Chemical equilibrium imposes . For blackbody photons, . Define the positive Hydrogen binding energy by , approximately . Multiplying the two Maxwell-Boltzmann distribution number densities and dividing by the neutral-hydrogen density gives
Use and to obtain the Saha ionization equation
The assumptions are nonrelativistic, dilute, nondegenerate species at a common temperature, ground-state hydrogen with the stated degeneracy factors, negligible mass correction in the prefactor, and sufficiently rapid reactions to maintain chemical equilibrium.

Articles by others on the same topic (0)

There are currently no matching articles.