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  2. 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).

  3. Mean free path - Wikipedia

    en.wikipedia.org/wiki/Mean_free_path

    where k B is the Boltzmann constant, is the pressure ... Mean free path for photons in energy range from 1 keV to 20 MeV for elements with Z = 1 to 100. [6]

  4. kT (energy) - Wikipedia

    en.wikipedia.org/wiki/KT_(energy)

    kT (also written as k B T) is the product of the Boltzmann constant, k (or k B), and the temperature, T.This product is used in physics as a scale factor for energy values in molecular-scale systems (sometimes it is used as a unit of energy), as the rates and frequencies of many processes and phenomena depend not on their energy alone, but on the ratio of that energy and kT, that is, on ⁠ E ...

  5. Electronvolt - Wikipedia

    en.wikipedia.org/wiki/Electronvolt

    The electronvolt is divided by the Boltzmann constant to convert to the Kelvin scale: / = = , where k B is the Boltzmann constant. The k B is assumed when using the electronvolt to express temperature, for example, a typical magnetic confinement fusion plasma is 15 keV (kiloelectronvolt), which is equal to 174 MK (megakelvin).

  6. Grand canonical ensemble - Wikipedia

    en.wikipedia.org/wiki/Grand_canonical_ensemble

    The grand canonical ensemble is the only ensemble with constant , V, and T that reproduces the fundamental thermodynamic relation. [5] Statistical equilibrium (steady state): A grand canonical ensemble does not evolve over time, despite the fact that the underlying system is in constant motion. Indeed, the ensemble is only a function of the ...

  7. Neutron moderator - Wikipedia

    en.wikipedia.org/wiki/Neutron_moderator

    where is the neutron mass, is the average squared neutron speed, and is the Boltzmann constant. [2] [3] The characteristic neutron temperature of several-MeV neutrons is several tens of billions kelvin.

  8. Maxwell–Boltzmann statistics - Wikipedia

    en.wikipedia.org/wiki/Maxwell–Boltzmann_statistics

    Boltzmann's fundamental equation = ⁡ relates the thermodynamic entropy S to the number of microstates W, where k is the Boltzmann constant. It was pointed out by Gibbs however, that the above expression for W does not yield an extensive entropy, and is therefore faulty. This problem is known as the Gibbs paradox.

  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.