scale factor — from formula anatomyA scale factor, in formula anatomy, is a dimensionless number that multiplies a quantity to change its magnitude without altering its physical nature. It appears in physics when transforming between different units, when scaling physical systems (e.g., in fluid dynamics or cosmology), or when relating model parameters to real-world values. Scale factors are crucial for dimensional analysis and for understanding how physical laws behave under changes of scale.
The concept of scaling has been used implicitly since ancient times, but it was formalized in the 19th century with the development of dimensional analysis by figures like Lord Rayleigh. In cosmology, the scale factor was introduced by Alexander Friedmann in the 1920s.
In a formula, a scale factor is often introduced as a multiplicative constant. For example, in cosmology, the scale factor a(t) describes how the universe expands: distances between galaxies scale as a(t) times their current separation. In dimensional analysis, scale factors ensure that equations are dimensionally consistent, and they can reveal how a system's behavior changes when its size is altered.
Scale factors are used in model testing (e.g., wind tunnels), in converting between unit systems, and in cosmology to describe the expansion of the universe.
In the standard model of cosmology, the scale factor has increased by about 1,100 times since the universe became transparent, meaning the universe is now 1,100 times larger than it was when the cosmic microwave background was emitted.
| q | variable | Deceleration parameter — deceleration parameter |
| a | variable | Scale factor of the universe — scale factor |
| t | variable | Cosmic time — time second |
| d/dt | operator | Computes the rate of change over time — time derivative |
| d^2/dt^2 | operator | Computes the acceleration over time — second time derivative |
| ds_E | variable | Euclidean line element — line element metre |
| τ | variable | Euclidean time coordinate — time second |
| a | variable | Scale factor of the universe — scale factor |
| dΩ_3 | variable | Line element on a unit 3-sphere — solid angle element |
| \ddot{a} | variable | second time derivative of scale factor — scale factor acceleration per second squared |
| a | variable | scale factor — scale factor |
| \rho | variable | energy density — energy density joule per cubic metre |
| p | variable | pressure — pressure pascal |
| G | constant | Constant of gravitation in Einstein's field equations. — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared |
| w | variable | Dark energy equation of state parameter — equation of state parameter |
| a | variable | Scale factor of the universe — scale factor |
| w_0 | variable | Equation of state parameter at present epoch — equation of state parameter |
| w_a | variable | Coefficient of the evolution term — equation of state parameter |
| k | variable | comoving wavenumber — wavenumber reciprocal metre |
| a | variable | scale factor — scale factor |
| H | variable | Hubble parameter — hubble parameter reciprocal second |
| kappa | variable | weak lensing convergence — convergence |
| theta | variable | angular position on the sky — angular position radian |
| chi | variable | comoving distance to the source — comoving distance metre |
| chi' | variable | comoving distance along the line of sight — comoving distance metre |
| q | variable | lensing efficiency function — lensing efficiency |
| a | variable | scale factor — scale factor |
| f_K | variable | comoving angular diameter distance — comoving angular diameter distance metre |
| delta | variable | matter density contrast — density contrast |
| H_0 | constant | current expansion rate of the universe — hubble constant = 2.2e-18 per second |
| Omega_m | constant | ratio of matter density to critical density today — matter density parameter = 0.315 |
| c | constant | speed of light in vacuum — speed of light = 299792458 metre per second |
| ∫ | operator | summation over infinitesimal elements — integral |









