Maxwell Boltzmann distribution

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SUMMARY

The discussion focuses on calculating the number of mercury atoms in the ground state (n=1) and the first excited state (n=2) using the Maxwell-Boltzmann distribution. Given the energy difference of 4.86 eV and a temperature of 1600K, participants clarify that the statistical weights of the states are not equal, despite initial assumptions. The correct approach involves applying the Boltzmann factor to determine the relative populations of the two states, emphasizing the importance of understanding energy differences in statistical mechanics.

PREREQUISITES
  • Understanding of the Maxwell-Boltzmann distribution
  • Knowledge of Boltzmann factors and statistical mechanics
  • Familiarity with energy levels in quantum mechanics
  • Basic thermodynamics concepts, particularly thermal equilibrium
NEXT STEPS
  • Study the derivation and application of the Boltzmann factor in statistical mechanics
  • Explore the implications of energy differences on population distributions in quantum systems
  • Learn about statistical weights and their role in determining state populations
  • Investigate the Maxwell-Boltzmann distribution in different thermodynamic contexts
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Students and professionals in physics, particularly those studying thermodynamics and quantum mechanics, as well as anyone involved in statistical mechanics and atomic population calculations.

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Homework Statement


The energy difference between the first excited state of mercury and the ground state is 4.86 eV.
(a) If a sample of mercury vaporized in a flame contains 10^20
atoms in thermal equilibrium at 1600K, calculate the number of atoms in the n=1 (ground) and n=2 (first-excited) states. (Assume the Maxwell-Boltzmann distribution applies and that the n=1 and n=2 states have equal statistical weights.)

Homework Equations


Maxwell Boltzmann Distribution

The Attempt at a Solution


I thought that since they have the same statistical weight, there must be 5*10^19 particles in each state. But I don't think it is the good answer since we use this number for another exercice and it doesn't yield the good answer.
I don't know how to figure out these number using Maxwell Boltzmann distribution.
 
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Maxwell-Boltzmann refers to the distributions of atom velocities and is not relevant here.

What are relative populations of 2 states, separated by energy ΔE and at a temperature T?
 
"Statistical weight" refers to the number of different states there are with n=1 and n=2, respectively. In reality the statistical weight is certainly not the same for these states, but never mind: all you need is the energy difference between the two states, and then answer Redbelly's question.

[It's a bit unfortunate that *sometimes* by "statistical weight" one means exactly the Boltzmann factor you will have to calculate: so by that definition you are correct to say the populations in the states are equal. But clearly, the person who phrased the question did not have that meaning of "statistical weight" in mind.]
 

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