Electron and phonon contribution dependence on temperature for heat capacity

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SUMMARY

The discussion focuses on the temperature dependence of heat capacity contributions from electrons and phonons in metals. The phonon contribution follows a T^3 dependence derived from the Debye model, while the electron contribution exhibits a linear T dependence based on the Sommerfeld model. At low temperatures, the electron contribution can surpass the phonon contribution due to the high Fermi temperature (typically T_F ≈ 10^4 K), which results in a term T/T_F that diminishes for most temperatures. The heat capacity can be calculated using the Free Electron Model, with improvements suggested by the Nearly Free Electron Model to account for lattice interactions.

PREREQUISITES
  • Understanding of the Debye model for phonons
  • Fermi-Dirac statistics and its application to conduction electrons
  • Knowledge of the Sommerfeld model for electron heat capacity
  • Basic principles of quantum gases and energy band theory
NEXT STEPS
  • Study the Debye model for phonon heat capacity in detail
  • Explore the Free Electron Model and its limitations
  • Investigate the Nearly Free Electron Model and its implications for heat capacity
  • Learn about Fermi temperature and its significance in metals
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Physicists, materials scientists, and engineers interested in thermodynamics, particularly in the context of heat capacity in metallic systems.

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Hi there!
So I'm aware that the phonon contribution is proportional to T^3 and for electrons it is T (this is for metals where the first result comes from the Debye model). I was wondering where the electron contribution is derived from and why it is such a low dependence.
 
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The T comes from the Sommerfeld model. Keep in mind that these are valid at *low* temperatures, so in that situation the electron contribution is larger than the phonon contribution (ie. T > T^3 for small T).
 
The contribution from conduction electrons to the heat capacity can be calculated by considering the conduction electrons as a perfect quantum gas of electrons, which are fermions and thus obey Fermi-Dirac statistics. Calculating the energy of this gas and taking the derivative of the energy wrt temperature you will find that the heat capacity has a T-dependence. (This is the so called Free Electron Model, not entirely correct since electron interactions are ignored. An improvement is the Nearly Free Electron Model which takes lattice interactions into account by modeling the lattice as a periodic potential that the electrons move in, giving rise to for example the energy bands.)

A guess as to why the electronic part is much smaller is that the Fermi temperature is very high in most metals (typically T_F \approx 10^4 K), and in the expression for the heat capacity I think you have a term T/T_F which is vanishingly low for most temperatures. Also, for temperatures not very small, T^3 >> T.
 

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