18-6 Heat Transfer Mechanisms

18-6 Heat Transfer Mechanisms#

Prompts

  • Name the three heat transfer mechanisms. For each, describe how energy is transferred.

  • Write the conduction rate equation \(P = kA\,\Delta T/L\). What does \(k\) depend on? Why do metals conduct heat well?

  • What is convection? How does natural convection differ from forced convection?

  • Write the Stefan–Boltzmann law for radiation. Why does \(P \propto T^4\)? What is emissivity \(\varepsilon\)?

  • An object at temperature \(T\) is in an environment at \(T_{\text{env}}\). When does it absorb net radiation? When does it emit net radiation?

Lecture Notes#

Overview#

  • Heat can be transferred by conduction (through a material), convection (by fluid motion), and radiation (by electromagnetic waves).

  • Conduction: energy passed by collisions; rate \(\propto\) area, \(\Delta T\), and \(1/L\); depends on thermal conductivity \(k\).

  • Convection: warmer fluid rises, cooler sinks; buoyancy-driven (natural) or forced.

  • Radiation: no medium needed; \(P \propto T^4\); works in vacuum (e.g., Sun to Earth).


Conduction#

Energy flows through a material by collisions between atoms and electrons. The conduction rate (power) through a slab of area \(A\), thickness \(L\), with temperature difference \(\Delta T = T_H - T_C\):

(159)#\[ P_{\text{cond}} = kA\,\frac{\Delta T}{L} \]
  • \(k\): thermal conductivity (W/(m·K)); material property.

  • High \(k\): good conductor (metals). Low \(k\): good insulator (foam, air, fiberglass).

Thermal resistance: \(R = L/k\). Higher \(R\) → better insulator.

Material

\(k\) (W/(m·K))

Copper

401

Aluminum

235

Iron

67

Glass

~1

Air

0.026

Foam

~0.02


Convection#

Heat is carried by bulk motion of a fluid (gas or liquid). Warmer fluid near a hot surface expands, becomes less dense, and rises; cooler fluid replaces it.

  • Natural convection: driven by buoyancy (density differences). Examples: candle flame, room heating, atmospheric circulation.

  • Forced convection: fluid is pumped or blown (e.g., fan, wind).


Radiation#

Energy transferred by electromagnetic waves. No medium required—works in vacuum.

Stefan–Boltzmann law (emission rate):

(160)#\[ P_{\text{rad}} = \sigma \varepsilon A T^4 \]
  • \(\sigma = 5.67 \times 10^{-8}\) W/(m²·K⁴)—Stefan–Boltzmann constant.

  • \(\varepsilon\): emissivity (\(0 \le \varepsilon \le 1\)); \(\varepsilon = 1\) for ideal blackbody.

  • \(T\) in kelvins. Any object with \(T > 0\) K emits radiation.

Net radiation (object at \(T\) in environment at \(T_{\text{env}}\)):

(161)#\[ P_{\text{net}} = \sigma \varepsilon A (T_{\text{env}}^4 - T^4) \]
  • \(T_{\text{env}} > T\) → net absorption. \(T_{\text{env}} < T\) → net emission.


Summary#

  • Conduction: \(P = kA\,\Delta T/L\); energy by collisions; \(k\) = thermal conductivity.

  • Convection: heat by fluid motion; natural (buoyancy) or forced.

  • Radiation: \(P = \sigma \varepsilon A T^4\); no medium; \(P \propto T^4\).