Fermi Energy Calculator

Calculate the Fermi energy of a metal from its electron number density.
Shows Fermi energy in eV and Fermi temperature.
Includes presets for common metals.

Only used when Custom is picked above. Enter 8.49 for copper, not 8.49e28.
Fermi Energy

The Fermi energy is the highest occupied electron energy level in a metal at absolute zero temperature:

E_F = (ħ²/2m_e)(3π²n)^(2/3)

Fermi temperature: T_F = E_F / k_B

Where:

  • E_F = Fermi energy (joules)
  • ħ = Reduced Planck constant = 1.0546 × 10⁻³⁴ J·s
  • m_e = Electron mass = 9.109 × 10⁻³¹ kg
  • n = Free electron number density (electrons/m³)
  • k_B = Boltzmann constant = 1.381 × 10⁻²³ J/K

Fermi energy of common metals:

Metal n (×10²⁸ /m³) E_F (eV) T_F (K)
Lithium 4.70 4.75 55,100
Sodium 2.65 3.24 37,600
Aluminum 18.10 11.67 135,400
Copper 8.49 7.05 81,700
Gold 5.90 5.53 64,100
Silver 5.86 5.50 63,800

Those figures come from the formula above, using the electron densities in the second column, so the calculator reproduces every row exactly. Textbook tables will differ by a percent or two, because they start from slightly different measured densities and quote slightly different values of the constants. If a table you are checking against says 4.74 eV for lithium where this one says 4.75, that gap is the density, not an error.

Why Fermi energy matters:

The Fermi energy is critical for understanding:

  • Electrical conductivity: Only electrons near E_F can be excited into higher states by an applied voltage. Metals conduct because E_F lies in the middle of an energy band.
  • Thermoelectric effects: The Seebeck coefficient depends on the density of states near E_F
  • X-ray emission: When electrons fall back to fill inner shell vacancies, they emit X-rays with energies related to E_F
  • White dwarf stars: The Fermi energy of degenerate electrons supports the star against gravitational collapse

Worked example: copper

Copper contributes one free electron per atom, giving n = 8.49 × 10²⁸ per cubic meter.

(ħ²/2mₑ) = (1.0546 × 10⁻³⁴)² / (2 × 9.109 × 10⁻³¹) = 6.105 × 10⁻³⁹
(3π²n)^(2/3) = (29.609 × 8.49 × 10²⁸)^(2/3) = 1.849 × 10²⁰
E_F = 6.105 × 10⁻³⁹ × 1.849 × 10²⁰ = 1.129 × 10⁻¹⁸ J = 7.05 eV
T_F = E_F / k_B = 81,700 K

Pick Copper from the dropdown, or type 8.49 into the custom box, and you get that back.

Why the Fermi temperature is so absurd

T_F for copper is 81,700 K. The metal melts at 1,358 K and boils at 2,835 K. There is no temperature at which solid copper is anything but deeply degenerate, and that is the point: room temperature is well under half a percent of T_F, so to a very good approximation the electrons in every metal you have ever touched are sitting in their ground-state configuration.

That is also why the electronic heat capacity of a metal is so small. Only the sliver of electrons within roughly k_B T of E_F can absorb energy at all, which is a fraction of about T/T_F, and 293/81,700 is 0.36%. Classical physics predicted metals should have far more heat capacity than they do, and this is the resolution.

The Bose-Einstein distribution is the other half of the story: swap the +1 in the Fermi-Dirac denominator for a -1 and you get particles that pile into one state instead of stacking up to E_F.


How we build and check this calculator

This calculator runs entirely in your browser, so the numbers you enter stay on your device. The math behind it is written by hand and tested against worked examples and standard references before the page goes live.

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