IB Chemistry SL Topic 1 — The Behaviour of Ideal Gases Paper 1 & 2 Core idea ~8 min read

Real Gas Behaviour

The ideal gas model makes two convenient assumptions that aren’t quite true. Real gases have particles that take up space and attract one another — so under some conditions they drift away from PV = nRT. Knowing when and why is a classic exam point.

📘 What you need to know

When real gases deviate

The two assumptions behind PV = nRT — that particles take up no space and feel no attractions — are good approximations most of the time. But they break down under two conditions:

PV / RT PRESSURE ideal 200K 500K 1000K
Real gases deviate most at low temperature and high pressure — the 200 K curve strays furthest from the ideal line; 1000 K stays closest.

The volume assumption

An ideal gas is assumed to have particles that take up no space at all. That’s fine when they’re far apart — but at high pressure the particles are pushed close together, and the space they physically occupy becomes a real fraction of the container. Less free space for movement means the gas no longer follows the ideal law.

LOW PRESSURE lots of empty space HIGH PRESSURE particle volume now matters
At high pressure the particles are crowded together, so the space they take up is a significant fraction of the container.

The attraction assumption

An ideal gas is also assumed to have no forces between particles. In reality there are weak attractions. At low temperatures the particles move slowly enough for those attractions to take hold — pulling particles slightly towards each other reduces how hard and how often they hit the walls, so the real pressure is lower than the ideal equation predicts.

Notice the neat symmetry: high pressure exposes the volume assumption, and low temperature exposes the attraction assumption. Both are minimised — and the gas behaves most ideally — at low pressure and high temperature.

💡 Exam tip

That completes The Behaviour of Ideal Gases — and with it, the whole of Topic 1, Models of the Particulate Nature of Matter. Next you’ll move into Topic 2, Models of Bonding & Structure.

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