Scientific Unit Matrix
Select a domain and enter a value. The matrix instantly computes all corresponding unit equivalents using strict scientific constants. Supports standard and exponential notation (e.g., 1.5e-3).
Conversion logic
All calculations run locally in your browser. Factors are the 2018 CODATA recommended values and exact SI (2019) definitions; hover any unit's for its definition and source, or see the full method & references below.
How the factors are defined, and where they come from
Every conversion in this tool reduces to a single reference constant per category. The numbers are not rounded conveniences, they are the 2018 CODATA recommended values and the exact SI (2019) definitions. Pick a domain below for the exact relations and the primary source of each constant.
Energy: the Hartree as the anchor
All energy units are expressed relative to the Hartree, Eh, the atomic unit of energy. Its SI value is fixed by the Rydberg constant through Eh = 2R∞hc.
The defining chain:
1 Eh ≡ 2625.4996 kJ/mol = 627.5095 kcal/mol = 219474.63 cm-1
Molar units (kcal/mol, kJ/mol) multiply the per-particle energy by the Avogadro constant NA = 6.022 140 76×1023 mol-1, which is exact since the 2019 SI redefinition. The thermochemical calorie (1 cal = 4.184 J, exact by definition) links kcal/mol to kJ/mol, this is the calorie used by AMBER and CHARMM, not the 15°C or IT calorie. The wavenumber relation E = hcν̃ makes cm-1 an energy unit in spectroscopy.
| Unit | 1 Eh equals | Basis |
|---|---|---|
| eV | 27.211386246 | CODATA 2018 (exact eV since 2019) |
| kJ/mol | 2625.499639 | CODATA 2018 × NA |
| kcal/mol | 627.509474 | + thermochemical calorie (4.184 J) |
| cm-1 | 219474.6314 | CODATA 2018 hartree–inverse-metre |
| K (E/kB) | 315775.02 | CODATA 2018 hartree–kelvin |
Atomic units: length, force, dipole, charge, polarizability
Quantum-chemistry codes (Gaussian, ORCA, Psi4, Quantum ESPRESSO) work internally in atomic units, where ℏ = me = e = 1 and 4πε0 = 1. Converting their output to lab units needs the CODATA values below.
The atomic units used here:
e a0 (dipole) = 8.478 353 6255 × 10-30 C·m = 2.541746 D
e (charge) = 1.602 176 634 × 10-19 C (exact)
Eh/a0 (force) = 8.238 723 4983 × 10-8 N
Eh/a03 (pressure) = 2.942 101 5697 × 1013 Pa
e2a02/Eh (polariz.) = 1.648 777 274 36 × 10-41 C2m2J-1
The debye is fixed exactly by 1 D = 10-21/c C·m = 3.335 641×10-30 C·m (c is exact), giving 1 e·a0 = 2.541746 D. Force-field partial charges are always in units of e, so the charge tab lets you cross-check RESP/CHELPG output against C or statC. Volume polarizability (Å3, the number usually tabulated) follows the Gaussian-CGS convention α[Å3] = α[a.u.] × 0.148185.
Spectroscopy: one photon, four ways to write it
Wavenumber, frequency, photon energy and wavelength all describe the same excitation. Three of them scale linearly; wavelength is the reciprocal.
The relations (h and c are exact SI constants):
1 cm-1 ≡ 29.9792458 GHz ≡ 0.1239842 meV ≡ 1/λ[cm]
Because wavelength is inversely proportional to the others, the matrix inverts correctly only when you type into a single field, the tool normalises to a base wavenumber and reciprocates for λ. Constants used: c = 299 792 458 m/s and h = 6.626 070 15×10-34 J·s, both exact since 2019. The cm-1↔eV factor, 1.239842×10-4, is the reciprocal of 8065.54 cm-1/eV.
Temperature, kBT, and molar entropy
Temperature conversions include the two offset scales (Celsius, Fahrenheit) and the thermal-energy equivalents kBT that appear constantly in statistical mechanics and free-energy work.
Offset scales are affine, not multiplicative:
kBT at 300 K = 2.4943 kJ/mol = 0.5961 kcal/mol = 25.85 meV
The tool converts temperature through kelvin with explicit affine maps, so °C and °F are handled correctly (a plain ratio would be wrong). The kBT rows use kB = 1.380 649×10-23 J/K (exact) and, for molar values, the gas constant R = NAkB = 8.314 462 618 J mol-1 K-1. In the Heat Capacity tab, the entropy unit (e.u., “gibbs”) is 1 cal mol-1 K-1, and quantities are also given as dimensionless multiples of R (or kB per particle).
References & data sources
- Tiesinga, E., Mohr, P. J., Newell, D. B., & Taylor, B. N. (2021). CODATA recommended values of the fundamental physical constants: 2018. Rev. Mod. Phys. 93, 025010. doi:10.1103/RevModPhys.93.025010.
- NIST. Fundamental Physical Constants (2018 CODATA adjustment), Hartree energy, Bohr radius, atomic units of time, force, pressure, electric dipole moment and polarizability, elementary charge. physics.nist.gov/cuu/Constants.
- NIST. Non-SI units accepted for use with the SI, and units based on fundamental constants (2018 CODATA). nonsi_2018.pdf (a.u. of electric dipole moment = 8.4783536255×10-30 C·m; a.u. of polarizability = 1.64877727436×10-41 C2m2J-1).
- BIPM. The International System of Units (SI Brochure), 9th edition (2019). Exact defined values of c, h, e, kB and NA. bipm.org/en/publications/si-brochure.
- Thompson, A., & Taylor, B. N. (2008). Guide for the Use of the International System of Units (SI), NIST Special Publication 811. Definitions of the atmosphere, torr, psi, calorie and other non-SI units. nist.gov/pml/special-publication-811.
- Abraham, M. J., et al. (2015). GROMACS: High performance molecular simulations through multi-level parallelism from laptops to supercomputers. SoftwareX 1–2, 19–25. See also the GROMACS Reference Manual, Definitions and Units. manual.gromacs.org.
- Case, D. A., et al. AMBER Reference Manual (unit system: kcal·mol-1, Å, thermochemical calorie). ambermd.org.
- Debye unit definition: 1 D = 10-18 statC·cm = (10-21/c) C·m ≈ 3.335641×10-30 C·m. See NIST Molecular Spectroscopy special-units notes. physics.nist.gov.
Conversion factors are the 2018 CODATA / exact SI (2019) values. All computation runs entirely in your browser, nothing you type leaves your device.
Frequently asked questions
Which calorie does the kcal/mol use?
Why is the Hartree the base unit for energy?
Why does the wavelength field behave differently in Spectroscopy?
Why can't temperature use a single multiplication factor?
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Is a.u. of polarizability the same as the Å3 I see in tables?
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