Fermi Level Calculator

Enter a metal's conduction-electron density (and an optional sample temperature) to get its Fermi energy, Fermi temperature, Fermi velocity, and degeneracy ratio from the free-electron model.

Quick Facts

Fermi energy
E_F = (ħ²/2mₑ)(3π²n)^(2/3)
Highest occupied electron energy at absolute zero in the free-electron model.
Fermi temperature
T_F = E_F / k_B
An effective temperature scale, typically tens of thousands of kelvin for metals.
Fermi velocity
v_F = √(2E_F / mₑ)
Speed of electrons at the Fermi surface; sets electrical and thermal conduction.
Typical metal
Copper: E_F ≈ 7.0 eV, T_F ≈ 8.2×10⁴ K
Since T_F ≫ room temperature, conduction electrons are always highly degenerate.

Your Results

Calculated
Fermi Energy
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E_F = (ħ²/2mₑ)(3π²n)^(2/3), in eV
Fermi Temperature
-
T_F = E_F / k_B, in kelvin
Fermi Velocity
-
v_F = √(2E_F / mₑ), in m/s
Degeneracy Ratio
-
T_F / T — ≫ 1 means a strongly degenerate electron gas

Ready

Enter an electron density and temperature, then press Calculate.

How the Fermi Level Is Calculated

In the free-electron (Sommerfeld) model of a metal, conduction electrons behave as a gas of fermions confined to the material. Because electrons obey the Pauli exclusion principle, no two can occupy the same quantum state, so at absolute zero they stack up from the lowest available momentum state to a maximum energy called the Fermi energy, E_F — the Fermi level measured from the bottom of the conduction band. This calculator computes E_F, the associated Fermi temperature, Fermi velocity, and a degeneracy ratio from the conduction-electron number density n.

Deriving the Fermi energy formula

Filling momentum states two at a time (spin up and spin down) out to a Fermi sphere of radius k_F in momentum space, and matching the enclosed states to the electron density n, gives the Fermi wavevector k_F = (3π²n)^(1/3). The Fermi energy follows from the free-particle dispersion relation E = ħ²k²/2mₑ evaluated at k_F: E_F = (ħ²/2mₑ)(3π²n)^(2/3), where ħ is the reduced Planck constant and mₑ is the electron mass. Copper, with about one free electron per atom and a density of 8.96 g/cm³, has n ≈ 8.5×10²⁸ m⁻³ and E_F ≈ 7.0 eV — a typical value for simple metals.

Fermi temperature, velocity, and degeneracy

Dividing E_F by Boltzmann's constant gives the Fermi temperature, T_F = E_F / k_B, an energy scale expressed in kelvin. For most metals T_F is tens of thousands of kelvin — far above room temperature — so the electron gas is always "degenerate": only the small fraction of electrons within roughly k_B T of E_F can be thermally excited, and Fermi-Dirac statistics (not the classical Maxwell-Boltzmann distribution) govern their behavior. The Fermi velocity, v_F = √(2E_F/mₑ) = ħk_F/mₑ, is the speed of the electrons that sit at the Fermi surface; it sets the scale for electrical conductivity, thermal conductivity, and mean free path in the Drude and Sommerfeld transport models.

Where this model applies

The free-electron formula here describes simple metals with a partially filled conduction band (alkali metals, copper, silver, gold, aluminum). It is less accurate for transition metals, where d-band structure distorts the density of states, and it does not describe semiconductors or insulators: in those materials the Fermi level lies inside a band gap and its position depends on doping concentration and temperature through a different calculation. Always confirm that the electron density you enter reflects the material's actual conduction-electron count (valence electrons per atom × atomic number density), not the total electron count.

Frequently Asked Questions

What is the Fermi level (Fermi energy)?
In the free-electron model of a metal, the Fermi level (or Fermi energy, E_F) is the highest occupied electron energy state at absolute zero. Because electrons are fermions and obey the Pauli exclusion principle, they fill available momentum states from the lowest energy up to E_F rather than all crowding into the ground state.
Why is copper's Fermi energy about 7 eV when room-temperature thermal energy is only about 0.025 eV?
E_F is set by the electron density and quantum statistics, not by temperature. Because k_B T (about 0.025 eV at 300 K) is far smaller than E_F, only the small fraction of electrons within roughly k_B T of the Fermi surface can be thermally excited — this is why metals are called a degenerate electron gas even far above absolute zero.
Does the free-electron formula apply to semiconductors?
No. This calculator uses the free-electron (Sommerfeld) model, which describes metals with a partially filled conduction band. In semiconductors, the Fermi level sits inside the band gap and depends strongly on doping concentration and temperature, governed by Fermi-Dirac statistics applied to the semiconductor's band structure — a different calculation from the one here.
What is the Fermi velocity used for?
The Fermi velocity v_F is the speed of electrons at the Fermi surface, the ones that dominate electrical and thermal conduction. It appears directly in the Drude model of conductivity, in mean-free-path estimates, and in Fermi liquid theory.