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Physics IV course sequence · Interactive lesson

The free-electron Fermi gas

Sommerfeld's answer to why a metal stuffed with mobile electrons still obeys Dulong-Petit. Count the states, fill them by Fermi-Dirac rather than Boltzmann, and the electronic heat capacity collapses to a linear term you can only see below a few kelvin. Learn what that buys — and what deleting the lattice costs.

UPIV-12.05 · Lesson 5 of 9 in this unit. Position is not a completion score.
Starting model: The free-electron Fermi gasTwo panels on one electron-energy axis. Above, the Fermi-Dirac occupancy f(E): a step at E_F = 7.0 eV smeared over a few k_B T. Below, the dashed square-root density of states g(E) and the solid occupied product g(E)f(E). At T = 300 K the ratio kT/E_F is 0.0037, and C_el is 0.0121 of the classical (3/2)Nk_B.T = 300 K · EF = 7.0 eVf(E) = 1 / (exp((E − EF)/kT) + 1)10EFdashed: g(E) ∝ √Esolid: g(E)⋅f(E)0510 eV
Start with a picture. Change the model in the lab below.
1

Build the model

Fill the levels by exclusion, and most of the electrons stop responding to heat.

The key idea

The free-electron Fermi gas is a model of a metal's valence electrons as non-interacting plane waves in a box, filling the lowest states two at a time up to the Fermi energy, with the lattice potential ignored entirely.

Example. Copper donates one electron per atom, n = 8.47 × 10²⁸ m⁻³, so EF = (ℏ²/2m)(3π²n)²⁄³ = 7.0 eV and TF = EF/kB = 8.2 × 10⁴ K — still degenerate at the melting point.

The complete physical model and assumptions

Drude had the right picture and the wrong statistics: a metal's valence electrons do roam free, but they are identical fermions, and at metallic densities Fermi-Dirac occupancy looks nothing like Maxwell-Boltzmann. Sommerfeld keeps the box and throws out the classical counting. Solve the free-particle Schrödinger equation in a cube with periodic boundaries and the allowed wavevectors form a grid in k-space, one state per (2π)³/V of volume; exclusion then makes filling the levels an exercise in geometry. At T = 0 the electrons occupy a sphere of radius kF = (3π²n)¹⁄³ whose surface sits at EF = (ℏ²/2m)(3π²n)²⁄³ — several electronvolts in any real metal, which is tens of thousands of kelvin in temperature units. Everything the model explains follows from that one number dwarfing kB T. Only electrons within a few kB T of the Fermi surface have empty states to move into, so heating a metal stirs a fraction of order T/TF of them rather than all of them, and the electronic heat capacity comes out linear in T and about a hundred times smaller than equipartition demands. The cost is the lattice. With the periodic potential deleted, g(E) ∝ √E is finite at every positive energy, so this model can never open a gap, and every insulator and semiconductor falls outside it.

1Count states in k-space, then fill the sphere

Sommerfeld keeps Drude's box and replaces his statistics. Solve the free-particle Schrödinger equation in a cube of side L with periodic boundaries: the allowed wavevectors form a grid with one state per (2π/L)³ of k-space, a volume (2π)³/V that depends on the sample's size and not its shape. Each state holds two electrons, spin up and spin down. At T = 0 exclusion forces you to fill outward from the origin, so the occupied region is a sphere. Setting N = 2 × (4πkF³/3) ÷ ((2π)³/V) gives N = V kF³/3π², that is kF = (3π²n)¹⁄³ with n = N/V. Copper's one free electron per atom gives n = 8.47 × 10²⁸ m⁻³, so kF = 1.36 × 10¹⁰ m⁻¹ and EF = ℏ²kF²/2m = 7.0 eV. Notice what EF does not depend on: not the chemistry of the metal, not the size of the crystal, not the temperature. Density alone.

2The density of states goes as √E, and never vanishes

Count states below an energy instead. A sphere of radius k = √(2mE)/ℏ holds N(E) = V k³/3π² = (V/3π²)(2mE/ℏ²)³⁄², so g(E) = dN/dE = (V/2π²)(2m/ℏ²)³⁄² √E. That square root is the three-dimensional signature: in two dimensions g is constant, and in one it diverges as E(−1/2). Eliminating the constants in favour of N and EF gives a tidier form, g(E) = (3N/2EF)√(E/EF), so g(EF) = 3N/2EF — about 0.21 states per electronvolt per electron in copper. Now the structural point. √E is nonzero for every energy above the band bottom, so wherever you put the Fermi level there are empty states immediately above it. This model cannot produce a forbidden band, which means it describes metals and nothing else; silicon, diamond and every insulator lie outside it. Opening a gap needs the periodic lattice potential Sommerfeld deleted, which is the business of Bloch's theorem in the next topic.

3Fermi-Dirac occupancy and the width of the blur

The occupancy of a state of energy E is f(E) = 1/[exp((E − μ)/kB T) + 1], with the chemical potential μ tending to EF as T tends to zero. At absolute zero it is a step: every state below EF full, every state above it empty. Warm the metal and the step feathers, but only over a few kB T — f = 0.73 at μ − kB T, exactly 0.5 at μ, 0.27 at μ + kB T, and 0.12 at μ + 2kB T, while μ itself sits below EF by a fraction (π²/12)(T/TF)², about 10⁻⁵ for copper at 300 K. Put numbers on it. At 300 K, kB T = 0.0259 eV; against copper's EF = 7.03 eV that is a feather 0.37% of the height of the cliff. Equivalently TF = EF/kB = 8.2 × 10⁴ K, so across the whole range in which copper is a solid, T/TF stays under 2%. That is what degenerate means: Fermi-Dirac and Maxwell-Boltzmann bear no resemblance to each other here, and the classical limit would need temperatures no metal survives.

4Why heating a metal barely touches its electrons

The argument is one line long. An electron well below EF cannot absorb kB T of energy, because every state kB T above it is already occupied — Pauli blocking, not any shortage of energy. Only those within a few kB T of the Fermi surface have somewhere to go, and they are a fraction of order T/TF of the whole. Each gains about kB T, so the thermal energy is U ≈ N kB T²/TF and Cₑₗ = dU/dT is proportional to T. The Sommerfeld expansion supplies the coefficient: Cₑₗ = (π²/3)kB²T g(EF) = (π²/2)N kB (T/TF). Take two things from that. The heat capacity is linear in T, not constant, so it is a different function altogether from the classical (3/2)NkB. And it is small: the ratio is (π²/3)(T/TF), which for copper at 300 K is 1.2%. That is why Dulong-Petit's 3R survived the discovery that every copper atom donates a mobile electron — those electrons contribute 0.15 J mol⁻¹ K⁻¹ against the lattice's 24.9.

5Measuring γ from a plot of C/T against T²

Far below the Debye temperature, T ≪ θD, the lattice contributes Cₗₐₜ = (12π⁴/5)R(T/θD)³, so a measured molar heat capacity is C = γT + AT³. Divide through by T: C/T = γ + AT². Plot C/T against T² and you get a straight line whose intercept is the electronic coefficient γ and whose slope A gives θD. The two terms are equal where γT = AT³, that is at T = √(γ/A), which for sodium is 1.5 K — so the linear law is a liquid-helium measurement, never a room-temperature one. What comes back is close to, but not equal to, the free-electron prediction. Copper: 0.50 mJ mol⁻¹ K⁻² predicted against 0.695 measured. Potassium: 1.67 against 2.08. The usual bookkeeping is a thermal effective mass, m*/m = γ/γfree, giving 1.38 and 1.25. That ratio is the receipt for what the model discarded — the lattice potential, and the interaction between the electrons themselves.

6What degeneracy holds up, and where the model stops

The filled sphere carries real energy and real pressure. Averaging E over it gives U/N = (3/5)EF, which is 4.2 eV per electron in copper at absolute zero, and the degeneracy pressure P = (2/5)nEF is 38 GPa, with a bulk modulus B = (2/3)nEF of 64 GPa against copper's measured 137 GPa. A factor of two, from a model with no lattice and no Coulomb interaction, is a real success. So is Wiedemann-Franz: the same Fermi-surface electrons carry charge and heat, so κ/σT = (π²/3)(kB/e)² = 2.44 × 10⁻⁸ W Ω K⁻², a constant most metals obey near room temperature. The failures are all one failure. There is no gap, so the model predicts every solid is a metal and cannot say why diamond insulates. Aluminium and beryllium show positive Hall coefficients, as though their carriers were positive. And fitting copper's conductivity demands a mean free path of 39 nm, some 150 atomic spacings, which is absurd for a particle bouncing off a dense array of ions. Each of those needs the periodic potential back.

2

Key equations

Read the units, assumptions and limits before substituting.

Fermi wavevector

kF = (3π² n)¹⁄³, with n = N/V

One number — the free electrons per cubic metre — fixes the radius of the filled sphere in k-space.

n in m⁻³, kF in m⁻¹; the factor 2 for spin is already inside the 3π²

Fermi energy and Fermi temperature

EF = ℏ²kF²/2m = (ℏ²/2m)(3π² n)²⁄³, TF = EF/kB

Sets every other scale in the model, and depends on density alone — not on temperature, chemistry or sample size.

Cu: n = 8.47 × 10²⁸ m⁻³ gives EF = 7.0 eV and TF = 8.2 × 10⁴ K

Density of states in three dimensions

g(E) = (V/2π²)(2m/ℏ²)³⁄² √E = (3N/2EF) √(E/EF)

√E is nonzero at every positive energy, so this model has no forbidden band and can describe metals only.

states per joule; g(EF) = 3N/2EF, about 0.21 eV⁻¹ per electron in copper

Fermi-Dirac occupancy

f(E) = 1/[exp((E − μ)/kB T) + 1], with μ → EF as T → 0

The zero-temperature step feathers over a few kB T — 0.026 eV at 300 K against a 7 eV cliff.

f(μ) = 0.5 exactly, with μ ≈ EF in a metal; f = 0.27 at μ + kB T and 0.12 at μ + 2kB T

Electronic heat capacity

Cₑₗ = (π²/3) kB² T g(EF) = (π²/2) N kB (T/TF) = γT

Linear in T, and (π²/3)(T/TF) = 1.2% of the classical (3/2)NkB for copper at 300 K.

Cu free-electron γ = 0.50 mJ mol⁻¹ K⁻², measured 0.695 mJ mol⁻¹ K⁻²

Ground-state energy and degeneracy pressure

U/N = (3/5)EF, P = (2/5) n EF, B = (5/3)P = (2/3) n EF

Exclusion alone, with no lattice and no Coulomb term, gets a metal's stiffness within a factor of two.

Cu at T = 0: 4.2 eV per electron, P = 38 GPa, B = 64 GPa against 137 GPa measured
3

Interactive lab

Predict first. Explore the model. Compare the result.

Explore the model

300 K
0 to 5000 K; steps of 50.
7.00 eV
3 to 9 eV; steps of 0.25.

Try this. Leave T at 300 K: the step edge is razor sharp, and that alone is why Cₑₗ sits near 1% of the classical value. You must drag T to thousands of kelvin before the blur is even visible. Then reset T and pull EF down to 3 eV — same temperature, more than twice the response.

Live results

FERMI TEMPERATURE TF
81228 K
ELECTRON DENSITY n
8.41 ×10²⁸ m⁻³
kT / EF
0.0037
Cₑₗ ÷ (3/2)NkB
0.0121

Results follow this lesson’s model and assumptions. Displayed values are rounded.

Interactive Physics IV modelTwo panels on one electron-energy axis. Above, the Fermi-Dirac occupancy f(E): a step at E_F = 7.0 eV smeared over a few k_B T. Below, the dashed square-root density of states g(E) and the solid occupied product g(E)f(E). At T = 300 K the ratio kT/E_F is 0.0037, and C_el is 0.0121 of the classical (3/2)Nk_B.T = 300 K · EF = 7.0 eVf(E) = 1 / (exp((E − EF)/kT) + 1)10EFdashed: g(E) ∝ √Esolid: g(E)⋅f(E)0510 eV
Two panels on one electron-energy axis. Above, the Fermi-Dirac occupancy f(E): a step at EF = 7.0 eV smeared over a few kB T. Below, the dashed square-root density of states g(E) and the solid occupied product g(E)f(E). At T = 300 K the ratio kT/EF is 0.0037, and Cₑₗ is 0.0121 of the classical (3/2)NkB.

Predict → change one variable → check

Plan a change before running it. Every other input stays at the saved baseline.

Saved baseline. Temperature T: 300 K; Fermi energy EF: 7.00 eV

Baseline 300; choose 0 to 5000, in steps of 50.
4. Compared with the saved baseline, this result will…

This experiment is kept only while this page is open. It does not change saved course progress.

4

Catch the common trap

Reading "only a kB T-wide slice is active" as "the electrons are sluggish, or nearly frozen". They are neither. At absolute zero copper's electrons average (3/5)EF = 4.2 eV each, more than a hundred times the 0.039 eV that equipartition would hand them at 300 K; the ones at the Fermi surface travel at 1.6 × 10⁶ m s⁻¹; and the gas pushes outward at 38 GPa while the metal sits still. What is small is not the energy but the accessibility. An electron 1 eV below EF cannot absorb a 0.026 eV phonon, because every state 0.026 eV above it is already occupied. Pauli blocking, not lethargy, is what makes Cₑₗ small. For the same reason TF is not a temperature the metal is at — it is the temperature at which the gas would stop being degenerate, and no solid metal comes near it.

5

Practice & worked examples

3 authored examples. Make an attempt, then reveal the reasoning one step at a time.

EasyExample 1

Sodium is monovalent, with a conduction-electron density n = 2.65 × 10²⁸ m⁻³. Find its Fermi wavevector, its Fermi energy in electronvolts, and its Fermi temperature. Take ℏ = 1.055 × 10⁻³⁴ J s, m = 9.11 × 10⁻³¹ kg, kB = 1.381 × 10⁻²³ J K⁻¹ and 1 eV = 1.602 × 10⁻¹⁹ J.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 4 steps revealed.

MediumExample 2

Using TF = 3.76 × 10⁴ K for sodium, find the molar electronic heat capacity at 300 K and compare it with the Dulong-Petit lattice value 3R. Then, given a Debye temperature θD = 158 K and a lattice term Cₗₐₜ = (12π⁴/5)R(T/θD)³, find the temperature below which the electrons dominate. Take R = 8.314 J mol⁻¹ K⁻¹.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 4 steps revealed.

HardExample 3

Low-temperature heat-capacity data for potassium fit C = γT + AT³. Two points on the C/T against T² line are (T = 1.00 K, C/T = 4.66 mJ mol⁻¹ K⁻²) and (T = 1.50 K, C/T = 7.88 mJ mol⁻¹ K⁻²). Extract γ and A, get the Debye temperature from A, and compare γ with the free-electron prediction, given n = 1.40 × 10²⁸ m⁻³ and hence TF = 2.46 × 10⁴ K.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 5 steps revealed.

6

Quick check

Select an answer and explain it before checking.

Copper's conduction electrons have EF = 7.03 eV, so TF = 8.2 × 10⁴ K. At 300 K, which statement correctly describes their contribution to the molar heat capacity?
7

Review & continue

The free-electron Fermi gas is a model of a metal's valence electrons as non-interacting plane waves in a box, filling the lowest states two at a time up to the Fermi energy, with the lattice potential ignored entirely.

  • Explain the relationship without looking at the equation.
  • Check a sign, a unit and a model assumption in your working.
  • Return to the lab or worked example if a step is still unclear.

Extra challenging questions

Connect several ideas, explore supplied data, and compare your reasoning with a worked solution.