Heat capacity (statistical physics)

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SUMMARY

The discussion focuses on calculating the heat capacity of a statistical physics system with three energy levels: E_1 = ε, E_2 = 2ε, and E_3 = 3ε, where the degeneracies are g(E1) = 1, g(E2) = 2, and g(E3) = 1. The partition function Q is derived as Q = exp(-B·E1) + 2exp(-B·E2) + exp(-B·E3), where B = kT. The internal energy U is computed using U = -d(lnQ)/dB, resulting in U = E·exp(-B·E1) + 4E·exp(-B·E2) + 3E·exp(-B·E3), illustrating the relationship between energy levels and their probabilities.

PREREQUISITES
  • Understanding of statistical mechanics concepts, particularly the partition function.
  • Familiarity with thermodynamic quantities such as internal energy and heat capacity.
  • Knowledge of Boltzmann factors and their application in statistical physics.
  • Basic calculus for differentiation in the context of thermodynamic equations.
NEXT STEPS
  • Study the derivation and applications of the partition function in statistical mechanics.
  • Learn how to compute heat capacity from internal energy in various systems.
  • Explore the implications of degeneracy in energy levels on thermodynamic properties.
  • Investigate the relationship between temperature and energy distribution in statistical physics.
USEFUL FOR

Students of statistical physics, researchers in thermodynamics, and anyone interested in understanding the foundational concepts of heat capacity and energy distribution in physical systems.

broegger
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Hi. I've just started a course on statistical physics and the first assignment is this:

A system possesses 3 energy levels, E_1 = \epsilon, E_2 = 2\epsilon and E_3 = 3\epsilon. The degeneracy of the levels are g(E1) = g(E3) = 1, g(E2) = 2. Find the heat capacity of the system.

I've forgotten all this thermodynamics stuff, so I would appreciate some hints :-)
 
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Anyone? Please :rolleyes:
 
If you are given a description of a system, what quantity do you first compute, from which you can determine other thermodynamic quantities ?
 
Yes, yes, the partition function, I know :-)
 
sum over states to get Q

Q= exp{-B.E) + 2exp{-B.2E} + exp{-B.3E}

B=kT Q=partition E=energy (two in front of second term beacuse of degenercy)


U= - Diff (lnQ) w.r.t (B)

U= internal energy prof can be found ( http://www.chem.arizona.edu/~salzmanr/480b/statt01/statt01.html)... if you are interested

gives U= E.exp(-B.E) + 4E.exp(-B.2E) + 3E.exp(-B.3E)

makes sense highest energy has least probability of being populated but contributes three times as much to internal energy when it is. same would apply to the middle state but there is two of them so it is four instead of two.
 

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