Physics Contents

🌌 Introduction to Physics

The Science That Explains How the Universe Works

Physics is the science that seeks to understand the fundamental laws of natureโ€”the forces, energies, and interactions that shape everything from the tiniest particles to the vastness of galaxies. It explores how objects move, why they move, and what rules govern their behavior.

At its heart, physics asks questions like:

  • Why do things fall?

  • How does light travel?

  • What causes electricity and magnetism?

  • What is time, space, energy, and matter?

Often called the “foundation of all sciences,” physics underpins everything from chemistry and biology to engineering and astronomy. Whether it’s explaining why the sky is blue, how bridges stay standing, or how smartphones work, physics provides the framework.

From Isaac Newtonโ€™s laws of motion to Albert Einsteinโ€™s theory of relativity, and from quantum mechanics to black holes, physics challenges us to think bigโ€”and small. It combines deep curiosity with mathematical precision to uncover the rules of reality.

Studying physics not only helps us understand the universeโ€”it equips us with problem-solving skills that drive innovation and technological progress.

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?   Certain stars called Cepheid Variables have changes to their magnitude which increase and decrease at regular intervals (or periods).     This image is from NASA’s Hubble telescope showing RS Puppis, as Cepheid Variable with a period of 40 days and a change in magnitude of around 5 factors.     Why are they useful?   In 1912 American astronomer, Henrietta Leavitt, came up with a way to use the characteristics of Cepheid Variables to calculate their distance.   The periods of changes in magnitude from Cepheid Variables vary from star to star but, if the period is recorded, the variation in magnitude can be used to calculate the distance. Some of these Cepheid Variables were close enough to have their distance measured using the parallax method (see below). Henrietta Leavitt noticed a relationship between the absolute magnitude and the star’s period allowing modern astronomers to accurately calculate the distances of stars far beyond the parallax method.   It is this technique that has allowed modern astronomers to calculate the size and shape of our galaxies, distant galaxies and even help calculate the age of our universe.   The bright blue star is one of 50 cepheid variables used to measure the distance of galaxy NGC 4603 which they inhabit. It is one of the furthest galaxies measured using the method and is believed to reside 107,000,000 light years...

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 Discovery of Electrons Properties of Electrons Protons Discovery of Protons Properties of Protons Neutrons Discovery of Neutrons Properties of Protons     About Atoms         It has been known for a thousand years that all matter is made up of small particles known as atoms, but for much of this time, it was believed that atoms were the smallest component of matter. It was not until the late 19th and early 20th century that the first evidence that atoms were made up of smaller sub-atomic particles came to light.         A = The Nucleus of the atom contains the protons and neutrons. Despite accounting for the majority of an atomโ€™s mass, the nucleus occupies a minute proportion of the total space. The Diameter of the nucleus is approximately 4 femtometres or 4 x 10-15 meters. It is very difficult to measure the diameter of the nucleus because, like our atmosphere, it has no defined edge but gradually fades away.   B = This is mainly just empty space where the electrons orbit the nucleus. Its diameter (and that of the whole atom) is 0.1 nanometres or 0.1 x 10-9 meters.         Here is the chemical symbol for helium as you might see it on a periodic table. The number at the top is known as...

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