Using Maxwell Boltzmann distribution to find number of atoms

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SUMMARY

The discussion focuses on calculating the number of mercury atoms in the first excited state using the Maxwell-Boltzmann distribution. Given that the energy difference between the ground state and the first excited state is 4.86 eV, and with a sample containing 1.06×1020 atoms at 1563 K, the user applies the Maxwell-Boltzmann distribution formula, f(E)=A eE/kbT, to find the normalization constant A, which is determined to be 3.854. The user correctly identifies the statistical weights for the ground state (n=1) and first excited state (n=2) as 2 and 8, respectively, and expresses the total number of atoms as a sum of the distributions for both states.

PREREQUISITES
  • Understanding of the Maxwell-Boltzmann distribution
  • Familiarity with statistical mechanics concepts
  • Knowledge of energy states in quantum mechanics
  • Basic calculus for integration and normalization
NEXT STEPS
  • Study the derivation and application of the Maxwell-Boltzmann distribution in detail
  • Learn about statistical weights and their significance in quantum states
  • Explore the Franck-Hertz experiment and its implications in atomic physics
  • Investigate integration techniques for calculating distributions in statistical mechanics
USEFUL FOR

Students in physics, particularly those studying thermodynamics and quantum mechanics, as well as educators and researchers interested in atomic behavior and statistical distributions.

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Homework Statement



You will recall from our discussion of the Franck-Hertz experiment that the energy difference between the first excited state of mercury and the ground state is 4.86 eV. If a sample of mercury vaporized in a flame contains 1.06×1020 atoms in thermal equilibrium at 1563 K, calculate the number of atoms in the first excited state. Assume that the Maxwell-Boltzmann distribution applies and that the n = 1 (ground) and n = 2 (first excited) states have equal statistical weights.

Homework Equations



The Maxwell-Boltzmann distribution:

f(E)=A e^{\frac{E}{k_{b}T}}

where A is a constant
k_b is the Boltzmann constant = 8.617*10^-5 eV/K
and T is the temperature

n(E)dE = g(E) * f(E) dE

where n(E) = # per unit energy
g(E) = # of states per energy E
f(E) = MB distribution

The Attempt at a Solution



I'm still having trouble learning how to use distributions, so bear with me (or help me understand it :))

I started off by normalizing the distribution by:

\int\limits_0^\infty f(E)^2 dE

then I set it equal to 1 and solved for A. I found A=3.854.

I think that was the right first step.

and I know that g(E) for n=1 is 2 possible states
and n=2 has 8.

This is as far as I have gotten, as my professor hasn't really gone over how to use these distributions.

My guess is that I set

1.06*10^{20} = n_{1}(E) dE + n_{2} (E) dE <br /> <br /> after this I know I have to integrate, but I'm not sure how to set up the limits, among other things.
 
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never mind I figured it out!
 

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