Find relative number of H atoms in n=1,2,3,4 energy levels

AI Thread Summary
The discussion revolves around calculating the relative number of hydrogen atoms in the n=1, 2, 3, and 4 energy levels within the chromosphere at a temperature of 5000 K. The initial solution provided uses the Boltzmann distribution formula, yielding a ratio of 1 : 5.4 x 10^-11 : 6.7 x 10^-13 : 1.5 x 10^-13. However, some participants argue that the Boltzmann distribution is not applicable due to the discrete nature of energy levels in hydrogen. A counterpoint is made that the formula can be correctly applied by considering the degeneracies of the energy levels. The conversation highlights the importance of correctly applying statistical mechanics to systems with discrete energy states.
xatu
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The problem:

Find the relative numbers of hydrogen atoms in the chromosphere (T=5000 K) in the n=1, 2, 3, and 4 energy levels.

Solution:

The Boltzmann distribution of energies is

n(ε)dε=\frac{2πN}{(πkT)^{3/2}}\sqrt{ε}e^{-ε/kT}dε

So using this I calculated the ratio to be, 1 : 5.4 x 10^-11 : 6.7 x 10^-13 : 1.5 x 10^-13.

Can anyone confirm this?
 
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xatu said:
The Boltzmann distribution of energies is

n(ε)dε=\frac{2πN}{(πkT)^{3/2}}\sqrt{ε}e^{-ε/kT}dε

This is not applicable to this problem. You are dealing with a system that has discrete energies. See http://en.wikipedia.org/wiki/Boltzmann_distribution
 
Actually I used that formula, accounting for the degeneracies of the energy levels, and got the correct answer.
 
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