Wiki · Constants and the Nature Ledger
Dimensionless numbers
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The ratios that carry meaning without units.
23 rows.
| name | symbol | formula | meaning | critical values | source |
|---|---|---|---|---|---|
| Reynolds number | Re | Re = ρuL/μ = uL/ν | ratio of inertial to viscous forces | Pipe transition: Re_c = 2040 ± 10 for the onset of SUSTAINED turbulence (Avila et al. 2011), where mean puff-decay time equals mean puff-splitting time; the textbook ~2300 (range ~2000–4000) answers a different question. Scope: smooth circular pipe only — it does not transfer to a wing or an artery. | Purcell (1977) Am J Phys 45:3–11; Avila et al. (2011) Science 333:192–196 |
| Péclet number | Pe | Pe = uL/D | ratio of advection to diffusion | Pe ≪ 1 → stirring is useless. Crossover: advection beats diffusion beyond L* = D/u (~30 µm for typical D and bacterial v). | Purcell (1977) Am J Phys 45:3–11 |
| Damköhler number | Da | Da_I = k·τ (τ = residence time); Da_II = kL²/D | ratio of reaction rate to transport rate | Da ≪ 1 → reaction-limited (stirring does nothing). Da ≫ 1 → transport-limited (the problem is delivery, not catalysis). Da ≈ 1 → both matter; model, don't estimate. | NA-07 (standard chemical-engineering definition) |
| Froude number | Fr | Fr = v²/(gL) — some authors use Fr = v/√(gL); one is the square of the other. A Froude number without its convention stated is defective. | ratio of inertial to gravitational forces; L = hip height (gait) or waterline length (hulls) | Walk→run transition at Fr ≈ 0.5 — scoped to ADULT HUMANS AT 1 g. It FAILED off-Earth: in actual lunar gravity the measured transition was Fr = 1.39 ± 0.45, with 6 of 8 subjects choosing Fr > 1.0 (De Witt et al. 2014). The inverted-pendulum mechanical ceiling is Fr = 1. | Alexander (1976) Nature 261:129–130; Alexander (1983) J. Zool.; De Witt et al. (2014) JEB 217:3200–3203; Prescott et al. (2025) Biol Lett 21:20250191 |
| Strouhal number | St | St = fA/U | ratio of oscillatory to forward speed; f = beat frequency, A = peak-to-peak amplitude, U = cruise speed | 0.2 < St < 0.4 AT CRUISE — the band of high propulsive efficiency (Taylor, Nudds & Thomas 2003). Scope is the science: not takeoff, not manoeuvre, not hovering. Individual scatter is large — only 44% of 248 odontocete values fall in 0.225–0.275 (Rohr & Fish 2004). Eloy (2012) models the OPTIMAL St as size-dependent, rising 0.15 → 0.8 from the largest cetaceans to the smallest tadpoles. | Taylor, Nudds & Thomas (2003) Nature 425:707–711; Bush & Hu (2006) ARFM 38:339–369; Rohr & Fish (2004) JEB 207:1633–1642; Eloy (2012) J Fluids Struct 30:205–218 |
| Womersley number | α | α = R√(ωρ/μ), ω = 2πf | ratio of transient (oscillatory) inertia to viscous shear | α ≫ 1 (aorta ≈13.2, some studies ≈20.3): inertia-dominated, blunt plug-like profile lagging the pressure gradient. α ≪ 1 (capillary ≈0.005; all microcirculation < 1): quasi-steady, Poiseuille-like, parabolic and in phase — the capillary does not know the heart is beating. | Cardiovasc. Eng. Technol. (2024) doi 10.1007/s13239-024-00723-4 |
| Weber number | We | We = ρU²w/σ | ratio of inertia to surface tension; σ = surface tension (air–water ≈ 0.07 N/m), w = leg width | We < 1 → the driving leg's meniscus survives — satisfied by all water-walking insects APART FROM the galloping fisher spider (carry the exception, it is real). Bush & Hu report the fit Bo ∼ We across water walkers. | Bush & Hu (2006) ARFM 38:339–369; Hu, Chan & Bush (2003) Nature 424:663–666 |
| Bond (Eötvös) number | Bo | Bo = ρghw/σ | ratio of gravity to surface tension | Bo < 1 → supported by surface tension. The capillary length is the crossover: ℓ_c = (σ/ρg)^(1/2) ≈ 2.6 mm (CN-02 recomputes 2.71 mm at 25 °C). Below it, surface tension dominates gravity; above it, gravity wins. | Bush & Hu (2006) ARFM 38:339–369 |
| Knudsen number | Kn | Kn = λ/L; λ ≈ 68 nm for air at 1 atm, 25 °C | ratio of molecular mean free path to system size — where 'fluid' stops being a fluid | Gas flows: continuum Kn < 0.01 (Navier–Stokes, no-slip); slip 0.01–0.1 (N–S usable IF slip boundary conditions are added); transition 0.1–10 (kinetic theory required); free-molecular > 10 (molecules collide only with walls). | standard rarefied-gas references; standard kinetic theory |
| Deborah number | De | De = t_relax / t_observe | ratio of the material's relaxation time to your observation time | De ≫ 1 → BEHAVES AS a solid. De ≪ 1 → BEHAVES AS a liquid. Not 'appears to' — behaves as. | Reiner (1964) Physics Today 17(1):62, doi 10.1063/1.3051374; mantle viscosity quoted in Purcell (1977) |
| Prandtl number | Pr | Pr = ν/α | ratio of momentum to thermal diffusivity | Pr ≪ 1 → heat outruns momentum; thermal boundary layer THICKER than the velocity layer. | standard property tables |
| Schmidt number | Sc | Sc = ν/D | ratio of momentum to mass diffusivity — Prandtl's mass-transfer twin | Sc ≫ 1 in liquids: momentum spreads far faster than solute. | NA-07 'The rest of the kit' |
| Nusselt number | Nu | Nu = hL/k_fluid | ratio of total to conductive heat transfer | Nu = 1 → pure conduction, no convective benefit. | NA-07 'The rest of the kit' |
| Sherwood number | Sh | Sh = k_c L/D | ratio of total to diffusive mass transfer — Nusselt's twin | Sphere in stagnant fluid: Sh = 2 — the diffusion-limited floor that Purcell's 4πaND expresses. | NA-07 'The rest of the kit' |
| Grashof number | Gr | Gr = gβΔT L³/ν² | ratio of buoyancy to viscous forces — free convection's Reynolds number | Gr/Re² ≫ 1 → buoyancy dominates forced flow. | NA-07 'The rest of the kit' |
| Rayleigh number | Ra | Ra = Gr·Pr = gβΔT L³/(να) | ratio of buoyancy to diffusive damping | Ra_c = 1707.762 (rigid–rigid boundaries), critical wavenumber ≈ 3.117, INDEPENDENT OF Pr AT ONSET. Below it, no convection; above it, Bénard cells. | Rayleigh–Bénard linear stability |
| Biot number | Bi | Bi = hL/k_solid | ratio of internal conductive to surface resistance | Bi < 0.1 → lumped-capacitance admissible. MODELED: an engineering convention, not a law. | standard heat-transfer texts |
| Mach number | Ma | Ma = u/c | ratio of flow speed to sound speed | Ma < 0.3 → density change <~5%, incompressible admissible (a convention). Ma = 1 → shocks. | standard gas dynamics |
| Rossby number | Ro | Ro = U/(fL), f = 2Ω sin φ; Ω = 7.2921 × 10⁻⁵ rad/s, f(45°) = 1.031 × 10⁻⁴ s⁻¹ | ratio of inertial to Coriolis forces — whether rotation matters at all | Ro ≈ 0.1 → rotation DOMINATES → geostrophic balance, which is the whole reason weather maps work: pressure-gradient and Coriolis forces nearly balance, so wind blows ALONG isobars rather than across them. Ro ≫ 1 → rotation irrelevant. Inside the Hadley cells the vorticity-based LOCAL Rossby number is order 1 — a different definition and a different regime. | CN-03; Shapiro (1962) Nature 196(4859):1080–1081 |
| Golden angle (phyllotactic divergence) | ψ / θ_φ / α_golden | ψ = 360/φ² = 137.507764050038…°, φ = (1+√5)/2 | dimensionless divergence angle; the attractor of repulsion-driven sequential primordia | Clusters near 137.5° in spiral-phyllotactic vascular plants — but NOT universal: in the largest sunflower study with explicit inclusion criteria, 18% of scored counts (136/768) were NON-Fibonacci (Swinton & Ochu 2016). Scope: the attractor at LOW control parameter G — the same experiment yields OTHER angles at other G. | Douady & Couder (1992) Phys. Rev. Lett. 68(13):2098–2101, DOI 10.1103/PhysRevLett.68.2098; Swinton & Ochu (2016) R. Soc. Open Sci. 3:160091 |
| Drag anisotropy ratio (resistive-force theory) | ζ⊥/ζ∥ | ζ⊥/ζ∥ = 2(ln(2λ/a) − 0.5)/(ln(2λ/a) + 0.5) | ratio of normal to tangential drag on a slender filament — the asymmetry that makes flagellar thrust possible at all | ≈2 ASYMPTOTIC ONLY; ~1.5–1.8 at realistic aspect ratios (ln(2λ/a) ≈ 3–5). Strictly < 2 for any real filament; reaches 2 only as aspect ratio → ∞. Set the ratio to 1 and thrust integrates to ZERO — travelling wave or not. | Gray & Hancock 1955, J Exp Biol 32:802–814 |
| Buckingham Pi theorem | Π | Number of groups = n − j, where j = the RANK of the dimensional matrix (NOT the number of base dimensions — that is the common failure mode, and it is wrong whenever the dimensions are not independently represented). Then Π₁ = f(Π₂, …, Π_{n−j}). | the recipe for generating your OWN dimensionless groups | Worked example — drag on a sphere: variables F, ρ, U, D, μ; n = 5, rank j = 3 → 2 groups. Π₁ = F/(ρU²D²) → drag coefficient C_d; Π₂ = μ/(ρUD) → 1/Re. Result: C_d = f(Re). Five variables collapse to one curve. | Buckingham (1914) Physical Review 4(4):345–376, doi 10.1103/PhysRev.4.345 (not first: Vaschy 1892; Federman and Riabouchinsky 1911 have priority) |
| Dynamic similarity and the conflict you cannot escape | Fr vs Re | Fr matching requires v_m = v_s·√λ (model goes SLOWER); Re matching requires v_m = v_s/λ (model goes FASTER) | geometrically similar systems sharing every relevant group have identical dimensionless results — but you can rarely match all groups at once | At scale λ = 1/25: v_m = 0.2·v_s versus v_m = 25·v_s. INCOMPATIBLE BY A FACTOR OF 125. No cleverness removes this. | NA-07 'Dynamic similarity — and the conflict you cannot escape' |
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