Ludwig Eduard Boltzmann is responsible for a lot of equations
and in various fields, different equations are termed the
In the field of Stellar Structure, an equation giving
the count of atoms at different possible Atomic Excitation
levels is given the name, or sometimes
N - N
^{i+1}, N^{i}- Number Density of two States of Excitation i and i+1. - g
^{i+1}, g^{i}- quantum-mechanical Degeneracy Weights. - k - Boltzmann Constant.
- T - Temperature.
This equation is related to the equation,physics,model)Referenced by:
Degeneracy Weight State of Excitation Temperature |