Thermal Properties: Expansion, Calorimetry & Heat Transfer
Apply concepts from Thermal Properties: Expansion, Calorimetry & Heat Transfer to problem-solving. Focus on numerical practice, shortcuts, and real-world applications.
Concept Core
Thermal Expansion
When a body is heated, its dimensions increase due to increased molecular vibrations. Three types of expansion:
Linear Expansion:
- : coefficient of linear expansion (K)
- Typical values: steel K, aluminium K
Area Expansion:
- : coefficient of area expansion;
Volume Expansion:
- : coefficient of volume expansion;
Relation:
Expansion of Holes and Cavities
A hole or cavity in a solid expands exactly as if it were filled with the same material. A metal ring heated gets a larger inner diameter, not smaller.
Thermal Stress
When expansion is constrained: , (covered in JME-08 but relevant here).
Anomalous Expansion of Water
Water has maximum density at 4 degrees C. Between 0 degrees C and 4 degrees C, water contracts on heating (anomalous). Above 4 degrees C, it expands normally. This is crucial for aquatic life — lakes freeze from the top while the bottom stays at 4 degrees C.
Calorimetry
Heat capacity: (J K)
Specific heat capacity: (J kg K)
Molar heat capacity: (J mol K)
Principle of Calorimetry (conservation of energy):
Latent Heat
Latent heat of fusion: — heat required to change unit mass from solid to liquid at constant temperature.
- Water: J kg = 80 cal g
Latent heat of vaporization: — heat required to change unit mass from liquid to gas at constant temperature.
- Water: J kg = 540 cal g
Heat Transfer Mechanisms
1. Conduction:
- : thermal conductivity (W m K)
- : cross-sectional area
- : length of conductor
- Dimensional formula of : [M L T K]
Thermal resistance: (analogous to electrical resistance)
For slabs in series: For slabs in parallel:
2. Convection: Heat transfer by bulk movement of fluid. Natural convection (density-driven) and forced convection (fan/pump driven). Not easily quantified by simple formulas at the JEE level.
3. Radiation: Stefan-Boltzmann Law:
- W m K (Stefan-Boltzmann constant)
For a non-blackbody: (where is emissivity, )
Newton's Law of Cooling (for small temperature excess): where is surrounding temperature. Approximately:
Wien's Displacement Law: Higher temperature shifts peak wavelength to shorter (bluer) wavelengths.
Key Testable Concept
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