos theorised?

The conservation of energy in Beta decay.

Beta particles emitted had a range of energies up to a maximum so another particle had to be emitted also to conserve the amount of energy lost by the nucleus.

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8

What is an antiparticle?

For every particle, there is an antiparticle with equal mass and rest energy but all other properties are opposite - e.g charge.

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Antiparticle examples

electron - positron

proton - antiproton

neutron - antineutron

neutrino - antineutrino

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10

What is a Photon?

A small packet of EM radiation. The energy of a photon is given by the eqn:

E = hf

h - planck’s constant

f - frequency

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11

What is annihilation?

When a particle and its corresponding antiparticle meet they annihilate and all their mass gets converted into energy in the form of two photons (to account for the conservation of momentum).

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Annihilation Equation

2hf = 2E

the combined energy of the photons = the rest energy of the particle - antiparticle pair.

therefore -

hf = E

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13

Pair Production

If a photon with sufficient energy passes near an electron or nucleus then it can be converted into a particle - antiparticle pair; these then move away from each other.

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Pair Production - Equation

hf = 2E

one photon produces a particle and antiparticle.

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15

The Four Fundamental Forces

Gravity

Electromagnetic

Strong Nuclear Force

Weak Nuclear Force

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16

Gravitational Force

Gravity affects any particle with mass over an infinite range.

Its exchange particle is the graviton.

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Electromagnetic Force

The EM force affects any charged particle over an infinite range.

Its exchange particle is the (virtual) photon.

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Strong Nuclear Force/ Interaction

The SNF affects hadrons only over a range of 0 - 3fm.

Its exchange particle is the gluon.

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Weak Nuclear Force/ Interaction

The WNF affects all particles over a range of up to 10^-18 m.

Its exchange particle is the W+ or W- Boson.

It is responsible for Beta decay, electron capture and electron - proton collisions.

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20

What are Exchange Particles?

They carry energy and momentum between the particles experiencing the force.

e.g repulsion can be imagined as two people throwing a ball between them causing them both to be pushed apart due to momentum; the ball is the exchange particle.

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WNF - Beta minus Decay

A nucleus converts into a proton and emits a W- boson which then decays into an e- and electron anti neutrino.

<p>A nucleus converts into a proton and emits a W- boson which then decays into an e- and electron anti neutrino.</p>
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WNF - Beta plus Decay

A proton converts into a neutron and emits a W+ boson which decays into a positron and an electron neutrino.

<p>A proton converts into a neutron and emits a W+ boson which decays into a positron and an electron neutrino.</p>
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23

WNF - Electron Capture

When an atomic e- is absorbed by a proton, a neutron and electron neutrino are emitted.

The W+ boson is the exchange particle.

<p>When an atomic e- is absorbed by a proton, a neutron and electron neutrino are emitted.</p><p></p><p>The W+ boson is the exchange particle.</p>
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WNF - electron proton collisions

When an electron and proton collide, a neutron and electron neutrino are emitted.

The W- boson is the exchange particle.

<p>When an electron and proton collide, a neutron and electron neutrino are emitted.</p><p></p><p>The W- boson is the exchange particle.</p>
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25

Classification of particles

All particles are either hadrons or leptons.

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What is a hadron?

A hadron is a sub-atomic particle that interacts through the SNF and is made up of quarks. There are two types of hadron:

Baryons & Antibaryons

Mesons

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27

Baryons

Particles made up of three quarks.

They have a baryon number of +1. Protons (uud) and neutrons (dud) are both examples of baryons

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Antibaryons

Particles made up of three antiquarks.

They have a baryon number of -1.

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Baryon decay

All baryons eventually decay into protons as this is the most stable baryon.

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Mesons

Mesons are quark - antiquark pairs such as kaons or pions. They’re the exchange particle for the Strong Nuclear Interaction.

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Pions

π+ = up and anti-down quark.

π^0 = up , anti-up or down, anti-down, or strange, anti-strange.

π- = down and anti-up quark.

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Neutral Pion Decay

As neutral pions are made by quarks and antiquarks of the same ‘flavour’ they annihilate and form two photons.

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Charged Pion Decay

Decay into a muon and an antimuon neutrino (negative pion) or a antimuon and a muon neutrino (positive pion).

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Kaons

Kaons are another type of meson that last longer before decaying than pions; they’re produced by the SNF and decay via the WNF as they’re ‘strange’ particles.

K+ = up and anti-strange quark.

K^0 = down and anti-strange quark.

(anti) K^0 = strange and anti-down quark.

K- = strange and anti-up quark.

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Kaon decay

Kaons decay into pions or directly into (anti)muons and the equivalent (anti)muon neutrinos.

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Quarks

Quarks are the fundamental particles that all hadrom=ns are composed of. There are three main quarks (up, down and strange).

<p>Quarks are the fundamental particles that all hadrom=ns are composed of. There are three main quarks (up, down and strange).</p>
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Leptons

Leptons are fundamental particles - they cannot be broken down further. Examples include the muon or the electron.

They do not experience the SNF.

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Muons

Muons are negatively charged and have a mass 200x bigger than the electron so is often referred to as a ‘heavy electron’.

It has a corresponding antimuon (”+), muon neutrino and antimuon neutrino.

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Muon decay

Muons decay into electrons (or positrons) and the corresponding (anti)electron neutrino.

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Lepton Number

Leptons have a lepton number = 1

Antileptons have a lepton number = -1

Non-leptons have a lepton number = 0

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41

Baryon Number

Baryons have a baryon number = 1

Antibaryons have a baryon number = -1

Non-baryons have a baryon number = 0

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42

Strangeness Number

Anti-strange particles have a strangeness number = 1

Strange particles have a strangeness number = -1

Non-strange particles have a strangeness number = 0

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43

Conservation Rules

During particle interactions, the following must always be conserved:

  • Energy and Momentum

  • Charge

  • Baryon Number

  • Lepton (electron and muon) Number

Strangness is conserved during the SNF but during the WNF it may change by 0, -1 or +1.

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