University Physics IV · Molecular and Solid-State Physics · 12.5
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.
Build the model
Connect the measurement to the mechanism.
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.
- Simple definition
- 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.
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
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
√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
The zero-temperature step feathers over a few kB T — 0.026 eV at 300 K against a 7 eV cliff.
f(EF) = 0.5 exactly; f = 0.27 at EF + kB T and 0.12 at EF + 2kB T
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
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
Count 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.
The 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. Dropping the constants 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.
Fermi-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 EF − kB T, exactly 0.5 at EF, 0.27 at EF + kB T, and 0.12 at EF + 2kB T. 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.
Why 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.
Measuring γ from a plot of C/T against T²
Below the Debye temperature 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.
What 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.
Change one variable at a time
Make the relationship visible.
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.
FERMI TEMPERATURE TF81228 K
ELECTRON DENSITY n8.41 ×10²⁸ m⁻³
kT / EF0.0037
Cₑₗ ÷ (3/2)NkB0.0121
Live interpretationFERMI TEMPERATURE TF: 81228 K. ELECTRON DENSITY n: 8.41 ×10²⁸ m⁻³. kT / EF: 0.0037. Cₑₗ ÷ (3/2)NkB: 0.0121
Catch the common trap
Explain before calculating.
Copper's conduction electrons have EF = 7.0 eV, so TF = 8.2 × 10⁴ K. At 300 K, which statement correctly describes their contribution to the molar heat capacity?
Choose an answer to test the model.
Practice & worked examples
Reason from the model, then test the result.
EasySodium 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.
- The two spin states per k-point are already inside the constant, so kF = (3π²n)¹⁄³. First the bracket: 3π² = 29.61, and 29.61 × 2.65 × 10²⁸ = 7.85 × 10²⁹ m⁻³.
- Cube root: kF = (7.85 × 10²⁹)¹⁄³ = 9.22 × 10⁹ m⁻¹. Sanity check — the Fermi wavelength 2π/kF is 0.68 nm, a couple of atomic spacings, which is the right size for an electron shared across a lattice.
- EF = ℏ²kF²/2m = (1.055 × 10⁻³⁴)² × (9.22 × 10⁹)² ÷ (2 × 9.11 × 10⁻³¹) = 9.46 × 10⁻⁴⁹ ÷ 1.822 × 10⁻³⁰ = 5.19 × 10⁻¹⁹ J.
- Convert, then divide: EF = 5.19 × 10⁻¹⁹ ÷ 1.602 × 10⁻¹⁹ = 3.24 eV, and TF = EF/kB = 5.19 × 10⁻¹⁹ ÷ 1.381 × 10⁻²³ = 3.76 × 10⁴ K.
AnswerkF = 9.22 × 10⁹ m⁻¹, EF = 3.24 eV, TF = 3.76 × 10⁴ K. Sodium melts at 371 K, about one hundredth of TF, so its electron gas is degenerate everywhere the metal exists.
MediumUsing 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.
- Per mole N = NA and N kB = R, so Cₑₗ = (π²/2)R(T/TF) = γT with γ = (π²/2)R/TF = 4.935 × 8.314 ÷ 3.76 × 10⁴ = 41.03 ÷ 37600 = 1.09 × 10⁻³ J mol⁻¹ K⁻².
- At 300 K: Cₑₗ = 1.09 × 10⁻³ × 300 = 0.327 J mol⁻¹ K⁻¹, against 3R = 24.9 J mol⁻¹ K⁻¹. The electrons carry 1.3% of the lattice's share — which is why Dulong-Petit outlived the discovery of the electron.
- The two terms carry different powers of T. The phonon coefficient is A = (12π⁴/5)R/θD³ = 233.8 × 8.314 ÷ 158³ = 1944 ÷ 3.944 × 10⁶ = 4.93 × 10⁻⁴ J mol⁻¹ K⁻⁴.
- They are equal when γT = AT³, so T = √(γ/A) = √(1.09 × 10⁻³ ÷ 4.93 × 10⁻⁴) = √2.21 = 1.49 K.
AnswerCₑₗ(300 K) = 0.33 J mol⁻¹ K⁻¹, about 1.3% of 3R; the electronic term overtakes the phonon term only below 1.5 K, which is why the linear law is a liquid-helium result.
HardLow-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.
- Divide C = γT + AT³ through by T: C/T = γ + AT². Against T² that is a straight line, intercept γ, slope A — the standard way to separate electrons from phonons, because only the electronic term survives as T² tends to zero.
- Slope: A = (7.88 − 4.66) ÷ (1.50² − 1.00²) = 3.22 ÷ 1.25 = 2.58 mJ mol⁻¹ K⁻⁴. Intercept: γ = 4.66 − 2.58 × 1.00 = 2.08 mJ mol⁻¹ K⁻².
- Debye temperature from A = (12π⁴/5)R/θD³: θD³ = 233.8 × 8.314 ÷ 2.58 × 10⁻³ = 7.54 × 10⁵ K³, so θD = 91 K.
- Free-electron prediction: γfree = (π²/2)R/TF = 41.03 ÷ 2.46 × 10⁴ = 1.67 mJ mol⁻¹ K⁻².
- Ratio: m*/m = γ/γfree = 2.08 ÷ 1.67 = 1.25. The heat capacity is linear in T exactly as Sommerfeld says, but the electrons respond as though 25% heavier — the lattice potential and the electron-electron interaction, reappearing as a mass.
Answerγ = 2.08 mJ mol⁻¹ K⁻², A = 2.58 mJ mol⁻¹ K⁻⁴, θD = 91 K, and a thermal effective mass m* = 1.25 m. The model gets the functional form exactly right and the coefficient 25% wrong.