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Thermal Properties of Matter

topicmedium9 MCQ

Thermal expansion, specific and latent heat, conduction, convection and radiation with Newton's law of cooling. (Physics › Properties of Bulk Matter, NEET UG syllabus.)

What is Thermal Properties of Matter?

The amount of heat energy required to raise the temperature of a unit mass of a substance by one ° Celsius or one Kelvin.

Key formula / rule: Linear Thermal Expansion

Key points

  • Define and apply coefficients of linear, area, and volume expansion.
  • Calculate heat absorbed or released during temperature changes and phase changes.
  • Distinguish between conduction, convection, and radiation as modes of heat transfer.
  • Apply Fourier's Law of heat conduction, Stefan-Boltzmann Law, and Wien's Displacement Law.

Common exam trap

Confusing specific heat with latent heat; specific heat involves temperature change, latent heat involves phase change.

Definitions

Term

Specific Heat Capacity (c)

Meaning

The amount of heat energy required to raise the temperature of a unit mass of a substance by one ° Celsius or one Kelvin.

Term

Latent Heat (L)

Meaning

The amount of heat energy absorbed or released by a substance during a phase change (e.g., melting, boiling) at a constant temperature.

Term

Thermal Conductivity (k)

Meaning

A measure of a material's ability to conduct heat. Higher k means better conductor.

Term

Emissivity (e)

Meaning

The ratio of the thermal energy radiated by a surface to the thermal energy radiated by a perfect black body at the same temperature and with the same surface area.

Term

Black Body

Meaning

An idealized physical body that absorbs all incident electromagnetic radiation, regardless of frequency or angle of incidence, and emits thermal radiation perfectly.

Term

Anomalous Expansion of Water

Meaning

The unusual property of water where it contracts upon heating from 0°C to 4°C, reaching its maximum density at 4°C, and then expands upon further heating.

Learning objectives

  • Define and apply coefficients of linear, area, and volume expansion.

  • Calculate heat absorbed or released during temperature changes and phase changes.

  • Distinguish between conduction, convection, and radiation as modes of heat transfer.

  • Apply Fourier's Law of heat conduction, Stefan-Boltzmann Law, and Wien's Displacement Law.

  • Understand and apply Newton's Law of Cooling to solve problems.

Formulae

Name

Linear Thermal Expansion

Note

L₀ is initial length, L is final length, α is coefficient of linear expansion, ΔT is temperature change.

Expression

L = L₀(1 + αΔT)

Name

Area Thermal Expansion

Note

A₀ is initial area, A is final area, β is coefficient of area expansion. For isotropic solids, β ≈ 2α.

Expression

A = A₀(1 + βΔT)

Name

Volume Thermal Expansion

Note

V₀ is initial volume, V is final volume, γ is coefficient of volume expansion. For isotropic solids, γ ≈ 3α.

Expression

V = V₀(1 + γΔT)

Name

Heat absorbed/released (temperature change)

Note

Q is heat, m is mass, c is specific heat capacity, ΔT is temperature change.

Expression

Q = mcΔT

Name

Heat absorbed/released (phase change)

Note

Q is heat, m is mass, L is latent heat (fusion or vaporization).

Expression

Q = mL

Name

Rate of Heat Conduction (Fourier's Law)

Note

dQ/dt is heat flow rate, k is thermal conductivity, A is cross-sectional area, dT/dx is temperature gradient. For uniform rod: Q/t = kA(T₁-T₂)/L.

Expression

dQ/dt = -kA(dT/dx)

Name

Stefan-Boltzmann Law (radiated power)

Note

P is power radiated, e is emissivity (0 to 1), σ is Stefan-Boltzmann constant, A is surface area, T is absolute temperature (in Kelvin).

Expression

P = eσAT⁴

Name

Net Power Radiated

Note

T is body temperature, T₀ is surrounding temperature (both in Kelvin).

Expression

Pnet = eσA(T⁴ - T₀⁴)

Name

Wien's Displacement Law

Note

λm is wavelength of peak emission, T is absolute temperature (in Kelvin), b is Wien's constant.

Expression

λm T = b

Name

Newton's Law of Cooling

Note

dQ/dt is rate of heat loss, k is a constant, T is body temperature, T₀ is surrounding temperature. Also expressed as (T₂-T₁)/t = K((T₁+T₂)/2 - T₀).

Expression

dQ/dt = -k(T - T₀)

Prerequisites

  • Basic understanding of temperature and heat.

  • Knowledge of states of matter (solid, liquid, gas) and phase changes.

  • Basic algebra and proportionality concepts.

Common mistakes

  • Confusing specific heat with latent heat; specific heat involves temperature change, latent heat involves phase change.

  • Incorrectly applying units for temperature (Celsius vs. Kelvin) in formulas like Stefan-Boltzmann Law (always use Kelvin).

  • Forgetting the emissivity (e) factor in radiation formulas for non-black bodies.

  • Not understanding the conditions for Newton's Law of Cooling (small temperature difference).

  • Mixing up the coefficients of linear, area, and volume expansion.

Keywords

  • Thermal Expansion

  • Specific Heat

  • Latent Heat

  • Conduction

  • Convection

  • Radiation

  • Stefan-Boltzmann Law

  • Wien's Displacement Law

  • Newton's Law of Cooling

  • Thermal Conductivity

  • Emissivity

  • Anomalous Expansion

Practice preview

  • What is the correct relationship between the coefficient of linear expansion (alpha), coefficient of area expansion (beta), and coefficient of volume expansion (gamma) for an isotropic solid?…

    easy

  • 100 g of water at 80 degree C is mixed with 50 g of water at 20 degree C. Assuming no heat loss to the surroundings, what is the final temperature of the mixture? (Specific heat capacity of water = 4.2 J g^-1 K^-1)…

    medium

  • Two rods of the same length and area of cross-section are joined in series. Their thermal conductivities are K1 and K2. The equivalent thermal conductivity of the combination is:…

    hard