quantity

scale factor

scale factor — from formula anatomy
23 related articles · 6 formulas

Description

A 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.

History

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.

How it works

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.

In practice

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.

Fun fact

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.

Concept graph →

Formulas

$$q = - rac{ rac{ ext{d}^2 a}{ ext{d} t^2} a}{ig( rac{ ext{d} a}{ ext{d} t}ig)^2}$$
Measures acceleration of the universe's expansion.
What is in the formula
qvariableDeceleration parameter — deceleration parameter
avariableScale factor of the universe — scale factor
tvariableCosmic time — time second
d/dtoperatorComputes the rate of change over time — time derivative
d^2/dt^2operatorComputes the acceleration over time — second time derivative
$$ds_E^2 = d\tau^2 + a^2(\tau) d\Omega_3^2$$
Euclidean metric for closed universe with scale factor a(τ).
What is in the formula
ds_EvariableEuclidean line element — line element metre
τvariableEuclidean time coordinate — time second
avariableScale factor of the universe — scale factor
dΩ_3variableLine element on a unit 3-sphere — solid angle element
$$\frac{\ddot{a}}{a} = -\frac{4\pi G}{3}(\rho + 3p)$$
Relates acceleration to energy density and pressure.
What is in the formula
\ddot{a}variablesecond time derivative of scale factor — scale factor acceleration per second squared
avariablescale factor — scale factor
\rhovariableenergy density — energy density joule per cubic metre
pvariablepressure — pressure pascal
GconstantConstant of gravitation in Einstein's field equations. — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared
$$w(a) = w_0 + w_a (1 - a)$$
Dark energy equation of state evolves with scale factor.
What is in the formula
wvariableDark energy equation of state parameter — equation of state parameter
avariableScale factor of the universe — scale factor
w_0variableEquation of state parameter at present epoch — equation of state parameter
w_avariableCoefficient of the evolution term — equation of state parameter
$$k = aH$$
A mode enters the horizon when its wavelength equals the Hubble radius.
What is in the formula
kvariablecomoving wavenumber — wavenumber reciprocal metre
avariablescale factor — scale factor
HvariableHubble parameter — hubble parameter reciprocal second
$$\kappa(\boldsymbol{\theta}) = \frac{3H_0^2\Omega_m}{2c^2} \int_0^{\chi} d\chi' \, \frac{q(\chi')}{a(\chi')} f_K(\chi') \delta(f_K(\chi')\boldsymbol{\theta}, \chi')$$
Convergence is a weighted integral of density contrast along the line of sight.
What is in the formula
kappavariableweak lensing convergence — convergence
thetavariableangular position on the sky — angular position radian
chivariablecomoving distance to the source — comoving distance metre
chi'variablecomoving distance along the line of sight — comoving distance metre
qvariablelensing efficiency function — lensing efficiency
avariablescale factor — scale factor
f_Kvariablecomoving angular diameter distance — comoving angular diameter distance metre
deltavariablematter density contrast — density contrast
H_0constantcurrent expansion rate of the universe — hubble constant = 2.2e-18 per second
Omega_mconstantratio of matter density to critical density today — matter density parameter = 0.315
cconstantspeed of light in vacuum — speed of light = 299792458 metre per second
∫operatorsummation over infinitesimal elements — integral

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