Math 2.0

Classical thermodynamics, heat transfer Thermal radiation Theorem

Planck's law

Builds on Black bodyThermal radiationThermodynamic temperatureEmissivity

Statement

Let a black body be in thermal equilibrium at absolute temperature T>0T > 0. Let hh be the Planck constant, cc the speed of light in vacuum and kBk_B the Boltzmann constant. Then, in every direction, its spectral radiance per unit frequency at frequency ν>0\nu > 0 is Bν(ν,T)=2hν3c2 1ehν/(kBT)−1.B_\nu(\nu, T) = \frac{2 h \nu^3}{c^2} \, \frac{1}{e^{h\nu / (k_B T)} - 1}. Here spectral radiance is the emitted power per unit area normal to the direction, per unit solid angle and per unit frequency. Equivalently, the spectral radiance per unit wavelength at wavelength λ>0\lambda > 0 is Bλ(λ,T)=2hc2λ5 1ehc/(λkBT)−1.B_\lambda(\lambda, T) = \frac{2 h c^2}{\lambda^5} \, \frac{1}{e^{hc / (\lambda k_B T)} - 1}.

Remarks

Proof idea: in a cavity, the number of electromagnetic modes per unit volume and unit frequency is 8πν2/c38\pi \nu^2 / c^3. If each mode of frequency ν\nu can hold only energies nhνn h \nu with n=0,1,2,…n = 0, 1, 2, \dots, the Boltzmann distribution gives the mean energy hν/(ehν/(kBT)−1)h\nu / (e^{h\nu/(k_B T)} - 1) per mode. Multiplying gives the energy density uνu_\nu, and the radiance is Bν=c uν/(4π)B_\nu = c \, u_\nu / (4\pi). The second form follows from Bλ ∣dλ∣=Bν ∣dν∣B_\lambda \, |d\lambda| = B_\nu \, |d\nu| with ν=c/λ\nu = c/\lambda.

For hν≪kBTh\nu \ll k_B T the law reduces to the Rayleigh–Jeans law Bν≈2ν2kBT/c2B_\nu \approx 2 \nu^2 k_B T / c^2, and for hν≫kBTh\nu \gg k_B T to Wien's approximation Bν≈(2hν3/c2)e−hν/(kBT)B_\nu \approx (2h\nu^3/c^2) e^{-h\nu/(k_B T)}. Integrating over frequency gives the Stefan–Boltzmann law, and locating the maximum gives Wien's displacement law. Max Planck found the law in 1900.

Going deeper

For a student

The law is the reference spectrum of radiative heat transfer: real surfaces are described by their emissivity relative to it. The two classical limits show where classical physics works: at low frequency equipartition is correct, and at high frequency the quantisation of energy suppresses emission. The same formula describes the cosmic microwave background, which fits a black-body spectrum at about 2.72.7 K.

Reading path

To understand this page from the ground up, read these 5 pages in order. The foundations come first.

Show the path as a graph
Each page uses the pages above it. The colour of the bar on a box shows how strong the evidence is, and the box also gives it as text. The list has the same pages.
  • no evidence level
  1. Black body concept
  2. Emissivity concept
  3. Thermal radiation concept
  4. Thermodynamic temperature concept
  5. Planck's law statement

Where this leads

5 pages build on this one.

Further reading

  1. Web https://en.wikipedia.org/wiki/Planck%27s_law
About this page
TagQKQ0V5S04R
URIm2://QKQ0V5S04R
Kindstatement, theorem
WritingW0 stub
MSC80A21, 78A40, 82B30
StatusThis copy of the site has no build data. Run m2 status QKQ0V5S04R.
AboutBlack body
UsesBlack body, Thermal radiation, Thermodynamic temperature, Emissivity
Same as
Changed3 November 2026

Markdown · JSON · Edit on GitHub

What this page needs for W1

  • an inventory row: the row of the inventory that the node accounts for (0 of 1)
  • a source with a locator (0 of 1)

The writing levels say how complete the text of a page is. They do not measure its truth.

What links here

Used by