Cambridge IGCSE Physics 0625
Chapter 2
Thermal Physics
Explore how particles explain states of matter, temperature, changes of state and thermal energy transfer.
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Table of Contents
Study the topics in order so the particle model supports the later ideas about thermal energy transfer.
Big picture
Chapter Overview
Thermal physics studies matter, temperature, internal energy and the ways thermal energy moves. The chapter begins with the kinetic particle model. In this model, all matter is made of particles whose arrangement, movement and energy explain the observable properties of solids, liquids and gases.
Heating a substance transfers energy to it. This usually increases the kinetic energy of its particles, so its temperature rises. During a change of state, however, energy is used to change particle separation and overcome attractive forces. The temperature remains constant until the change is complete.
Thermal expansion explains why gaps are left in bridges and railway tracks. Specific heat capacity explains why equal masses of different substances require different amounts of energy for the same temperature rise.
Evaporation occurs when energetic particles escape from the surface of a liquid. The particles left behind have a lower average kinetic energy, so the liquid cools.
Thermal energy is transferred through conduction, convection and radiation. Conduction is particularly important in solids, convection occurs in liquids and gases, and infrared radiation can travel through a vacuum. Real situations frequently involve more than one transfer process.
How the topics fit together
Concept Connections
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1
Start with particles
Learn how particle arrangement and motion differ in solids, liquids and gases.
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2
Connect motion to temperature
A higher temperature means a greater average kinetic energy of particles.
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3
Follow energy during heating
Energy may raise temperature, produce expansion or cause a change of state.
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4
Track energy transfer
Use particle collisions, density changes and infrared radiation to explain transfer.
Chapter reference
Key Equations
Use SI units before substituting values and include a unit with every final answer.
| Quantity | Equation | Symbols and units | Course |
|---|---|---|---|
| Specific heat capacity | ΔE = mcΔθ | ΔE in J, m in kg, c in J/(kg °C), Δθ in °C | Core |
| Constant-temperature gas relationship | p1V1 = p2V2 | p is pressure and V is volume. Use consistent units. | Extended |
The gas relationship applies to a fixed mass of gas at constant temperature.
Recommended order
Study Route
Understand the models
Draw particle diagrams and explain observations using particle arrangement, movement and energy.
Master explanations
Use complete cause-and-effect explanations for expansion, evaporation, conduction and convection.
Apply and calculate
Practise specific heat capacity and gas calculations, then apply the transfer processes to unfamiliar situations.
