Classical Limits:-The classical limit is the ability of a physical theory to approximate or "recover" classical mechanics when considered over special values of its parameters. The classical limit is used with physical theories that predict non-classical behavior.
The function f(e) depends on whether or not the particles obey the Pauli exclusion principle.
We know that for the bosons distribution function "f_{BE}(\\epsilon)=\\dfrac{1}{e^{\\alpha+\\frac{\\epsilon}{kT}}-1}"
For fermions, the distribution function is "f_{FE}(\\epsilon)=\\dfrac{1}{e^{\\alpha+\\frac{\\epsilon}{kT}}+1}"
We know that max well distribution function "f(\\epsilon)=Ae^{\\frac{-\\epsilon}{kT}}"
The number of particles having energy "\\epsilon" at temperature T,
"n(\\epsilon)= Ag(\\epsilon)e^{-\\epsilon\/kT}"
So, for atom in ground state,
"n(\\epsilon_1)= Ag(\\epsilon_1)e^{-\\epsilon_1\/kT}" --------(i)
So, for atom in first excited state,
"n(\\epsilon_2)= Ag(\\epsilon_2)e^{-\\epsilon_21\/kT}" -----(ii)
Now dividing equation (ii) by (i)
"\\dfrac{n(\\epsilon_2)}{n(\\epsilon_1)}=\\dfrac{g(\\epsilon_2)}{g(\\epsilon_1)}e^{-\\frac{\\epsilon_2-\\epsilon_1}{kT}}"
="Ae^{-\\epsilon\/kT}"
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