PYQ Vault

Playbook

Thermal Properties of Matter

84 q - 2.13/paper - 17% HARD. 53 of the 84 are radiation — Stefan and Wien as ratio questions.

Questions in the bank
84
q/paper (2024–25 papers)
2.13
Tagged HARD
17%
Subtopics
4

Strand: Long Tail

When you’ll see it

A hot body radiating, a black body and its peak wavelength, a body cooling, a rod or plate expanding, or heat flowing through a slab.

How this chapter is tested

84 q at 2.13 a paper, 17% HARD — and on this paper the chapter is mostly radiation: Radiation — Stefan, Wien, Newton's Law of Cooling, Black Body is 53 of the 84 questions at 23% HARD.

Almost every radiation question is a ratio. Stefan: P = σAeT⁴, so doubling the absolute temperature multiplies the power by 16. Wien: λ_max T = constant, so a hotter body peaks at a shorter wavelength. Newton's law of cooling: the rate of cooling is proportional to the excess temperature, used with the average temperature over an interval.

Thermal expansion (19 q, 11%) is β = 2α and γ = 3α. Conduction (8 q) and calorimetry (4 q) are small and have never produced a HARD question.

The sub-skills

The distinct skills inside the chapter, in the order to learn them.

  • Stefan–Boltzmann

    P = σAeT⁴ with T in kelvin. Net loss to surroundings ∝ T⁴ − T₀⁴.

  • Wien's law

    λ_max T = b ≈ 2.9 × 10⁻³ m K.

  • Newton's law of cooling

    (T₁ − T₂)/t = k[(T₁ + T₂)/2 − T₀]. Use it twice and take the ratio.

  • Expansion

    ΔL = LαΔT; area β = 2α; volume γ = 3α.

Traps to expect

Distractor shapes this chapter reuses. The Traps page covers the patterns that cut across chapters.

  • Using Celsius in Stefan's law

    T⁴ needs kelvin. 227 °C to 727 °C is 500 K to 1000 K: power ×16, not ×(727/227)⁴.

  • Forgetting the surroundings

    A body in a room at T₀ loses net power σAe(T⁴ − T₀⁴). Using T⁴ alone overstates the loss.

Learn it before you drill it

This chapter has full teaching notes — foundations, worked examples, self-checks and a per-subtopic mastery checkpoint. Read the notes once, then drill subtopic by subtopic below.

Thermal Properties of Matter notes

Drill every thermal properties of matter question

84 questions from the bank, scoped to 4 bundled subtopics.

Drill one subtopic at a time

The 4 subtopics this playbook covers, in catalog order.

  • Radiation — Stefan, Wien, Newton's Law of Cooling, Black BodyDrill
  • Thermal Expansion — Linear, Surface, VolumetricDrill
  • Heat Conduction and Thermal ResistanceDrill
  • Calorimetry, Latent Heat, and Heat CapacityDrill

Related playbooks

Often paired with this one — the technique, the trap or the taxonomy overlaps. Drill these next.