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  2. Stefan–Boltzmann law - Wikipedia

    en.wikipedia.org/wiki/StefanBoltzmann_law

    The StefanBoltzmann constant, σ, is derived from other known physical constants: = where k is the Boltzmann constant, the h is the Planck constant, and c is the speed of light in vacuum. [19] [4]: 388

  3. Boltzmann constant - Wikipedia

    en.wikipedia.org/wiki/Boltzmann_constant

    Boltzmann constant: The Boltzmann constant, k, is one of seven fixed constants defining the International System of Units, the SI, with k = 1.380 649 x 10 −23 J K −1. The Boltzmann constant is a proportionality constant between the quantities temperature (with unit kelvin) and energy (with unit joule).

  4. Black-body radiation - Wikipedia

    en.wikipedia.org/wiki/Black-body_radiation

    The law was formulated by Josef Stefan in 1879 and later derived by Ludwig Boltzmann. The formula E = σT 4 is given, where E is the radiant heat emitted from a unit of area per unit time, T is the absolute temperature, and σ = 5.670 367 × 10 −8 W·m −2 ⋅K −4 is the StefanBoltzmann constant. [28]

  5. List of physical constants - Wikipedia

    en.wikipedia.org/wiki/List_of_physical_constants

    These include the Boltzmann constant, which gives the correspondence of the dimension temperature to the dimension of energy per degree of freedom, and the Avogadro constant, which gives the correspondence of the dimension of amount of substance with the dimension of count of entities (the latter formally regarded in the SI as being dimensionless).

  6. Thermal radiation - Wikipedia

    en.wikipedia.org/wiki/Thermal_radiation

    where is the StefanBoltzmann constant and is temperature. [18] A negative value for Q ˙ {\displaystyle {\dot {Q}}} indicates that net radiation heat transfer is from surface 2 to surface 1. For two grey-body surfaces forming an enclosure, the heat transfer rate is:

  7. Mass–luminosity relation - Wikipedia

    en.wikipedia.org/wiki/Mass–luminosity_relation

    Approximating the star by a black body, the energy density is related to the temperature by the StefanBoltzmann law: = where = =. is the StefanBoltzmann constant, c is the speed of light, k B is Boltzmann constant and is the reduced Planck constant. As in the theory of diffusion coefficient in gases, the diffusion coefficient D ...

  8. Stefan–Boltzmann constant - Wikipedia

    en.wikipedia.org/?title=StefanBoltzmann...

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  9. Boltzmann's entropy formula - Wikipedia

    en.wikipedia.org/wiki/Boltzmann's_entropy_formula

    where is the Boltzmann constant (also written as simply ) and equal to 1.380649 × 10 −23 J/K, and is the natural logarithm function (or log base e, as in the image above). In short, the Boltzmann formula shows the relationship between entropy and the number of ways the atoms or molecules of a certain kind of thermodynamic system can be arranged.