IB SL

Thermal Physics and the Particulate Nature of Matter

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How to Use This Guide

  • Thermal Energy and Temperature — internal energy, specific heat capacity, latent heat, and phase diagrams
  • Ideal Gas Laws — Boyle’s, Charles’s, Gay-Lussac’s laws, and the combined ideal gas equation
  • Molecular Model of an Ideal Gas — kinetic theory assumptions, pressure derivation, mean kinetic energy
  • Real Gases and Phase Changes — departure from ideal behaviour, evaporation vs boiling, latent heat explained

Aligned to IB Physics 2025 syllabus — Theme B: The Particulate Nature of Matter (first assessment 2025)


Jump to section: Thermal Energy · Ideal Gas Laws · Molecular Model · Real Gases and Phase Changes · Practice Questions

Videos on this page: Watch: Ideal Gas Law


Section 1: Thermal Energy and Temperature

Internal Energy

Internal energy is the total random kinetic energy and potential energy of all the particles in a substance. It is NOT the same as temperature.

Internal energy = sum of random kinetic energy + intermolecular potential energy of all particles

  • Kinetic energy component: energy of random translational, rotational, and vibrational motion of molecules
  • Potential energy component: energy stored in intermolecular bonds (relevant in liquids and solids)
  • In an ideal gas, the potential energy component is zero — molecules do not interact except during collisions

Temperature vs thermal energy — a source of Paper 1 marks every year. Temperature is a measure of the average random kinetic energy per particle. Thermal energy (heat) is a total quantity for the whole system. A large cold lake contains more internal energy than a small hot cup of tea, even though the tea is at a higher temperature. Never write “temperature = thermal energy.”

The Kelvin Scale and Absolute Zero

The Kelvin scale is the SI temperature scale used in all physics equations.

T(K)=T(°C)+273.15T(°C)+273T(\text{K}) = T(°\text{C}) + 273.15 \approx T(°\text{C}) + 273

  • Absolute zero (0 K = −273.15 °C) is the temperature at which particles have minimum possible kinetic energy (zero in the classical model).
  • You cannot have a temperature below 0 K.
  • Always convert to Kelvin before using any gas law or kinetic theory equation.

Forgetting to convert to Kelvin is the single most common error in thermal physics. A temperature of 27 °C must be entered as 300 K in every equation. The IB mark scheme deducts the mark if you use Celsius in a gas law calculation.

Specific Heat Capacity

Specific heat capacity (cc) is the energy required to raise the temperature of 1 kg of a substance by 1 K (or 1 °C).

Q=mcΔTQ = mc\Delta T

SymbolMeaningSI Unit
QQheat energy transferredJ
mmmasskg
ccspecific heat capacityJ kg1K1\text{J kg}^{-1}\text{K}^{-1}
ΔT\Delta Ttemperature changeK or °C

Worked Example B1 — Heating water:

A kettle contains 1.5 kg1.5 \text{ kg} of water initially at 18 °C18 \text{ °C}. The specific heat capacity of water is 4200 J kg1K14200 \text{ J kg}^{-1}\text{K}^{-1}. Calculate the energy needed to bring the water to boiling point (100 °C).

Given: m=1.5 kgm = 1.5 \text{ kg}, c=4200 J kg1K1c = 4200 \text{ J kg}^{-1}\text{K}^{-1}, ΔT=10018=82 K\Delta T = 100 - 18 = 82 \text{ K}

Q=mcΔT=1.5×4200×82=517,000 J=517 kJQ = mc\Delta T = 1.5 \times 4200 \times 82 = 517{,}000 \text{ J} = 517 \text{ kJ}

Examiner tip: Units for cc are always J kg1K1\text{J kg}^{-1}\text{K}^{-1} — do not write J/kg/K\text{J/kg/K} in an IB paper; use the 1^{-1} superscript notation. Note ΔT\Delta T in K equals ΔT\Delta T in °C, so converting to Kelvin does not change ΔT\Delta T — only the absolute temperature TT needs converting (e.g., for gas laws).

Specific Latent Heat

Specific latent heat (LL) is the energy required to change the phase of 1 kg of a substance at constant temperature.

Q=mLQ = mL

  • Specific latent heat of fusion (LfL_f): solid ↔ liquid (melting/freezing)
  • Specific latent heat of vaporisation (LvL_v): liquid ↔ gas (boiling/condensing)
  • For water: Lf3.34×105 J kg1L_f \approx 3.34 \times 10^5 \text{ J kg}^{-1}; Lv2.26×106 J kg1L_v \approx 2.26 \times 10^6 \text{ J kg}^{-1}
  • During a phase change, temperature is constant — energy goes into breaking/forming intermolecular bonds, not increasing kinetic energy.

Worked Example B2 — Melting ice:

Calculate the total energy needed to convert 0.50 kg0.50 \text{ kg} of ice at 10 °C-10 \text{ °C} to liquid water at 20 °C20 \text{ °C}.

Use cice=2100 J kg1K1c_{\text{ice}} = 2100 \text{ J kg}^{-1}\text{K}^{-1}, Lf=3.34×105 J kg1L_f = 3.34 \times 10^5 \text{ J kg}^{-1}, cwater=4200 J kg1K1c_{\text{water}} = 4200 \text{ J kg}^{-1}\text{K}^{-1}.

Step 1 — heat ice from −10 °C to 0 °C:

Q1=0.50×2100×10=10,500 JQ_1 = 0.50 \times 2100 \times 10 = 10{,}500 \text{ J}

Step 2 — melt ice at 0 °C:

Q2=0.50×3.34×105=167,000 JQ_2 = 0.50 \times 3.34 \times 10^5 = 167{,}000 \text{ J}

Step 3 — heat water from 0 °C to 20 °C:

Q3=0.50×4200×20=42,000 JQ_3 = 0.50 \times 4200 \times 20 = 42{,}000 \text{ J}

Total: Q=10,500+167,000+42,000=219,500 J220 kJQ = 10{,}500 + 167{,}000 + 42{,}000 = 219{,}500 \text{ J} \approx 220 \text{ kJ}

Phase Change Diagram

A heating curve shows temperature vs. energy supplied for a pure substance. Its characteristic shape has two flat regions (phase changes) and three sloping regions (temperature increases in each phase).

  • Slope 1 (solid region): gradient =1/(mcsolid)= 1/(mc_{\text{solid}}). Steeper slope = smaller specific heat capacity.
  • Flat region 1 (melting): temperature is constant at the melting point. Length mLf\propto m L_f.
  • Slope 2 (liquid region): gradient =1/(mcliquid)= 1/(mc_{\text{liquid}}).
  • Flat region 2 (boiling): temperature is constant at the boiling point. Length mLv\propto m L_v.
  • Slope 3 (gas region): steepest, since gases typically have lower specific heat capacities per kg than liquids.

The boiling plateau is always longer than the melting plateau for water (and most substances), because LvLfL_v \gg L_f. Examiners often ask students to sketch heating curves — if you draw the plateaus the same length, you lose marks.


Section 2: Ideal Gas Laws

The Three Empirical Gas Laws

An ideal gas is a theoretical model in which molecules are treated as point masses with no intermolecular forces.

Boyle’s Law (constant TT, fixed amount of gas):

pV=constantp1V1=p2V2pV = \text{constant} \qquad \Rightarrow \qquad p_1 V_1 = p_2 V_2

Charles’s Law (constant pp, fixed amount of gas):

VT=constantV1T1=V2T2\frac{V}{T} = \text{constant} \qquad \Rightarrow \qquad \frac{V_1}{T_1} = \frac{V_2}{T_2}

Gay-Lussac’s Law (constant VV, fixed amount of gas):

pT=constantp1T1=p2T2\frac{p}{T} = \text{constant} \qquad \Rightarrow \qquad \frac{p_1}{T_1} = \frac{p_2}{T_2}

All three combine to give the combined gas law:

p1V1T1=p2V2T2\frac{p_1 V_1}{T_1} = \frac{p_2 V_2}{T_2}

The Ideal Gas Equation

Adding Avogadro’s law (equal volumes of ideal gases at the same TT and pp contain equal numbers of molecules) to the combined gas law gives the ideal gas equation:

pV=nRTpV = nRT

SymbolMeaningValue / Unit
pppressurePa (N m2\text{N m}^{-2})
VVvolumem3\text{m}^3
nnamount of substancemol
RRuniversal gas constant8.31 J mol1K18.31 \text{ J mol}^{-1}\text{K}^{-1}
TTabsolute temperatureK

RR and the equation are given in the IB data booklet. You need to know what each symbol means and be able to rearrange.

Avogadro’s number: NA=6.02×1023 mol1N_A = 6.02 \times 10^{23} \text{ mol}^{-1}. The number of molecules N=nNAN = nN_A. Molar mass (MrM_r, in kg mol1\text{kg mol}^{-1}): mass of substance m=nMrm = nM_r, so n=m/Mrn = m/M_r. Example: 8.0 g of oxygen (Mr=0.032 kg mol1M_r = 0.032 \text{ kg mol}^{-1}) contains n=0.008/0.032=0.25 moln = 0.008/0.032 = 0.25 \text{ mol}.

Worked Example B3 — Gas in a cylinder:

A fixed amount of ideal gas is enclosed in a cylinder. Initially, T1=300 KT_1 = 300 \text{ K}, p1=1.0×105 Pap_1 = 1.0 \times 10^5 \text{ Pa}, and V1=2.0×103 m3V_1 = 2.0 \times 10^{-3} \text{ m}^3. The gas is heated at constant volume until T2=450 KT_2 = 450 \text{ K}.

(a) Find the final pressure p2p_2.

(b) Calculate the number of moles of gas.

(a) Using Gay-Lussac’s Law (constant VV):

p1T1=p2T2    p2=p1×T2T1=1.0×105×450300=1.5×105 Pa\frac{p_1}{T_1} = \frac{p_2}{T_2} \implies p_2 = p_1 \times \frac{T_2}{T_1} = 1.0 \times 10^5 \times \frac{450}{300} = 1.5 \times 10^5 \text{ Pa}

(b) Using pV=nRTpV = nRT:

n=p1V1RT1=1.0×105×2.0×1038.31×300=20024930.080 moln = \frac{p_1 V_1}{RT_1} = \frac{1.0 \times 10^5 \times 2.0 \times 10^{-3}}{8.31 \times 300} = \frac{200}{2493} \approx 0.080 \text{ mol}

Always check: is volume constant, pressure constant, or temperature constant? Identify which law applies before calculating. If two of pp, VV, TT change, use the combined gas law. If you have mass information, find nn first via n=m/Mrn = m/M_r, then use pV=nRTpV = nRT.


Watch: Ideal Gas Law — Khan Academy

Khan Academy · 14 min · Derives the ideal gas equation from the three empirical gas laws, explains the meaning of each variable, and works through pressure-temperature and pressure-volume examples directly relevant to IB Paper 2.


Section 3: Molecular Model of an Ideal Gas

Assumptions of the Kinetic Theory

The kinetic model explains macroscopic gas behaviour (pressure, temperature) in terms of molecular motion.

Six assumptions of an ideal gas (state these precisely in exam answers):

  1. The gas consists of a large number of identical molecules (or atoms for monatomic gases).
  2. Molecules are point masses — their volume is negligible compared with the volume of the container.
  3. Molecules undergo random motion in all directions with a range of speeds.
  4. Collisions between molecules and with container walls are perfectly elastic — no kinetic energy is lost.
  5. There are no intermolecular forces except during collisions.
  6. The duration of collisions is negligible compared with the time between collisions.

Pressure from Molecular Motion

Pressure arises from the force exerted when molecules collide with the container walls. Using Newton’s second law and the impulse of a molecule bouncing off a wall, kinetic theory gives:

pV=13Nmv2pV = \frac{1}{3}Nm\langle v^2 \rangle

where NN is the total number of molecules, mm is the mass of one molecule, and v2\langle v^2 \rangle is the mean square speed.

The root mean square (rms) speed is vrms=v2v_{\text{rms}} = \sqrt{\langle v^2 \rangle}.

You are not required to reproduce the full derivation at SL, but you should be able to describe the physical reasoning (molecular collisions with walls → impulse → force → pressure) and use the result. The formula is in the data booklet.

Mean Kinetic Energy and Temperature

Comparing pV=13Nmv2pV = \frac{1}{3}Nm\langle v^2 \rangle with pV=NkTpV = NkT (where k=R/NAk = R/N_A is the Boltzmann constant):

12mv2=32kT\frac{1}{2}m\langle v^2 \rangle = \frac{3}{2}kT

The average translational kinetic energy of a molecule is directly proportional to absolute temperature.

ConstantValueUnit
kk (Boltzmann constant)1.38×10231.38 \times 10^{-23}J K1\text{J K}^{-1}
RR (gas constant)8.318.31J mol1K1\text{J mol}^{-1}\text{K}^{-1}
Relationshipk=R/NAk = R/N_A

For one mole of gas: mean total kinetic energy =32RT= \frac{3}{2}RT.

Worked Example B4 — rms speed of a gas:

Calculate the rms speed of nitrogen molecules (Mr=0.028 kg mol1M_r = 0.028 \text{ kg mol}^{-1}) at T=300 KT = 300 \text{ K}.

Using 12mvrms2=32kT\frac{1}{2}mv_{\text{rms}}^2 = \frac{3}{2}kT:

vrms=3kTm=3RTMr=3×8.31×3000.028=74790.028=267,000517 m s1v_{\text{rms}} = \sqrt{\frac{3kT}{m}} = \sqrt{\frac{3RT}{M_r}} = \sqrt{\frac{3 \times 8.31 \times 300}{0.028}} = \sqrt{\frac{7479}{0.028}} = \sqrt{267{,}000} \approx 517 \text{ m s}^{-1}

Note: m=Mr/NAm = M_r / N_A for one molecule, so the formula can also be written vrms=3RT/Mrv_{\text{rms}} = \sqrt{3RT/M_r} using molar quantities.

Temperature must be in Kelvin in ALL kinetic theory equations. Also note that 12mv2=32kT\frac{1}{2}m\langle v^2 \rangle = \frac{3}{2}kT gives the average kinetic energy per molecule (using kk), not per mole. For per mole, multiply by NAN_A: EK,mol=32RTE_{K,\text{mol}} = \frac{3}{2}RT.


Section 4: Real Gases and Phase Changes

Departures from Ideal Behaviour

Real gases deviate from ideal gas behaviour because real molecules:

  • Do have a finite volume (so at very high pressure, VV cannot be compressed to zero)
  • Do have intermolecular forces — attractive at moderate distances, repulsive at very short distances

When does a real gas behave most like an ideal gas?

  • High temperature — molecules have enough kinetic energy that intermolecular potential energy is negligible
  • Low pressure — molecules are far apart, so intermolecular forces and finite volume are negligible

When does a real gas deviate most from ideal behaviour?

  • High pressure (molecules close together — volume effect matters)
  • Low temperature — especially near the boiling point (intermolecular attractions significant)

HL The van der Waals equation corrects for real gas behaviour:

(p+an2V2)(Vnb)=nRT\left(p + \frac{an^2}{V^2}\right)(V - nb) = nRT

where aa accounts for intermolecular attractions and bb accounts for the finite volume of molecules. This is beyond SL but useful context.

Evaporation and Boiling

These are two distinct processes by which a liquid becomes a gas.

FeatureEvaporationBoiling
Where it occursSurface onlyThroughout the liquid (bubbles form)
TemperatureAny temperature below boiling pointAt the boiling point (fixed for given pressure)
RateIncreases with temperature, surface area, air flowDepends on heating rate
Effect on liquidCools the liquid (highest-energy molecules escape)Temperature stays constant while boiling

Exam command: “Explain in terms of molecular behaviour why the temperature of a liquid drops during evaporation.” Model answer: The molecules that escape have above-average kinetic energy. The remaining molecules therefore have a lower average kinetic energy. Since temperature is proportional to average kinetic energy, the temperature of the liquid decreases. (3 marks — include: high-energy molecules escape, average KE of remainder decreases, temperature proportional to average KE.)


Exam-Style Practice Questions

Paper 1 Style (MCQ)

Q1. A gas is heated at constant volume. Which of the following correctly describes what happens?

A. The pressure decreases because molecules move faster and collide less frequently.

B. The pressure increases because molecules move faster and hit the walls with greater force and frequency.

C. The volume increases to maintain constant pressure.

D. The number of moles of gas increases.

Answer

B. At constant volume, heating increases the average kinetic energy (speed) of molecules. Molecules hit the walls more frequently and with greater momentum change per collision, so the pressure increases. Option C describes what happens at constant pressure (Charles’s Law), not constant volume.


Q2. An ideal gas is compressed isothermally (at constant temperature) to half its original volume. Which of the following statements is correct?

A. The pressure doubles and the mean kinetic energy of molecules doubles.

B. The pressure doubles and the mean kinetic energy of molecules is unchanged.

C. The pressure halves and the mean kinetic energy of molecules is unchanged.

D. The pressure is unchanged because temperature is constant.

Answer

B. By Boyle’s Law (pV=pV = constant at constant TT), halving VV doubles pp. Mean kinetic energy depends only on temperature (EK=32kTE_K = \frac{3}{2}kT) — since temperature is constant, mean kinetic energy is unchanged. Option D is a common misconception.


Paper 2 Style (Structured Response)

Q3. A sealed container of volume 5.0×103 m35.0 \times 10^{-3} \text{ m}^3 contains an ideal gas at pressure 2.0×105 Pa2.0 \times 10^5 \text{ Pa} and temperature 27 °C27 \text{ °C}.

(a) Show that the number of moles of gas is approximately 0.40 mol. [2]

(b) The temperature is raised to 127 °C127 \text{ °C} at constant volume. Calculate the new pressure. [2]

(c) State and explain the effect on the pressure if the same number of moles of a real gas (rather than an ideal gas) were used under these conditions (high temperature, moderate pressure). [2]

Mark-scheme answers

(a) Convert: T=27+273=300 KT = 27 + 273 = 300 \text{ K}.

n=pVRT=2.0×105×5.0×1038.31×300=100024930.401 mol0.40 moln = \frac{pV}{RT} = \frac{2.0 \times 10^5 \times 5.0 \times 10^{-3}}{8.31 \times 300} = \frac{1000}{2493} \approx 0.401 \text{ mol} \approx 0.40 \text{ mol}

[1 mark for correct substitution with TT in Kelvin; 1 mark for correct answer]

(b) T2=127+273=400 KT_2 = 127 + 273 = 400 \text{ K}. Volume is constant, so Gay-Lussac’s Law applies:

p2=p1×T2T1=2.0×105×400300=2.67×105 Pap_2 = p_1 \times \frac{T_2}{T_1} = 2.0 \times 10^5 \times \frac{400}{300} = 2.67 \times 10^5 \text{ Pa}

[1 mark for method; 1 mark for correct answer with unit]

(c) At high temperature and moderate pressure, the real gas behaves very close to an ideal gas (intermolecular forces negligible, molecular volume negligible compared to container volume). The pressure would be approximately the same as the ideal gas prediction — the deviations are small under these conditions.

[1 mark for stating pressure would be approximately equal; 1 mark for correct reasoning referencing high temperature/moderate pressure meaning ideal behaviour is a good approximation]


Common Theme B errors that cost marks:

  1. Using °C instead of K in gas law and kinetic theory equations — always add 273 (or 273.15).
  2. Confusing Q=mcΔTQ = mc\Delta T (sensible heat) and Q=mLQ = mL (latent heat) — during a phase change, use LL not cc.
  3. Stating “temperature is thermal energy” — temperature is proportional to average kinetic energy per particle.
  4. Forgetting that the mean kinetic energy equation gives energy per molecule (use kk); for per mole, use 32RT\frac{3}{2}RT.
  5. Drawing a heating curve with equal-length plateaus — the vaporisation plateau is always longer than the melting plateau (LvLfL_v \gg L_f).
  6. Describing evaporation incorrectly — it cools the liquid because high-energy molecules escape, lowering the average KE of those remaining.

May 2026 Exam Predictions

Based on past IB Physics paper patterns, Theme B questions in May 2026 are likely to include:

  • Paper 1 MCQ: Boyle’s Law graph interpretation (which graph is correct at constant T), or a temperature/kinetic energy question.
  • Paper 2 Short Answer: A multi-step gas law calculation requiring temperature conversion and identification of the correct law. Likely 4–6 marks total.
  • Paper 2 Extended Answer: An “explain using the molecular model” question (2–3 marks) — most commonly asking students to explain why pressure increases when temperature increases at constant volume, or to explain evaporative cooling at the molecular level.
  • Specific latent heat calculation: Often combined with Q=mcΔTQ = mc\Delta T (calculate total energy to melt ice and warm the resulting water).

Highest-value skill in Theme B: Writing molecular-level explanations. The mark scheme always awards marks for: (1) a specific statement about molecular motion or energy, (2) a link to the macroscopic property being asked about. Vague answers like “the molecules move more” score zero. Precise answers like “the molecules move faster, so they collide with the walls more frequently and with greater change in momentum, increasing the force on the walls” score full marks.