MadSci Network: Physics |
The formation of a blackbody spectrum isn't a process like free-free emission (bremsstrahlung) or spontaneous emission. The photons don't come directly from the movement of an electron. Instead, the source of photons depends entirely on what object is giving rise to the blackbody spectrum. If the object in question is a star, then the photons come from nuclear fusion. If it's the canonical blackbody they always talk about in physics books (a heated cavity with a rough inner surface and one small hole to let light out) then the photons come from the thermally excited walls of the chamber. What actually forms the blackbody spectrum is the fact that the photons bounce around zillions of times before escaping. Each time the photon bounces it's re-emitted with a different amount of energy. The result of all this bouncing is the statistical distribution that bears Bolztmann's name. So it doesn't matter where the photons come from. As long as the object that's producing them is optically thick (meaning it allows for a large number of collisions before the photon is released) and in thermal equilibrium then the energy distribution of the resultant light will be a blackbody curve. Reference: Rybicki, G.B., and Lightman, A.P. "Radiative Processes In Astrophysics" Wiley Interscience, 1979.
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