PX154 - B4 - heat transfer mechanisms

[YF 17.6]

conduction

examples of conduction

convection

radiation

P=dQdt=eσAT4

e= surface emissivity
σ=5.67×108Wm2K1 (stefan boltzmann constant)
- all bodies emit and absorb radiation
- we will need a quantum theory to describe it properly - stefan-boltzmann law for blackbodies