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Thermal Properties of Matter

Heat and temperature govern the behavior of matter. Bridges expand in summer, food cooks when thermal energy transfers, and water has a remarkably high specific heat.

Feynman Lens

Start with the simplest version: this lesson is about Thermal Properties of Matter. If you can explain the core idea to a friend using everyday language, examples, and one clear reason why it matters, you have moved from memorising to understanding.

Heat and temperature govern the behaviour of matter. A frozen nail is brittle; when heated, it becomes malleable. Bridges expand in summer and contract in winter. Food cooks when thermal energy transfers to it. This chapter explores how matter responds to temperature changes, how heat flows, and the physical foundations of thermal phenomena.

Temperature versus Heat

Temperature measures the average kinetic energy of particles — a property of a state. Heat is energy in transit between systems due to a temperature difference; it is a process, not a quantity stored in a body. SI unit of temperature is the kelvin (K); 0 K is absolute zero. Conversions: T(K) = T(°C) + 273.15; T(°F) = (9/5) T(°C) + 32.

Ideal Gas Law and Absolute Temperature

For an ideal gas, PV = nRT, with R = 8.314 J/(mol·K). At constant V, P ∝ T (Charles's/Gay-Lussac's law); at constant P, V ∝ T. Linear extrapolation of these proportionalities defines the absolute (Kelvin) scale.

Thermal Expansion

Linear expansion: ΔL = α L₀ ΔT. Area expansion: ΔA = β A₀ ΔT with β ≈ 2α. Volume expansion: ΔV = γ V₀ ΔT with γ ≈ 3α for isotropic solids. Water is anomalous: between 0 °C and 4 °C it contracts on heating (maximum density at 4 °C), which is why ice floats and lakes freeze from the top.

Specific Heat Capacity

Q = m c ΔT; SI unit of c is J/(kg·K). Water has c ≈ 4186 J/(kg·K), unusually high — making it a good coolant and stabiliser of climate. Molar heat capacity C = M·c. For an ideal gas: C_p − C_v = R (Mayer's relation); ratio γ = C_p/C_v.

Calorimetry

For an isolated system, heat lost by the hot body = heat gained by the cold body: m₁c₁(T₁ − T_f) = m₂c₂(T_f − T₂). The calorimeter constant accounts for heat absorbed by the container.

Change of State and Latent Heat

During a phase change, temperature stays constant while heat is supplied. Energy needed: Q = m L, where L is the latent heat. For water: L_f ≈ 3.34 × 10⁵ J/kg (fusion), L_v ≈ 2.26 × 10⁶ J/kg (vaporisation). The very high L_v is why sweating is so cooling.

Heat Transfer

Conduction in a steady state through a slab: H = dQ/dt = k A (T_H − T_C)/L, where k is thermal conductivity. Convection involves bulk flow (e.g. land–sea breezes). Radiation: every body emits electromagnetic radiation; the Stefan–Boltzmann law gives radiated power per unit area σ T⁴ for a blackbody (σ = 5.67 × 10⁻⁸ W·m⁻²·K⁻⁴).

Newton's Law of Cooling

For small temperature differences with the surroundings, the rate of cooling is proportional to the excess temperature: dT/dt = −k(T − T_s).

Socratic Questions

  1. Why does pouring boiling water into a thick glass tumbler shatter it, while a thin glass survives?
  1. Why do coastal regions have milder temperatures than inland regions at the same latitude?
  1. Why does ice float on water, and what would happen to lakes in winter if water did not have its density anomaly?
  1. Why is sweating an effective way to cool the body, even when the air is warmer than the skin?
  1. Why does a hot cup of tea cool faster on a windy day than on a still day, even at the same air temperature?

Distinction
Heat vs. temperature
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Temperature is a state property (avg KE per particle, in kelvin). Heat is energy in transit driven by a temperature difference, in joules.
Equation
Ideal gas law
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PV = nRT, R = 8.314 J/(mol·K). Equivalently PV = NkT with k = 1.38 × 10⁻²³ J/K.
Formula
Linear thermal expansion
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ΔL = α L₀ ΔT. For isotropic solids: area coefficient β ≈ 2α; volume coefficient γ ≈ 3α.
Anomaly
Anomalous expansion of water
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Water contracts when heated from 0 °C to 4 °C; density is maximum at 4 °C. Ice floats; lakes freeze from the top.
Definition
Specific heat capacity (c)
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Q = m c ΔT. Heat per unit mass per unit temperature rise. SI unit J/(kg·K). Water: c ≈ 4186 J/(kg·K).
Concept
Latent heat (L)
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Q = m L. Energy per unit mass to change phase at constant temperature. For water: L_f ≈ 3.34 × 10⁵ J/kg, L_v ≈ 2.26 × 10⁶ J/kg.
Principle
Calorimetry (mixture rule)
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In an isolated system, heat lost = heat gained: m₁c₁(T₁ − T_f) = m₂c₂(T_f − T₂).
Equation
Steady-state conduction
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H = dQ/dt = k A (T_H − T_C)/L. k is the thermal conductivity (W/(m·K)).
Law
Stefan–Boltzmann law
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A blackbody radiates power per unit area σ T⁴, with σ = 5.67 × 10⁻⁸ W·m⁻²·K⁻⁴. For a real body: e σ T⁴ (e = emissivity).
Law
Newton's law of cooling
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For small ΔT, dT/dt = −k (T − T_s). Solution: T(t) − T_s = (T₀ − T_s) e^(−kt).
A 2 kg mass of water is heated from 25 °C to 75 °C. The heat absorbed is (c_water = 4186 J/(kg·K)):
  • A 4.19 × 10⁵ J
  • B 8.37 × 10⁵ J
  • C 2.09 × 10⁵ J
  • D 1.05 × 10⁵ J
A steel rod of length 1.000 m at 20 °C is heated to 220 °C. Its new length is (α = 1.2 × 10⁻⁵ K⁻¹):
  • A 1.0012 m
  • B 1.012 m
  • C 1.0024 m
  • D 1.0048 m
How much heat is required to convert 0.5 kg of ice at 0 °C completely to water at 0 °C? (L_f = 3.34 × 10⁵ J/kg)
  • A 6.68 × 10⁴ J
  • B 1.67 × 10⁵ J
  • C 3.34 × 10⁵ J
  • D 6.68 × 10⁵ J
If the absolute temperature of a blackbody is doubled, the total power radiated per unit area becomes:
  • A 2 times
  • B 4 times
  • C 8 times
  • D 16 times
100 g of water at 20 °C is mixed with 100 g of water at 80 °C. Assuming no heat loss, the equilibrium temperature is:
  • A 50 °C
  • B 60 °C
  • C 40 °C
  • D 70 °C