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NotesPhysics HLTopic 2.1Internal energy and the particle model
Back to Physics HL Topics
2.1.15 min read

Internal energy and the particle model (Physics HL)

IB Physics • Unit 2

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Contents

  • What internal energy is
  • The particle model & states of matter
  • Exam-style question
The big idea: Warm a metal spoon in hot soup and it soon feels hot too — inside, its particles are jiggling faster and tugging harder on each other. The total energy stored in all that jiggling and tugging is the spoon's internal energy.

It is made of two parts:

- their random kinetic energy (KE) — the energy of the particles jiggling and moving about (this sets the temperature); - their intermolecular potential energy (PE) — the energy stored in the forces between the particles (this depends on how far apart they are).
Internal energy — the definition: Internal energy = total random KE of the particles + total intermolecular PE of the particles.

Random KE = energy of the particles' motion. Intermolecular PE = energy stored in the bonds/forces holding particles together or apart.

For a real gas both parts count. (An ideal gas is a model with no forces between particles, so its internal energy is the random KE only.)
Spot it: Temperature tells you about the average random KE of the particles — not the PE.

So heating something up always raises its KE part; the PE part changes mainly when the state changes (solid ↔ liquid ↔ gas).

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The particle model pictures matter as particles with random KE (motion) and intermolecular PE (forces between them). It explains the three states of matter and why solids are usually denser than liquids.

StateParticle spacingParticle motionShape & volume
SolidVery close, in a fixed patternVibrate about fixed positionsFixed shape, fixed volume
LiquidClose, but free to move past each otherMove/slide aroundNo fixed shape, fixed volume
GasFar apartMove fast in all directionsNo fixed shape, fills the container
Why solids are denser than liquids: Density = mass packed into a volume. In a solid the particles are held in a tight, regular pattern — packed closer together than in the same liquid.

More particles in the same space → more mass per volume → higher density. So melting a solid usually makes it less dense (the particles spread out a little).

Density links a substance's mass to its volume. It is a simple quotient (one quantity divided by another), and it is given in the data booklet:

Density = mass ÷ volume. Given in the data booklet.
density (kg m⁻³)
mass (kg)
volume (m³)

m = mass, ρ = density, V = volume. Cover the one you want: two side by side → multiply; one above the other → divide.

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IB-style questionCalculate[3 marks]

200 g of solid wax fills 2.0 × 10⁻⁴ m³. When melted, the same 200 g fills 2.2 × 10⁻⁴ m³. Find the density in each state and say which is denser.

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How this is tested — this micro appears as short explain / identify questions:

Paper 1A

  • A quick MCQ — identify what makes up the internal energy of a real gas (random KE + intermolecular PE).

Paper 2

  • Explain why most substances are denser as solids than as liquids.
  • Read a density–temperature graph for water to identify the temperature of maximum density.
The classic trap: Saying internal energy is only the kinetic (temperature) part, and forgetting the intermolecular PE.
Water is the odd one out: Most liquids get steadily denser as they cool. Water does not.

Water is densest at about 4 °C. Cool it further and it gets less dense, and ice is less dense still — so ice floats.

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IB-style questionIdentify[2 marks]

The graph shows how the density of a sample of water changes as it is warmed from 0 °C. From the graph, identify the temperature at which the water has its maximum density, and state what this tells you about ice compared with liquid water.

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the two contributions that together make up the internal energy of a substance. [2 marks]

Related Physics HL Topics

Continue learning with these related topics from the same unit:

2.1.2Specific heat capacity
2.1.3Latent heat and calorimetry
2.1.4Conduction, convection and radiation
2.2.1Solar radiation, intensity and the solar constant
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