The T^4 term in the Stefan-Boltzmann law comes from integrating photon energy density over a Planck distribution.
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Reference literature establishes that the Stefan-Boltzmann law is obtained by integrating Planck's radiation law (representing the photon energy distribution) over all frequencies.
The generalized uncertainty principle (GUP) modifies the uncertainty relation between momentum and position giving room for a minimal length, as predicted by candidates theories of quantum gravity. Inspired by GUP, Planck’s distribution is derived by considering a new quantization of the electromagnetic field. We elaborate on the thermodynamics of the black body radiation obtaining Wien’s law and the Stefan–Boltzmann law. We show that such thermodynamics laws are modified at Planck-scale.
the energy will be redistributed until the ensemble of photons achieves a Planck distribution. The time taken for thermalization is much faster with condensed
A black body or blackbody is an idealized physical body that absorbs all incident electromagnetic radiation, regardless of frequency or angle of incidence. The radiation emitted by a black body in thermal equilibrium with its environment is called black-body radiation. The name "black body" is given because it absorbs all colors of light. In contrast, a white body is one with a "rough surface that
The integration of Planck's law over all frequencies provides the total energy per unit of time per unit of surface area radiated by a black body maintained at a temperature T, and is known as the Stefan–Boltzmann law:
Boltzmann built on two known properties of cavity radiation. (1) The energy density, $u$, defined as $u = U/V$, depends only on temperature, $T$. (2) The radiation pressure, $p$ is given by $p= u/3$. Radiation pressure was given a firm basis c1862 by Maxwell. The factor of 1/3 arises because of the three-dimensionality of the cavity, in which radiation is propagating in all possible directions. [It's easy for us now to derive this equation by considering the cavity as containing a photon gas.] Boltzmann (1884) used a thought-experiment in which a cavity is fitted with a piston, and we take the radiation inside it through a Carnot cycle. On a $p–V$ diagram the isothermals are just horizontal lines, because $u$ is constant so $p$ is constant. The heat input along the top (temperature $T$) isothermal is $\Delta U + p \Delta V$. This works out to be $4 p \Delta V$. If the lower temperature i
"... Das Lebenswerk Boltzmanns war die Neuaufstellung der Thermodynamik. Dabei begründete er mit James Clerk Maxwell die Statistische Mechanik (Boltzmann-Statistik) und deutete die Entropie als eine mikroskopische Größe (siehe unten). Boltzmann war ein Verfechter der atomistischen Vorstellung. Er hatte dabei zahlreiche Fachgenossen seiner Zeit als Gegner, unter ihnen Wilhelm Ostwald und Max Planck. Dieser griff jedoch bei seinem Planckschen Strahlungsgesetz auf die Vorstellungen Boltzmanns zurück. Das Stefan-Boltzmann-Gesetz (die ausgestrahlte Leistung ist der 4. Potenz der absoluten Temperatu
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