Physics Contents

Physics by Topic
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Chapter 1. Cosmology

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Solar System Test

1.1 The Solar System

The Sun Test

1.1.1 The Sun

Mercury Test

1.1.2 Mercury

Venus Test

1.1.3 Venus

Earth Test

1.1.4 Earth

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1.1.5 Our Moon

Mars Test

1.1.6 Mars

Jupiter Test

1.1.7 Jupiter

Saturn Test

1.1.8 Saturn

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1.1.9 Uranus

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1.1.10 Neptune

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1.1.11 Pluto

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Milky Way Test

1.2 The Milky Way

Local Galactic Group Test

1.3 Local Galactic Group

The Big Bang Test

1.4 The Big Bang

Stars Test

1.5 Stars

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1.5.1 The Birth of Stars

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1.5.2 Plasma

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1.5.3 Nuclear Fusion in Stars

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1.5.4 The Life of Stars

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1.5.5 Hydrogen Fuelled Stars (Stage I)

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1.5.6 Helium Fuelled Stars (Stage II)

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1.5.7 Carbon Fuelled Stars (Stage III)

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1.5.8 White Dwarf Stars

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1.5.9 Supernova

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1.5.10 Neutron Stars

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1.5.11 Pulsars

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1.5.12 Black Holes

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Chapter 2. Particle Physics

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Standard Model Test

2.1 The Standard Model of Particle Physics

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2.1.1 The discovery of sub-atomic particles

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2.1.2 Electron Shells

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2.1.3The Photoelectric Effect

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2.1.4 Dirac’s Prediction of Antimatter

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2.1.5 The discovery of anti-matter

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2.1.6 Particle Accelerators

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2.1.7 Hadrons

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2.1.8 Baryons

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2.1.9 Mesons

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2.1.10 The Standard Model

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2.1.11 Fermions

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2.1.12 Quarks

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2.1.13 Leptons

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2.1.14 Fundamental Forces and Force Carrying Particles

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2.1.15 Bosons

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2.1.16 Photons (y) โ€“ The Electromagnetic Force

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2.1.17 Gluons (g) โ€“ The Strong Force

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2.1.18 Z and W Bosons – The Weak Force

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2.1.19 Gravity and the Higgs Boson

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Atoms Test

Chapter 3. Atoms

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3.1 Diagram of an atom

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3.2 Electrons

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3.3 Discovery of Electrons

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3.4 Properties of Electrons

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3.5 Protons

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3.6 Discovery of Protons

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3.7 Properties of Protons

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3.8 Neutrons

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3.9 Discovery of Neutrons

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3.10 Properties of Protons

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Chapter 4. Isotopes

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4.1 What Are Isotopes?

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4.2 How are isotopes formed?

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4.3 Stable Isotopes

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4.4 Unstable Isotopes (Radioactive Isotopes)

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4.4 Alpha Radiation or Alpha Decay

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4.5 Beta Radiation or Beta Decay

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4.6 Radioactive half-life

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Chapter 5. Decay Chains

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Chapter 6. Nuclear Reactions

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6.1 What are Nuclear Reactions?

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6.2 Nuclear Fusion (summary)

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6.3 Nuclear Fission (summary)

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6.4 Forces That Hold Atoms Together

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6.5 How Nuclear Reactions Produce Energy

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Chapter 7. Nuclear Fusion

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7.1 What is Nuclear Fusion

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7.2 Overcoming the Electromagnetic Forces

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7.3 Nuclear Fusion in Stars

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7.4 Energy Production through Nuclear Fusion

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Chapter 8. Nuclear Fission

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8.1 Energy Production in Nuclear Fission

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8.2 Induced Nuclear Fission

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8.3 Nuclear Fission Reactors

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8.4 Why use Uranium for Nuclear Fission

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8.5 Difficulties with Nuclear Fission as an Energy Source

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8.6 Nuclear Fission and the Environment

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8.7 Plutonium Fast Breeder Reactors

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Chapter 9. Binding Energy

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9.1 Nuclear Binding Energy

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9.2 Calculating Binding Energy

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9.3 Calculating the Assumed Mass

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9.4 Binding Energy Per Nucleon

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Chapter 10. Radiactive Dating

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10.1 What is Radioactive Dating?

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10.2 Carbon Dating

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10.3 Geological Dating

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10.4 Isotopes used in Geological Dating

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10.5 Radioactive Dating with Uranium-238

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Cepheid Variables

Cepheid Variables

        What are Cepheid Variables? Why are they useful? Measuring the Milky Way Hubble’s work with Cepheid Variables Existence of other galaxies The Expanding Universe Dark Energy Dating the Universe     What are Cepheid Variables?...

Atoms

Atoms

It was believed for a thousand years that atoms were the smallest component of matter, but in the late 19th century, the first evidence that atoms were made up of smaller sub-atomic particles came to light.     About Atoms Diagram of an atom Electrons...

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