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Topic: 11.1 Atoms, Nuclei and Radiation | Level: A-Level Physics | Reading Time: 50 minutes

1. The α-Particle Scattering Experiment

Background

Before Rutherford's groundbreaking experiment in 1909, physicists believed in the "plum pudding model" proposed by J.J. Thomson. This model suggested that atoms were spheres of positive charge with electrons embedded throughout.

The Experiment

Ernest Rutherford, working with Hans Geiger and Ernest Marsden, designed an elegant experiment to test the structure of the atom. They fired α-particles (helium nuclei) at a thin gold foil and observed their scattering patterns.

Key Observations

  • Most α-particles passed straight through with little or no deflection
  • A small number were deflected through large angles (greater than 90°)
  • Very few (approximately 1 in 8000) were deflected backwards

Conclusions About Nuclear Structure

  • Most of the atom is empty space – explains why most α-particles passed through
  • The nucleus is extremely small – only tiny fraction came close enough to deflect
  • The nucleus contains most of the atom's mass – needed to deflect massive α-particles
  • The nucleus is positively charged – repulsive electrostatic force causes deflection
Size Scale: The nucleus has diameter ≈ 10-15 m, while the atom has diameter ≈ 10-10 m. The nucleus is about 100,000 times smaller than the atom!

2. Simple Model of the Nuclear Atom

The Nucleus (Central Core)

  • Protons: Positive charge +e (+1.60 × 10-19 C)
  • Neutrons: Neutral, no charge
  • Contains virtually all the atom's mass
  • Diameter ~10-15 m
  • Held together by the strong nuclear force

Orbital Electrons

  • Negative charge -e (-1.60 × 10-19 C)
  • Orbit the nucleus in shells or energy levels
  • Very small mass compared to protons and neutrons
  • Occupy space around nucleus (~10-10 m diameter)

Particle Masses

Particle Mass (kg) Mass (u)
Proton 1.673 × 10-27 ≈ 1
Neutron 1.675 × 10-27 ≈ 1
Electron 9.109 × 10-31 ≈ 0.0005
Key Point: Proton and neutron are ~2000 times more massive than electron. In neutral atoms, number of protons = number of electrons.

3. Nucleon Number and Proton Number

Proton Number (Z) – Atomic Number

  • Number of protons in the nucleus
  • Defines the element
  • Determines chemical properties
  • In neutral atom, Z = number of electrons

Nucleon Number (A) – Mass Number

  • Total number of protons and neutrons
  • A = Z + N (where N = neutrons)

Neutron Number (N)

  • Number of neutrons in nucleus
  • N = A - Z
Example: Carbon-12: 126C
  • Proton number (Z) = 6
  • Nucleon number (A) = 12
  • Neutron number (N) = 12 - 6 = 6

4. Isotopes

Definition

Isotopes are atoms of the same element (same Z) with different numbers of neutrons (different A).

Key Characteristics

  • Identical chemical properties – same electron configuration
  • Different physical properties – different masses
  • Variable stability – some stable, some radioactive

Carbon Isotopes Example

  • Carbon-12: 126C (6p, 6n) – stable, most abundant
  • Carbon-13: 136C (6p, 7n) – stable, less abundant
  • Carbon-14: 146C (6p, 8n) – radioactive, carbon dating

Hydrogen Isotopes Example

  • Protium: 11H (1p, 0n)
  • Deuterium: 21H (1p, 1n)
  • Tritium: 31H (1p, 2n) – radioactive

5. Nuclide Notation

Standard Notation

AZX

Where:

  • X = chemical symbol
  • A = nucleon number (top left)
  • Z = proton number (bottom left)

Examples

Notation Name Protons Neutrons
23892U Uranium-238 92 146
23490Th Thorium-234 90 144
42He Helium-4 (α) 2 2
0-1e Electron (β-) - -

6. Conservation Laws in Nuclear Processes

In ALL nuclear reactions:

  1. Nucleon number (A) is conserved – total before = total after
  2. Charge/Proton number (Z) is conserved – total before = total after
Alpha Decay Example:
23892U → 23490Th + 42He
Check:
  • Nucleon: 238 = 234 + 4 ✓
  • Proton: 92 = 90 + 2 ✓
Beta Decay Example:
146C → 147N + 0-1e
Check:
  • Nucleon: 14 = 14 + 0 ✓
  • Proton: 6 = 7 + (-1) ✓

7. Types of Nuclear Radiation

Alpha (α) Radiation

  • Composition: 42He nuclei (2 protons, 2 neutrons)
  • Charge: +2e (positive)
  • Mass: ≈ 4 u (heavy)
  • Ionizing power: Very high
  • Penetration: Very low (stopped by paper)
  • Speed: ~5% speed of light
  • Energy: Discrete (fixed values)

Beta-minus (β-) Radiation

  • Composition: 0-1e (electrons from nucleus)
  • Charge: -e (negative)
  • Mass: ≈ 1/2000 u (light)
  • Ionizing power: Medium
  • Penetration: Medium (stopped by few mm Al)
  • Speed: 30-99% speed of light
  • Energy: Continuous range (0 to Emax)

Beta-plus (β+) Radiation

  • Composition: 0+1e (positrons)
  • Charge: +e (positive)
  • Similar properties to β-
  • Energy: Continuous range

Gamma (γ) Radiation

  • Composition: EM radiation (photons)
  • Charge: Zero
  • Mass: Zero
  • Ionizing power: Low
  • Penetration: Very high (needs thick lead)
  • Speed: Speed of light (3 × 108 m/s)
  • Energy: Discrete values
  • Not deflected by fields

Comparison Summary

Property α β- β+ γ
Charge +2e -e +e 0
Mass 4 u ~1/2000 u ~1/2000 u 0
Ionizing Very high Medium Medium Low
Penetration Very low Medium Medium Very high
Energy Discrete Continuous Continuous Discrete

8. Antiparticles

Definition

An antiparticle has the same mass as its particle but opposite charge.

Key Examples

  • Electron: 0-1e, charge = -e
  • Positron: 0+1e, charge = +e (antiparticle of electron)
  • Proton: charge = +e
  • Antiproton: charge = -e

Annihilation

When particle meets antiparticle, they annihilate, converting mass to energy (gamma rays):

e+ + e- → 2γ

Pair Production

Reverse process - high-energy γ-rays create particle-antiparticle pairs:

γ → e+ + e-

(Requires γ-ray energy ≥ 1.02 MeV)

9. Neutrinos in Beta Decay

The Problem

Early β-decay observations showed:

  • β-particles had continuous energy range (not discrete)
  • Energy and momentum didn't appear conserved
  • Violated fundamental physics principles

The Solution: Neutrinos

In 1930, Pauli proposed neutrinos to explain this. Properties:

  • Symbol: ν (nu)
  • Charge: Zero
  • Mass: Nearly zero
  • Interaction: Very weak (can pass through Earth)
  • Not detected until 1956

Beta-minus Decay

Neutron transforms, emitting electron + antineutrino:

n → p + e- + ν̄e
146C → 147N + 0-1e + ν̄e

Beta-plus Decay

Proton transforms, emitting positron + neutrino:

p → n + e+ + νe

Why Continuous Energy?

Energy is shared between β-particle and (anti)neutrino in variable proportions. This gives β-particles a continuous range from 0 to Emax.

10. Energy in Radioactive Decay

Alpha Decay - Discrete Energy

All α-particles from a specific isotope have the same kinetic energy.

Reason:
  • Two-body decay (α + daughter nucleus)
  • Energy released is fixed
  • Energy sharing ratio is fixed
  • α-particle carries most energy (lighter than daughter)
Example: 238U → 234Th + α

All α-particles have KE ≈ 4.2 MeV

Beta Decay - Continuous Energy

β-particles have continuous range from 0 to Emax.

Reason:
  • Three-body decay (β + neutrino + daughter)
  • Energy shared variably between β and neutrino
  • When neutrino takes most → β has low energy
  • When neutrino takes minimal → β has max energy
Example: 14C → 14N + e- + ν̄e
  • Emax = 156 keV
  • Most β-particles: 0 to 156 keV
  • Average ≈ 49 keV

Energy Spectrum Comparison

Radiation Energy Spectrum Reason
α-particles Discrete Two-body decay
β-particles Continuous Three-body decay (with neutrino)
γ-rays Discrete Fixed nuclear energy levels

11. Radioactive Decay Equations

Alpha Decay

AZX → A-4Z-2Y + 42α
Changes:
  • A decreases by 4
  • Z decreases by 2
  • Element moves 2 places back in periodic table
23892U → 23490Th + 42α
22688Ra → 22286Rn + 42α

Beta-minus Decay

AZX → AZ+1Y + 0-1e + ν̄e
Changes:
  • A stays same
  • Z increases by 1
  • Neutron converts to proton
  • Element moves 1 place forward
146C → 147N + 0-1e + ν̄e
23490Th → 23491Pa + 0-1e + ν̄e

Beta-plus Decay

AZX → AZ-1Y + 0+1e + νe
Changes:
  • A stays same
  • Z decreases by 1
  • Proton converts to neutron
  • Element moves 1 place back
2211Na → 2210Ne + 0+1e + νe

Gamma Decay

AZX* → AZX + γ

(*) = excited state

Changes:
  • No change in A or Z
  • Nucleus drops from excited to lower energy state
  • Often follows α or β decay
Key Points for Equations:
  • Always check: sum of A values equal on both sides
  • Always check: sum of Z values equal on both sides
  • Include neutrino in β-decay for completeness

12. The Unified Atomic Mass Unit (u)

Definition

1 u = exactly 1/12 the mass of a carbon-12 atom

1 u = 1.66054 × 10-27 kg

Alternative Names

  • Atomic mass unit (amu)
  • Dalton (Da)

Why Use It?

Makes atomic masses simple numbers instead of tiny powers of 10:

  • Proton: 1.007276 u ≈ 1 u
  • Neutron: 1.008665 u ≈ 1 u
  • Electron: 0.000549 u ≈ 1/2000 u
  • Carbon-12: exactly 12 u (by definition)

Standard Masses

Particle/Atom Mass (u) Approx
Proton 1.007276 ≈ 1
Neutron 1.008665 ≈ 1
Electron 0.000549 ≈ 1/2000
Carbon-12 12.000000 exactly 12

11.2 Fundamental Particles - Complete Study Guide

Topic: 11.2 Fundamental Particles | Level: A-Level Physics | Reading Time: 40 minutes

1. Quarks - The Building Blocks

What Are Quarks?

Quarks are fundamental particles - they cannot be broken down into anything smaller. They are the basic building blocks of matter, combining to form protons, neutrons, and other particles.

Key Point: Unlike protons and neutrons (which are made of quarks), quarks themselves are truly fundamental - they have no internal structure.

The Six Flavours of Quarks

There are six types (flavours) of quarks, organized in three generations:

Generation Quark Flavours Importance
First (lightest) Up (u) and Down (d) Make up ordinary matter (protons & neutrons)
Second Charm (c) and Strange (s) Found in unstable particles
Third (heaviest) Top (t) and Bottom (b) Very massive, only in high-energy collisions

Properties of Quarks

  • Fractional charges: Quarks have electric charges of +⅔e or -⅓e
  • Never found alone: Quarks are always found in combinations (confinement)
  • Color charge: Quarks carry "color charge" (not actual color) - red, green, or blue
  • Strong force: Held together by the strong nuclear force via gluons
For A-Level: You need to focus primarily on the up (u) and down (d) quarks, as these make up protons and neutrons. Knowledge of the other four flavours is useful for context but not always required in detail.

2. Quark Charges and Antiquarks

Electric Charges of Quarks

Each quark flavour has a specific electric charge (in units of the elementary charge e):

Quark Symbol Charge Approximate Mass
Up u +⅔e ~2-3 MeV/c²
Down d -⅓e ~4-8 MeV/c²
Charm c +⅔e ~1.3 GeV/c²
Strange s -⅓e ~95 MeV/c²
Top t +⅔e ~173 GeV/c²
Bottom b -⅓e ~4.2 GeV/c²
Pattern: Notice that up, charm, and top all have charge +⅔e, while down, strange, and bottom all have charge -⅓e.

Antiquarks

Every quark has a corresponding antiquark with opposite properties:

  • Opposite charge: If a quark has charge +⅔e, its antiquark has -⅔e
  • Same mass: Antiquarks have the same mass as their corresponding quarks
  • Anticolor: Antiquarks carry anticolor (antired, antigreen, antiblue)
Quark Charge Antiquark Charge
u (up) +⅔e ū (anti-up) -⅔e
d (down) -⅓e đ̄ (anti-down) +⅓e
c (charm) +⅔e c̄ (anti-charm) -⅔e
s (strange) -⅓e s̄ (anti-strange) +⅓e
t (top) +⅔e t̄ (anti-top) -⅔e
b (bottom) -⅓e b̄ (anti-bottom) +⅓e
Important: You do NOT need to memorize the properties of charm, strange, top, or bottom quarks for most A-Level exams. However, you MUST know the charges and properties of up and down quarks.

3. Protons and Neutrons - Quark Composition

Protons and Neutrons Are NOT Fundamental

A crucial understanding in particle physics is that protons and neutrons are not fundamental particles - they are made of quarks.

Key Concept: Protons and neutrons are composite particles made up of three quarks each. They belong to a class of particles called baryons.

Proton Quark Composition

A proton consists of two up quarks and one down quark:

Proton = uud

Calculating Proton Charge

Charge calculation:
2 up quarks: 2 × (+⅔e) = +4/3 e
1 down quark: 1 × (-⅓e) = -⅓e
Total charge = +4/3 e - ⅓e = +3/3 e = +e ✓

This confirms the proton has a charge of +1e (or +1.60 × 10-19 C).

Neutron Quark Composition

A neutron consists of one up quark and two down quarks:

Neutron = udd

Calculating Neutron Charge

Charge calculation:
1 up quark: 1 × (+⅔e) = +⅔e
2 down quarks: 2 × (-⅓e) = -⅔e
Total charge = +⅔e - ⅔e = 0 ✓

This confirms the neutron is electrically neutral (charge = 0).

Summary Comparison

Particle Quark Composition Charge Calculation Total Charge
Proton uud (+⅔) + (+⅔) + (-⅓) +e
Neutron udd (+⅔) + (-⅓) + (-⅓) 0
Exam Tip: You should be able to describe protons and neutrons in terms of their quark composition and calculate their charges. This is a common exam question!

Antiproton and Antineutron

The antiparticles of protons and neutrons are made of antiquarks:

  • Antiproton: ūūđ̄ (two anti-up, one anti-down) - charge = -e
  • Antineutron: ūđ̄đ̄ (one anti-up, two anti-down) - charge = 0

4. Hadrons: Baryons and Mesons

What Are Hadrons?

Hadrons are particles made of quarks. There are two main types:

Hadron Definition: Any particle made of quarks that experiences the strong nuclear force.

Baryons - Three Quarks

A baryon is a hadron consisting of three quarks (or three antiquarks for antibaryons).

Properties of Baryons

  • Made of three quarks (qqq)
  • Baryon number = +1 (antibaryons have baryon number = -1)
  • Examples: proton, neutron
  • Relatively stable (protons are stable, neutrons decay outside nucleus)
Baryon Examples:
  • Proton (p): uud - charge +e
  • Neutron (n): udd - charge 0
  • Lambda (Λ): uds - charge 0 (contains strange quark)
  • Sigma+ (Σ+): uus - charge +e
  • Antiproton: ūūđ̄ - charge -e

Mesons - Quark-Antiquark Pairs

A meson is a hadron consisting of one quark and one antiquark.

Properties of Mesons

  • Made of quark-antiquark pair (qQ̄)
  • Baryon number = 0
  • Generally unstable - decay quickly
  • Examples: pions, kaons
Meson Examples:
  • Pion+ (π+): uđ̄ - charge +e
  • Pion- (π-): ūd - charge -e
  • Pion⁰ (π⁰): uū or dđ̄ - charge 0
  • Kaon+ (K+): us̄ - charge +e
  • Kaon- (K-): ūs - charge -e

Calculating Meson Charges

Example 1: Pion+ (π+) = uđ̄
u quark charge: +⅔e
đ̄ antiquark charge: +⅓e (opposite of d quark)
Total: +⅔e + ⅓e = +e ✓
Example 2: Pion- (π-) = ūd
ū antiquark charge: -⅔e
d quark charge: -⅓e
Total: -⅔e - ⅓e = -e ✓

Hadron Classification Summary

Type Composition Baryon Number Examples
Baryon 3 quarks (qqq) +1 Proton (uud), Neutron (udd)
Antibaryon 3 antiquarks (Q̄Q̄Q̄) -1 Antiproton (ūūđ̄)
Meson quark + antiquark (qQ̄) 0 Pions (π+, π-, π⁰), Kaons (K+, K-)
Common Mistake: Don't confuse baryons with mesons! Baryons have THREE quarks, mesons have ONE quark and ONE antiquark.

5. Quark Changes in Beta Decay

Beta Decay at the Quark Level

Beta decay can be understood as transformations of quarks inside nucleons. This gives us a deeper understanding of what's really happening during radioactive decay.

Beta-minus (β-) Decay

In β- decay, a neutron transforms into a proton.

At the Nucleon Level

n → p + e- + ν̄e

At the Quark Level

Looking at the quark composition:

Before: Neutron = udd
After: Proton = uud

What changed? One down quark transformed into an up quark
d → u + e- + ν̄e

Charge Conservation Check

Before:
Down quark charge: -⅓e

After:
Up quark: +⅔e
Electron: -e
Antineutrino: 0
Total: +⅔e - e = +⅔e - 3/3e = -⅓e ✓

Charge is conserved!

Beta-plus (β+) Decay

In β+ decay, a proton transforms into a neutron.

At the Nucleon Level

p → n + e+ + νe

At the Quark Level

Looking at the quark composition:

Before: Proton = uud
After: Neutron = udd

What changed? One up quark transformed into a down quark
u → d + e+ + νe

Charge Conservation Check

Before:
Up quark charge: +⅔e

After:
Down quark: -⅓e
Positron: +e
Neutrino: 0
Total: -⅓e + e = -⅓e + 3/3e = +⅔e ✓

Charge is conserved!

Summary of Quark Changes

Decay Type Quark Change Nucleon Change Particles Emitted
β- decay d → u n → p e- + ν̄e
β+ decay u → d p → n e+ + νe
Key Understanding: Beta decay is fundamentally about quarks changing flavour:
  • β- decay: down quark becomes up quark
  • β+ decay: up quark becomes down quark

The Weak Force

These quark transformations are mediated by the weak nuclear force, one of the four fundamental forces of nature. The weak force is responsible for:

  • Changing quark flavour
  • Beta decay processes
  • Interactions involving neutrinos

6. Leptons - The Other Fundamental Particles

What Are Leptons?

Leptons are fundamental particles that do NOT experience the strong nuclear force. Unlike protons and neutrons (which are made of quarks), leptons are truly fundamental - they have no internal structure.

Key Distinction:
  • Quarks: Experience strong force, found in combinations (protons, neutrons, mesons)
  • Leptons: Do NOT experience strong force, exist independently

The Six Leptons

There are six leptons, organized in three generations:

Generation Charged Lepton Charge Neutrino Charge
First Electron (e-) -e Electron neutrino (νe) 0
Second Muon (μ-) -e Muon neutrino (νμ) 0
Third Tau (τ-) -e Tau neutrino (ντ) 0

Properties of Leptons

Charged Leptons (Electron, Muon, Tau)

  • Charge: -e (or +e for antileptons)
  • Experience: Electromagnetic force, weak force, gravity
  • Do NOT experience: Strong nuclear force
  • Fundamental: No internal structure

Neutrinos (νe, νμ, ντ)

  • Charge: Zero (neutral)
  • Mass: Extremely small (nearly zero)
  • Experience: Only weak force and gravity
  • Interaction: Very weak - can pass through matter easily

Electron - The Most Important Lepton

The electron is the most familiar lepton and crucial for:

  • Atomic structure (orbits nucleus)
  • Chemical bonding
  • Electrical current
  • Beta decay processes
Electron Properties:
  • Symbol: e-
  • Charge: -e (-1.60 × 10-19 C)
  • Mass: 9.109 × 10-31 kg (≈ 0.0005 u)
  • Lepton number: +1
  • Fundamental particle (no internal structure)

Neutrinos in Beta Decay

Neutrinos play a crucial role in beta decay:

  • β- decay: Emits electron antineutrino (ν̄e)
  • β+ decay: Emits electron neutrino (νe)
Beta-minus decay:
n → p + e- + ν̄e

Beta-plus decay:
p → n + e+ + νe

Antileptons

Every lepton has a corresponding antilepton:

Lepton Charge Antilepton Charge
Electron (e-) -e Positron (e+) +e
Electron neutrino (νe) 0 Electron antineutrino (ν̄e) 0
Muon (μ-) -e Antimuon (μ+) +e

Lepton Number Conservation

In all particle interactions, lepton number is conserved:

  • Leptons: lepton number = +1
  • Antileptons: lepton number = -1
  • Non-leptons: lepton number = 0
abel.masitsa.com Works

In quantum chromodynamics (QCD)—the theory describing the strong force—quarks carry a type of “charge” called color charge. It’s not related to actual colors; the names “red,” “green,” and “blue” are just labels to help visualize it.

Here’s the idea:

  1. Three colors: Every quark can have one of three color charges: red, green, or blue. Antiquarks have the corresponding anticolors: antired, antigreen, or antiblue.

  2. Strong interaction: The color charge is what allows quarks to interact via the strong force, mediated by gluons. Gluons themselves also carry color charge, which makes the strong force extremely complex.

  3. Color confinement: Quarks are never found alone because of color confinement. They always combine to form “color-neutral” particles:

    • Baryons (like protons and neutrons) have three quarks—one of each color—so they combine to “white” (neutral).

    • Mesons have a quark and an antiquark, combining a color with its anticolor to be neutral.

So when we say a quark has a color charge, it means it interacts via the strong force and must combine with other quarks in a way that the overall particle is color-neutral.

As Physics Topic 11:Particle Physics

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