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JEE · NEET Physics

Class 11 · Chapter 11

Thermal Properties of Matter

Overview, notes, short notes, formula sheet, daily practice problems, previous year questions, and videos for this chapter — all in one place.

Thermal Properties of Matter Formula Sheet

9 formulas across 3 topics in Thermal Properties of Matter.

1 min read

Updated 2026-07-04 · v1.0.0

Temperature Scales & Thermal Expansion

Temperature scales are linear maps of each other; expansion coefficients are linked by the simple chain α : β : γ = 1 : 2 : 3.

C/5 = (F − 32)/9 = (K − 273.15)/5

Temperature scale conversion

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
C, F, Ktemperature in Celsius, Fahrenheit, Kelvin°C, °F, K[Θ]

Valid when

  • −40° is the same on Celsius and Fahrenheit

Common mistakes

  • A temperature DIFFERENCE of 1 °C equals a difference of 1 K but 1.8 °F — conversions differ for readings vs differences

ΔL = L α ΔT; α : β : γ = 1 : 2 : 3

Thermal expansion (linear, areal, volumetric)

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
αcoefficient of linear expansionK⁻¹ (or °C⁻¹)[Θ⁻¹]
βareal coefficient (= 2α)K⁻¹[Θ⁻¹]
γvolumetric coefficient (= 3α)K⁻¹[Θ⁻¹]
ΔTtemperature changeK (or °C)[Θ]

Valid when

  • Isotropic solids
  • A hole in a plate EXPANDS on heating, exactly like a disc of the same material

Common mistakes

  • Thermal stress in a clamped rod: stress = YαΔT — no ΔL appears because the rod is NOT allowed to expand
  • Apparent expansion of liquid in a vessel: γ(apparent) = γ(liquid) − γ(vessel)

ΔT/T = ½ α Δθ (fractional time change of a pendulum clock)

Pendulum clock error due to temperature

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T ∝ √L with ΔL/L = αΔθ, then binomial approximation

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
ΔT/Tfractional change in the perioddimensionless[M⁰L⁰T⁰]
Δθrise in temperatureK (or °C)[Θ]

Valid when

  • Clock LOSES time in summer (pendulum longer, slower), gains in winter
  • Time lost per day = ½αΔθ × 86400 s

Worth remembering

  • Water is anomalous: it CONTRACTS on heating from 0 °C to 4 °C — maximum density at 4 °C is why lakes freeze from the top

Heat, Calorimetry & Change of State

Heat either raises temperature (mcΔT) or changes phase (mL) — never both at once. Mixture problems are pure bookkeeping of these two.

Q = m c ΔT

Heat for a temperature change

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
Qheat suppliedJ[ML²T⁻²]
cspecific heat capacitywater: 4186 J/(kg·K) ≈ 1 cal/(g·°C)J/(kg·K)[L²T⁻²Θ⁻¹]
ΔTtemperature changeK (or °C)[Θ]

Valid when

  • Principle of calorimetry: heat lost = heat gained (isolated system)

Common mistakes

  • In mixture problems, first CHECK whether all the ice melts (compare available heat with required mL) before assuming a final temperature above 0 °C

Q = m L

Heat for a change of state (latent heat)

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
Llatent heat of fusion/vaporisationice: 3.34 × 10⁵ J/kg; steam: 22.6 × 10⁵ J/kgJ/kg[L²T⁻²]

Valid when

  • Temperature stays CONSTANT during the phase change

Common mistakes

  • Steam at 100 °C burns far worse than water at 100 °C — it carries the huge latent heat of vaporisation extra

Worth remembering

  • The classic mixture: equal masses of ice at 0 °C and steam at 100 °C end as ALL water at 100 °C with some steam left — steam's latent heat dominates

Heat Transfer — Conduction, Radiation & Cooling

Conduction is Ohm's law with temperature in place of voltage; radiation follows Stefan's T⁴ law; Newton's cooling is its small-difference limit.

H = dQ/dt = kA(T₁ − T₂)/L

Rate of heat conduction

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
Hheat currentW[ML²T⁻³]
kthermal conductivity of the materialW/(m·K)[MLT⁻³Θ⁻¹]
Across-sectional area[L²]
Llength of the conductorm[L]

Valid when

  • Steady state, no lateral loss
  • Thermal resistance R = L/kA — series and parallel rods combine exactly like electrical resistors

Common mistakes

  • Two rods in series: the JUNCTION temperature divides in the ratio of thermal resistances, not lengths alone

P = σ A e T⁴; net loss: P = σAe(T⁴ − T₀⁴)

Stefan-Boltzmann law of radiation

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
σStefan-Boltzmann constantσ = 5.67 × 10⁻⁸ W/(m²·K⁴)W/(m²·K⁴)[MT⁻³Θ⁻⁴]
eemissivity (1 for a perfect black body)dimensionless[M⁰L⁰T⁰]
Tabsolute temperature of the surfaceK[Θ]
T₀temperature of the surroundingsK[Θ]

Valid when

  • Temperatures MUST be in kelvin — the T⁴ makes this unforgiving

Common mistakes

  • Doubling absolute temperature multiplies radiated power by 16, not 2

λ(max) T = b

Wien's displacement law

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
λ(max)wavelength of peak emissionm[L]
bWien's constantb = 2.9 × 10⁻³ m·Km·K[LΘ]

Valid when

  • Hotter body → peak shifts to SHORTER wavelength (red hot → white hot → blue)

Common mistakes

  • λ(max) is where the emission CURVE peaks — it is not the maximum wavelength emitted

dT/dt = −K(T − T₀)

Newton's law of cooling

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Stefan's law linearised for small (T − T₀)

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
Tbody temperature at time tK (or °C)[Θ]
T₀surrounding temperatureK (or °C)[Θ]
Kcooling constant (setup-dependent)s⁻¹[T⁻¹]

Valid when

  • Small temperature excess only
  • Approximate form for intervals: (T₁ − T₂)/t = K[(T₁ + T₂)/2 − T₀]

Common mistakes

  • Cooling is EXPONENTIAL, not linear — equal temperature drops take progressively longer

Worth remembering

  • Good absorbers are good emitters (Kirchhoff) — a black cup of tea cools faster than a shiny one

NEET rotates Stefan-ratio and Newton's-cooling interval questions yearly; JEE builds composite-slab conduction ladders — solve them as resistor networks.

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