Einasto profile

E237662

The Einasto profile is a mathematical model used in astrophysics to describe how the density of dark matter and stars varies smoothly with distance from the centers of galaxies and galaxy clusters.

All labels observed (1)

Label Occurrences
Einasto profile canonical 4

How this entity was disambiguated

Statements (50)

Predicate Object
instanceOf astrophysical model ⓘ
density profile ⓘ
mathematical model ⓘ
advantageOver Navarro–Frenk–White profile in fitting simulated dark matter halos ⓘ
appliesTo bulges of spiral galaxies ⓘ
elliptical galaxies ⓘ
galactic dark matter halos ⓘ
galaxy clusters ⓘ
assumes spherical symmetry in its simplest form ⓘ
canBeGeneralizedTo axisymmetric systems ⓘ
comparedTo Navarro–Frenk–White profile ⓘ
contrastWith isothermal sphere profile ⓘ
power-law density profiles ⓘ
dependsOn radius from system center ⓘ
describes smooth variation of density with radius ⓘ
describesComponent inner regions of dark matter halos ⓘ
outer regions of dark matter halos ⓘ
field astrophysics ⓘ
hasFunctionalForm ρ(r) = ρ_e · exp{−d_n[(r/r_e)^{1/n} − 1]} ⓘ
hasParameter d_n ⓘ
n ⓘ
r_e ⓘ
ρ_e ⓘ
introducedInContextOf galactic structure studies ⓘ
mathematicalType exponential of a power-law in radius ⓘ
namedAfter Jaan Einasto ⓘ
originCountryOfEponym Estonia ⓘ
parameterMeaning d_n is a constant fixed by n ⓘ
n is a shape parameter ⓘ
r_e is a scale radius ⓘ
ρ_e is the density at radius r_e ⓘ
property curved logarithmic slope ⓘ
finite central density ⓘ
monotonically decreasing density with radius ⓘ
spherically symmetric in its standard form ⓘ
relatedConcept Sérsic profile ⓘ
relationship mathematically analogous to the Sérsic profile in 3D ⓘ
scaleBehavior logarithmic slope varies continuously with radius ⓘ
timePeriodOfIntroduction 1960s ⓘ
typicalUseCase fitting observed galaxy mass distributions ⓘ
fitting simulated ΛCDM dark matter halos ⓘ
usedFor describing radial density profiles of galaxies ⓘ
describing radial density profiles of galaxy clusters ⓘ
modeling dark matter density distributions ⓘ
modeling stellar density distributions ⓘ
usedIn analysis of rotation curves of galaxies ⓘ
cosmological N-body simulations ⓘ
dark matter halo characterization ⓘ
gravitational lensing studies ⓘ
mass modeling of galaxy clusters ⓘ

How these facts were elicited

Referenced by (4)

Full triples — surface form annotated when it differs from this entity's canonical label.

Jaan Einasto → notableFor → Einasto profile ⓘ
Burkert profile → comparedWith → Einasto profile ⓘ