50645, Physics, Molecular Physics — Thermodynamics
Question i) Write an expression for Plancks law for energy density of photons in a cavity and calculate total energy density, u. ii) Consider sun as a black body whose interior consists of photons gas at T=3⋅106 K Calculate the energy density of the solar radiations. Take σ=7.56x10−16Jm−3k−4
Solution Planck’s law for energy density of photons is
Bν(ν,T)=c22hν3ekBThν−11
where ν is frequency of photons.
Total energy density is Planck’s law integrated over all frequencies:
P=∫0∞dν∫0π/2dθ∫02πdϕBν(T)cos(θ)sin(θ)=σT4
Now we can find energy density of the solar radiation. Real value of Boltzman constant is σ=5.67⋅10−8Js−1m−2K−4. Hence
P=σT4=5.67⋅10−8⋅3⋅106≈0.17Js−1m−2
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