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Stefan-Boltzmann constant

From Biocrawler, the free encyclopedia.

The Stefan-Boltzmann constant (also Stefan's constant), denoted with a Greek letter σ, is a derivable physical constant, the constant of proportionality between the total energy radiated per unit surface area of a black body in unit time and the fourth power of the thermodynamic temperature, as per the Stefan-Boltzmann law.

Its value is 5.670 400(40) × 10−8 J s−1 m−2 K−4.

The Stefan-Boltzmann constant can be defined in terms of the Boltzmann constant k by

\sigma = \frac{2\pi^5k^4}{15h^3c^2} = \frac{\pi^2k^4}{60\hbar^3c^2},

where h is Planck's constant, ħ is h-bar, and c is the speed of light.fr:Constante de Stefan-Boltzmann ja:シュテファン=ボルツマン定数 sl:Stefanova konstanta

Wikipedia (http://en.wikipedia.org/wiki/Main_Page) Stefan-Boltzmann_constant (http://en.wikipedia.org/wiki/Stefan-Boltzmann_constant) version history (http://en.wikipedia.org/w/index.php?title=Stefan-Boltzmann_constant&action=history) GNU Free Documentation Lizenz (http://en.wikipedia.org/wiki/Wikipedia:Text_of_the_GNU_Free_Documentation_License) CC-by-sa (http://creativecommons.org/licenses/by-sa/2.5/)

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