Stefan–Boltzmann constant: Difference between revisions
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The value of the Stefan–Boltzmann constant is derivable as well as experimentally determinable; see [[Stefan–Boltzmann law]] for details. It can be defined in terms of the [[Boltzmann constant]] ''k''<sub>B</sub> as: |
The value of the Stefan–Boltzmann constant is derivable as well as experimentally determinable; see [[Stefan–Boltzmann law]] for details. It can be defined in terms of the [[Boltzmann constant]] ''k''<sub>B</sub> as: |
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:<math>\sigma = \frac{2\pi^5k_{\rm B}^4}{15h^3c_0^2} = \frac{\pi^2k_{\rm B}^4}{60\hbar^3c_0^2}</math> |
:<math>\sigma = \frac{2\pi^5k_{\rm B}^4}{15h^3c_0^2} = \frac{\pi^2k_{\rm B}^4}{60\hbar^3c_0^2}</math> |
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where ''k<sub> |
where ''k<sub>B</sub>'' is the [[Boltzmann constant]], ''h'' is the [[Planck constant]], ''ħ'' is the reduced Planck constant, and ''c''<sub>0</sub> is the [[speed of light]] in a vacuum. The [[CODATA]] recommended value is calculated from the measured value of the [[gas constant]] ''R'': |
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:<math>\sigma = \frac{2 \pi^5 R^4}{15 h^3 c_0^2 N_{\rm A}^4} = \frac{32 \pi^5 h R^4 R_{\infty}^4}{15 A_{\rm r}({\rm e})^4 M_{\rm u}^4 c_0^6 \alpha^8}</math> |
:<math>\sigma = \frac{2 \pi^5 R^4}{15 h^3 c_0^2 N_{\rm A}^4} = \frac{32 \pi^5 h R^4 R_{\infty}^4}{15 A_{\rm r}({\rm e})^4 M_{\rm u}^4 c_0^6 \alpha^8}</math> |
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where ''N''<sub>A</sub> is the [[Avogadro constant]], ''R''<sub>∞</sub> is the [[Rydberg constant]], ''A''<sub>r</sub>(e) is the "[[relative atomic mass]]" of the [[electron]], ''M''<sub>u</sub> is the [[molar mass constant]] (1 g/mol by definition) and ''α'' is the [[fine structure constant]]. |
where ''N''<sub>A</sub> is the [[Avogadro constant]], ''R''<sub>∞</sub> is the [[Rydberg constant]], ''A''<sub>r</sub>(e) is the "[[relative atomic mass]]" of the [[electron]], ''M''<sub>u</sub> is the [[molar mass constant]] (1 g/mol by definition) and ''α'' is the [[fine structure constant]]. |
Revision as of 00:10, 26 March 2009
The Stefan–Boltzmann constant (also Stefan's constant), a physical constant denoted by the Greek letter σ, is the constant of proportionality in the Stefan–Boltzmann law: the total energy radiated per unit surface area of a black body in unit time is proportional to the fourth power of the thermodynamic temperature.
The value of the Stefan–Boltzmann constant is given by[1]
- .
The value of the Stefan–Boltzmann constant is derivable as well as experimentally determinable; see Stefan–Boltzmann law for details. It can be defined in terms of the Boltzmann constant kB as:
where kB is the Boltzmann constant, h is the Planck constant, ħ is the reduced Planck constant, and c0 is the speed of light in a vacuum. The CODATA recommended value is calculated from the measured value of the gas constant R:
where NA is the Avogadro constant, R∞ is the Rydberg constant, Ar(e) is the "relative atomic mass" of the electron, Mu is the molar mass constant (1 g/mol by definition) and α is the fine structure constant.
A related constant is the radiation constant a which is given by:[2]
- .
References
- ^ Template:CODATA2006
- ^ Radiation constant from ScienceWorld