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c059741
NotesPhysics HLTopic 2.3
Unit 2 · The particulate nature of matter · Topic 2.3

IB Physics HL — Gas laws

Topic 2.3 of IB Physics covers Gas laws, which is part of Unit 2: The particulate nature of matter. Students explore key concepts including Pressure, volume and temperature relationships, Ideal gas law, moles and Avogadro, Kinetic model of an ideal gas. A strong understanding of gas laws is essential for IB Physics HL exams and builds the foundation for connected topics across the syllabus.

Higher Level students should use this topic hub as a map: start with the shared sub-topics, then follow the HL-only extensions and exam-skill links where this topic asks for deeper analysis.

Exam technique guidePractice questions

Key concepts in Gas laws

Key Idea: This topic is about a gas's pressure P, volume V, temperature T and how much gas there is — and the handful of equations that tie them together. Hold one quantity fixed and the others are linked (the gas laws); count the particles and the ideal gas law PV = nRT = N kB T does it all at once; zoom in and the kinetic model explains why — pressure is particles hitting the walls and temperature is their average kinetic energy. It is examined on both papers — quick Paper 1A multiple-choice (compare two samples, P-against-1/V graphs, 'same T → same average KE') and longer Paper 2 structured questions (a before/after gas-law calculation, find moles or molecules, or explain the particle picture in words). One trap runs through the whole topic: temperature must be in kelvin.

📋 Key formulas

Every equation here is given in the data booklet — look for the booklet badge. There is nothing to memorise; the skill is choosing the right form and putting T in kelvin.

PVT=constant\frac{PV}{T} = \text{constant}TPV​=constant
Combined gas law for a fixed amount of gas. Given. Used as a before/after pair: P₁V₁ ÷ T₁ = P₂V₂ ÷ T₂. T is the absolute (kelvin) temperature.
PPP
pressure of the gas (Pa)
VVV
volume of the gas (m³)
TTT
absolute temperature (K) — always in kelvin
PV=nRT=NkBTPV = nRT = N k_B TPV=nRT=NkB​T
Ideal gas law. Given. Use the n-form (moles with R) OR the N-form (molecules with k_B) — never mix them. T in kelvin.
PPP
pressure (Pa)
VVV
volume (m³)
nnn
amount of gas, in moles (mol)
RRR
molar gas constant, 8.31 J K⁻¹ mol⁻¹ (given)
NNN
number of molecules (a plain count, no unit)
kBk_BkB​
Boltzmann constant, 1.38 × 10⁻²³ J K⁻¹ (given)
TTT
absolute temperature (K — kelvin)
n=NNAn = \frac{N}{N_A}n=NA​N​
Converts between the amount in moles and the raw number of molecules. Given. N_A = 6.02 × 10²³ per mole, so N = n × N_A.
nnn
amount of gas, in moles (mol)
NNN
number of molecules (a plain count)
NAN_ANA​
Avogadro constant, 6.02 × 10²³ mol⁻¹ (given)
Ek‾=32kBT\overline{E_k} = \tfrac{3}{2}k_B TEk​​=23​kB​T
Average kinetic energy of ONE particle. Given. Depends only on T (in kelvin) — not on the gas or its mass.
Ek‾\overline{E_k}Ek​​
average kinetic energy of ONE particle (J)
kBk_BkB​
Boltzmann constant, 1.38 × 10⁻²³ J K⁻¹ (given)
TTT
absolute temperature (K — kelvin)

⚖️ The three gas laws

Each gas law is the combined law PV ÷ T = constant with one quantity held fixed so it cancels. Boyle's needs no kelvin (no T in it); the other two must use kelvin.

LawHeld fixedWhat stays constantIn words
Boyle'stemperature TP × Vsqueeze it (V down) → pressure up. Halve V → double P.
Charles'pressure PV ÷ Theat it → it expands. Double the kelvin T → double V.
Gay-Lussac'svolume VP ÷ Theat a sealed rigid can → pressure up. Double the kelvin T → double P.
Boyle's law P V = K rearranges to P = K × (1/V). So a graph of P against 1/V (at fixed temperature) is a straight line through the origin whose slope is K. Its SI unit is pressure × volume = Pa m³ = J (the joule). This is the classic Paper 1B data-handling task.

🔢 The three constants (don't mix them up)

ConstantSymbol & valueGoes with…What it does
Molar gas constantR = 8.31 J K⁻¹ mol⁻¹the moles form: PV = nRTLinks P, V, T to the amount in moles.
Boltzmann constantkB = 1.38 × 10⁻²³ J K⁻¹the molecules form: PV = NkBT, and Ēₖ = (3/2)kBTLinks to the number of molecules, and to the energy of one particle.
Avogadro constantNA = 6.02 × 10²³ mol⁻¹the bridge n = N ÷ NAHow many particles in one mole — converts moles ↔ molecules.
R and kB describe the same gas, so the two forms PV = nRT and PV = NkBT must agree. Since N = n NA, that forces R = NA × kB. Check: 6.02 × 10²³ × 1.38 × 10⁻²³ = 8.31 ✓ — exactly the molar gas constant.

✏️ Worked exam-style questions

IB-style questionDetermine[3 marks]

A balloon holds 2.0 m³ of gas at a pressure of 100 kPa and a temperature of 27 °C. It is taken to a place where the pressure is 150 kPa and the temperature is 177 °C. Find the new volume of the gas.

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IB-style questionDetermine[4 marks]

An aerosol can holds gas at 200 kPa at 27 °C. It is left in the sun and warms to 87 °C. The can is rigid (fixed volume). (a) Find the new pressure. (b) Find the percentage increase in pressure.

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IB-style questionDetermine[4 marks]

A flask contains an ideal gas at a pressure of 2.0 × 10⁵ Pa in a volume of 3.0 × 10⁻⁴ m³ at a temperature of 27 °C. Taking kB = 1.38 × 10⁻²³ J K⁻¹ and NA = 6.02 × 10²³ mol⁻¹, find (a) the number of molecules N and (b) the amount of gas in moles.

🔒 Model answer plan

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IB-style questionDetermine[4 marks]

(a) A sample of neon is at 227 °C. With kB = 1.38 × 10⁻²³ J K⁻¹, find the average kinetic energy of one neon atom. (b) A sample of argon (heavier atoms) sits beside it at the same 227 °C. Compare the average kinetic energy of an argon atom with that of a neon atom.

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🧠 Quick self-check

Tap each card to reveal the answer.

Halve a gas's volume at constant temperature — what happens to its pressure? It doubles. Boyle's law: P × V stays constant, so V → V/2 forces P → 2P.

What unit must temperature be in for any gas-law formula? Kelvin (K). Convert from Celsius by adding 273 (27 °C = 300 K). This is the single most-common slip in the whole topic.

Which constant goes with the number of molecules N, and which with moles n? N pairs with the Boltzmann constant kB; n pairs with the molar gas constant R. Never mix them in one equation.

How many particles are in one mole, and how do you get N from n? 6.02 × 10²³ (the Avogadro constant NA). Multiply: N = n × NA.

What does the pressure of a gas actually come from? Particles colliding with the walls — billions of tiny pushes add up to a steady force per unit area. Faster or more frequent collisions → higher pressure.

Two different gases at the same temperature — same average kinetic energy? Yes. Ēₖ = (3/2)kB T depends only on T, not on the gas. The heavier gas's particles just move slower.


🎯 Exam tips

Exam Tips

  • Temperature ALWAYS in kelvin (K = °C + 273) before any gas-law or kinetic formula. Scaling on the Celsius numbers is the classic trap — pressure and volume scale with the kelvin temperatures.
  • For a before/after change, write the combined law P₁V₁ ÷ T₁ = P₂V₂ ÷ T₂. Whatever is held fixed cancels: fixed T → Boyle (P₁V₁ = P₂V₂); fixed P → Charles; fixed V → Gay-Lussac.
  • Ideal gas law: use n with R (8.31), or N with kB (1.38 × 10⁻²³) — never mix the two forms in one equation.
  • To compare two samples, write PV = NkT (or nRT) for each and DIVIDE one by the other — any equal quantity (P, V or T) cancels, leaving a clean ratio.
  • Convert moles ↔ molecules with n = N ÷ NA (NA = 6.02 × 10²³). To get N from n you multiply: N = n × NA.
  • A graph of P against 1/V (fixed temperature) is a straight line through the origin; its slope is the Boyle constant K, with SI unit Pa m³ = J.
  • Average kinetic energy Ēₖ = (3/2)kB T depends ONLY on the kelvin temperature — same T means the same average KE for any gas; heavier particles just move slower.
  • Pressure comes from particles hitting the walls; compressing a gas quickly does work on it, raising the particles' average KE — so a higher temperature and faster particles.

What you'll learn in Topic 2.3

  • 2.3.1 Pressure, volume and temperature relationships
  • 2.3.2 Ideal gas law, moles and Avogadro
  • 2.3.3 Kinetic model of an ideal gas
Suggested study order: Read the notes for each sub-topic below → test yourself with flashcards → attempt practice questions → review exam technique.

Study resources — 2.3 Gas laws

2.3.1

Pressure, volume and temperature relationships

Notes
2.3.2

Ideal gas law, moles and Avogadro

Notes
2.3.3

Kinetic model of an ideal gas

Notes

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Topic 2.3 Gas laws forms a core part of Unit 2: The particulate nature of matter in IB Physics HL. Mastering these concepts will strengthen your understanding of connected topics across the syllabus and prepare you for exam questions that require analysis, evaluation, and real-world application.

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