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## Photon gasIn physics, a A massive ideal gas with only one type of particle is uniquely described by three state functions such as the temperature, volume, and the number of particles. However, for a black body, the energy distribution is established by the interaction of the photons with matter, usually the walls of the container. In this interaction, the number of photons is not conserved. As a result, the chemical potential of the black body photon gas is zero. The number of state functions needed to describe a black body state is thus reduced from three to two (e.g. temperature and volume). ## Additional recommended knowledge
## Thermodynamics of a black body photon gasIn a gas with massive particles, the energy of the particles is distributed according to a Maxwell-Boltzmann distribution. This distribution is established as the particles collide with each other, exchanging energy (and momentum) in the process. In a photon gas, there will also be an equilibrium distribution, but photons do not collide with each other (except under very extreme conditions) so that the equilibrium distribution must be established by other means. The most common way that an equilibrium distribution is established is by the interaction of the photons with matter. If the photons are absorbed and emitted by the walls of the system containing the photon gas, and the walls are at a particular temperature, then the equilibrium distribution for the photons will be a black body distribution at that temperature. A very important difference between a gas of massive particles and a photon gas with a black body distribution is that the number of photons in the system is not conserved. A photon may collide with an electron in the wall, exciting it to a higher energy state, removing a photon from the photon gas. This electron may drop back to its lower level in a series of steps, each one of which releases an individual photon back into the photon gas. Although the sum of the energies of the emitted photons are the same as the absorbed photon, the number of emitted photons will vary. It can be shown that, as a result of this lack of constraint on the number of photons in the system, the chemical potential of the photons must be zero for black body radiation. The thermodynamics of a black body photon gas may be derived using quantum mechanical arguments. The derivation yields the spectral energy distribution where The derivation also yields the (expected) number of photons where ζ() is the Riemann zeta function. Note that for a particular temperature, the particle number varies with the volume in a fixed manner, adjusting itself to have a constant density of photons. The derivation is given in more detail in the "Derivation" section below. The following table summarizes the thermodynamic state functions for a black body photon gas. **Thermodynamic state functions for a black body photon gas**State function (T,V) Internal energy Particle number Chemical potential Pressure Entropy Enthalpy Helmholtz free energy Gibbs free energy
## Isothermal transformationsAs an example of a thermodynamic process involving a photon gas, consider a cylinder with a movable piston. The interior walls of the cylinder are "black" in order that the temperature of the photons can be maintained at a particular temperature. This means that the space inside the cylinder will contain a blackbody-distributed photon gas. Unlike a massive gas, this gas will exist without the photons being introduced from the outside - the walls will provide the photons for the gas. Suppose the piston is pushed all the way into the cylinder so that there is an extremely small volume. The photon gas inside the volume will press against the piston, moving it outward, and in order for the transformation to be isothermic, a counter force of almost the same value will have to be applied to the piston so that the motion of the piston is very slow. This force will be equal to the pressure times the cross sectional area ( x ) travelled yields the total work done to create this photon gas at this volume
where the relationship The pressure is Integrating, the work done is just The amount of heat that must be added in order to create the gas is where ## See also- Photon
- Gas in a box - derivation of distribution functions for all ideal gases
- Planck's law of black body radiation - The distribution of photon energies as a function of frequency or wavelength.
- Stefan-Boltzmann law - The total flux emitted by a black body.
- Radiation pressure
## References- Baierlein, Ralph (April 2001). "The elusive chemical potential".
*American Journal of Physics***69**(4): 423-434. doi:10.1119/1.1336839. - Herrmann, F.; Würfel, P. (August 2005). "Light with nonzero chemical potential" (PDF).
*American Journal of Physics***73**(8): 717-723. doi:10.1119/1.1904623#. - Leff, Harvey S. (August 2002). "Teaching the photon gas in introductory physics" (PDF).
*American Journal of Physics***70**(8): 792-797. doi:10.1119/1.1479743.
Categories: Thermodynamics | Statistical mechanics |
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This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Photon_gas". A list of authors is available in Wikipedia. |