The Tauc–Davis–Mott relation, the transition selection rules, the regression standard used to extract Eg, and the exact input conventions the calculator expects.
Originally formulated by Jan Tauc (1966) for amorphous semiconductors and generalized by Davis and Mott (1970), the optical absorption near the fundamental absorption edge satisfies:
α is the absorption coefficient,hν is the photon energy in electronvolts,B is an energy-independent transition constant,Eg is the optical band gap, andn encodes the nature of the electronic transition. Plotting (αhν)n againsthν therefore yields a linear onset whose extrapolation to the energy axis gives Eg. A term-by-term walkthrough of this equation, its axes and the intercept calculation lives on theTauc plot equation page.
| Electronic transition | Exponent (n) | Selection rules & mechanism | Canonical materials |
|---|---|---|---|
| Direct allowed | 2 | Δk = 0; vertical electric dipole transition at identical k-vector | ZnO, GaAs, CdTe, MAPbI₃ |
| Indirect allowed | 1/2 (0.5) | Δk ≠ 0; requires simultaneous phonon absorption/emission | Si, Ge, Anatase TiO₂, GaP |
| Direct forbidden | 3/2 (1.5) | Dipole matrix element vanishes at k = 0; higher-order transitions | Cu₂O, SnO |
| Indirect forbidden | 2/3 (~0.67) | Phonon-assisted transition with dipole forbidden matrix element | SnO₂, rare-earth oxides |
In practice the plotted quantity is written asF(R)hν or(αhν)n depending on the unit mode selected in the workspace; the exponent is applied after the unit conversion, never before.
When film thickness is unknown, or when analysing colloidal suspensions and powders, the absorbance A serves as an experimental proxy for α:
Assumes constant optical path length and negligible wavelength-dependent scattering.
Calculated using the Beer–Lambert transmission law through a sample of thickness d:
Assumes normal incidence, negligible specular/diffuse surface reflectance, and non-interfering sample boundaries.
Fitting must occur strictly in the linear onset region of the Tauc curve:
Within the selected window the calculator performs an ordinary least-squares fit ofy = mx + b and reports the coefficient of determination R². The fitted line is extrapolated to y = 0, giving the optical band gap Eg = −b / m.
Plain-text instrument exports with a .txt, .dat or .csv extension. Two columns are required: the horizontal axis and the measured intensity.
Comma, semicolon, tab and whitespace separators are detected automatically, as are header rows, comment lines and blank rows.
Wavelength (nm), photon energy (eV) or wavenumber (cm⁻¹). Wavelength is converted internally with E = hc / λ, using hc = 1239.841984 eV·nm.
Absorbance, transmittance (%) or a pre-computed absorption coefficient. Transmittance is converted with A = −log₁₀(T / 100).
| Output | Description |
|---|---|
| Eg (eV) | Optical band gap from the extrapolated x-intercept |
| m, b | Slope and intercept of the linear fit within the selected window |
| R² | Coefficient of determination for the fit window |
| PNG / SVG | Plot export including curve, fit line, dashed extrapolation and Eg annotation |