Atomic Model and Wave-Particle Duality

Summaries for Emission by Black Bodies(Thermal Radiation)1. Hotter objects emit more total radiation per unit surfacearea.‣ Stefan-Boltzmann’s Law2. Hotter objects emit bluer photons (with a higher frequencyν and average energy.)‣ Wien’s Displacement Law:‣ λ max = 2.9 x 10 6 / T(K) [nm]No need to know what the object is, just itstemperature T.But what is the exact form of the function f(ν/T)?27