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Instrument MI-03-119 · Physics

Debye Length Calculator

Distance at which a plasma, electrolyte, or doped semiconductor stops noticing a stray field: one carrier density, one temperature, one square root.

Instrument MI-03-119
Sheet 1 OF 1
Rev A
Verified
Type 03 — Plasma Physics SER. 2026-03119

Debye length

119.5270607444 nm

λ_D = √(ε₀k_BT ⁄ ne²)

The working Every figure verified twice
  1. lam = √(8.8542e-12·1.3806e-23·300 ⁄ (1.0000e+20·1.6022e-19^2)) = 0.0000001195
Worksheet log
  1. No entries yet — change an input to log a scenario.

How this instrument works

Debye length marks how far a single charge's electric field reaches before surrounding mobile carriers rearrange and cancel it. Push one extra electron into a plasma, an electrolyte, or a doped semiconductor, and nearby free carriers drift to neutralize that field within roughly this distance; beyond it, the material reads as electrically neutral again, whatever caused an imbalance at its center.

Formula balances two competing tendencies: electrostatic attraction, which wants carriers to pile up and build shielding, against thermal agitation, which keeps knocking that arrangement apart. That is why temperature multiplies and carrier density divides: hotter carriers resist settling into tight shielding, so screening distance stretches out, while denser carrier supply hands over more material for thinner shielding, shrinking length by reciprocal density's square root.

Result assumes carriers follow classical Boltzmann statistics, holding at modest densities typical of a diffuse plasma or a lightly doped semiconductor. Push density high enough, or temperature low enough, that most low-energy carrier states sit already occupied, and electrons stop obeying that classical picture — the crossover into that degenerate regime is where a Thomas-Fermi screening length takes over, since filled states block free redistribution this formula assumes.

λD=ε0kBTne2\lambda_D = \sqrt{\dfrac{\varepsilon_0 k_B T}{n e^{2}}}
λ_D — Debye length, metres (shown in nm) · ε₀ — vacuum permittivity, 8.8541878176×10⁻¹² F/m · k_B — Boltzmann constant, 1.380649×10⁻²³ J/K · T — absolute temperature, kelvin · n — charge carrier density, m⁻³ · e — elementary charge, 1.602176634×10⁻¹⁹ C.
  • Enter Charge carrier density, in mobile charges per cubic metre — 1×10²⁰ m⁻³ suits a moderately doped semiconductor.
  • Enter Temperature in kelvin; add 273.15 to a Celsius reading first if that is what you have.
  • Read Debye length — it defaults to nanometres, with micrometres and metres available for larger, sparser plasmas.
  • Watch for the density floor: values at or below zero are rejected, since formula divides by carrier density.

Worked example — carriers in a doped semiconductor at 300 K

Take a silicon sample with a carrier density of 1×10²⁰ per cubic metre sitting at room temperature, 300 K — figures typical of a moderately doped wafer. Multiply ε₀ (8.8541878176×10⁻¹² F/m) by k_B (1.380649×10⁻²³ J/K) by T (300 K), divide by n (1×10²⁰ m⁻³) times e squared (1.602176634×10⁻¹⁹ C, squared), then take square root: instrument returns λ_D = 1.19527060744×10⁻⁷ m, which nanometre display rounds to 119.527 nm.

Raise carrier density six orders of magnitude, to 1×10²⁶ m⁻³, near the free-electron density in a metal, with the same inputs otherwise unchanged: return becomes 1.19527060744×10⁻¹⁰ m, or 0.11953 nm. Millionfold jump in density shrinks screening length by square root of one million, exactly one-thousandfold — arithmetic reason metals shield fields at near-atomic range while lightly doped semiconductors need tens of nanometres for the same job.

Questions

What does Debye length mean physically?

A single charge's electric field survives out to this radius before mobile carriers rearrange and cancel it; beyond that radius, screening has erased it and surrounding material reads as electrically neutral — the working definition of quasineutrality used throughout plasma physics.

Why does raising carrier density shrink Debye length?

More carriers means more material available to build a shield, so a thinner one suffices. Taking density from 1×10²⁰ m⁻³ to 1×10²⁶ m⁻³ at the same 300 K drops length from 119.527 nm to 0.11953 nm — the square root in the formula turns a millionfold density increase into exactly a thousandfold shrink.

Why does raising temperature increase Debye length?

Thermal motion works against shielding — hot carriers keep drifting out of a tight arrangement that would otherwise cancel a nearby charge quickly, so screening needs a longer distance to succeed statistically. Doubling temperature from 300 K to 600 K at 1×10²⁰ m⁻³ raises length from 119.527 nm to 169.037 nm, a factor of √2, matching the square root in the formula exactly.

What happens if carrier density is entered as zero or negative?

Instrument rejects it, since the formula divides by carrier density and that operation is undefined at zero. Physically, zero mobile carriers means nothing is left to do any screening, so a stray charge's field would reach outward without limit — an infinite Debye length is exactly what that situation represents.

Who actually uses Debye length in practice?

Semiconductor engineers use it to judge how thin a depletion region or transistor channel can be made before classical device equations stop holding; plasma physicists use it to test whether a charged gas truly behaves as a plasma, by checking that many carriers fit inside a sphere of that radius; electrochemists apply the same formula, with ionic strength standing in for carrier density, to size the diffuse layer at an electrode surface.

Does this formula also apply to electrolytes and electron-ion plasmas?

Shape is identical, but electrolyte chemists usually swap in solution's ionic strength for n, naming the result the Debye-Hückel screening length; a plasma with both electrons and ions instead combines one such length per species in quadrature. This calculator uses the single-carrier form, matching a doped semiconductor or one-species electron gas directly.

References