Abstract:The Stefan-Boltzmann (SB) law relates the radiant emittance of an ideal black-body cavity at thermal equilibrium to the fourth power of the absolute temperature T as q = σT 4 , with σ = 5.67 × 10 −8 W m −2 K −4 the SB constant, firstly estimated by Stefan to within 11 per cent of the present theoretical value. The law is an important achievement of modern physics since, following Plnck (1901), its microscopic derivation implies the quantization of the energy related to the electromagnetic field spectrum. Somew… Show more
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