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  2. Planck units - Wikipedia

    en.wikipedia.org/wiki/Planck_units

    The Planck Units are derived from the left-most vertice of the triangle, where the schwarzchild radius meets the compton wavelength. In particle physics and physical cosmology, Planck units are a system of units of measurement defined exclusively in terms of four universal physical constants: c, G, ħ, and k B (described further

  3. Planck's law - Wikipedia

    en.wikipedia.org/wiki/Planck's_law

    In physics, Planck's law (also Planck radiation law [1]: 1305 ) describes the spectral density of electromagnetic radiation emitted by a black body in thermal equilibrium at a given temperature T, when there is no net flow of matter or energy between the body and its environment.

  4. Einstein coefficients - Wikipedia

    en.wikipedia.org/wiki/Einstein_coefficients

    From Planck's law of black-body radiation at temperature T we have for the spectral radiance (radiance is energy per unit time per unit solid angle per unit projected area, when integrated over an appropriate spectral interval) [26] at frequency ν (,) = /, where [27] =, where is the speed of light and is the Planck constant.

  5. Zero-point energy - Wikipedia

    en.wikipedia.org/wiki/Zero-point_energy

    In 1900, Max Planck derived the average energy ε of a single energy radiator, e.g., a vibrating atomic unit, as a function of absolute temperature: [24] = / (), where h is the Planck constant, ν is the frequency, k is the Boltzmann constant, and T is the absolute temperature. The zero-point energy makes no contribution to Planck's original ...

  6. Planckian locus - Wikipedia

    en.wikipedia.org/wiki/Planckian_locus

    T is the temperature of the black body h is the Planck constant c is the speed of light k is the Boltzmann constant. This will give the Planckian locus in CIE XYZ color space. If these coordinates are X T, Y T, Z T where T is the temperature, then the CIE chromaticity coordinates will be = + +

  7. Rayleigh–Jeans law - Wikipedia

    en.wikipedia.org/wiki/Rayleigh–Jeans_law

    Comparison of Rayleigh–Jeans law with Wien approximation and Planck's law, for a body of 5800 K temperature.. In physics, the Rayleigh–Jeans law is an approximation to the spectral radiance of electromagnetic radiation as a function of wavelength from a black body at a given temperature through classical arguments.

  8. Partition function (statistical mechanics) - Wikipedia

    en.wikipedia.org/wiki/Partition_function...

    It may not be obvious why the partition function, as we have defined it above, is an important quantity. First, consider what goes into it. The partition function is a function of the temperature T and the microstate energies E 1, E 2, E 3, etc. The microstate energies are determined by other thermodynamic variables, such as the number of ...

  9. Natural units - Wikipedia

    en.wikipedia.org/wiki/Natural_units

    Planck considered only the units based on the universal constants G, h, c, and k B to arrive at natural units for length, time, mass, and temperature, but no electromagnetic units. [7] The Planck system of units is now understood to use the reduced Planck constant, ħ, in place of the Planck constant, h. [8]