Einasto density profile

E237665

The Einasto density 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.

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All labels observed (3)

Label Occurrences
Einasto density profile canonical 1
Einasto index 1
Sérsic profile 1

Statements (46)

Predicate Object
instanceOf astrophysical model
density profile
galactic structure model
advantage better fits to simulated dark matter halos than NFW in many cases
appliesTo dark matter halos
galaxies
galaxy clusters
assumes spherical symmetry in simplest form
canBeExtendedTo axisymmetric systems
characteristic curved logarithmic slope
smoothly varying density with radius
comparedWith Burkert profile
Hernquist profile
Jaffe profile
contrastWith Navarro–Frenk–White profile
isothermal sphere profile
creator Jaan Einasto
dependsOn radius
describes radial mass density distribution
field astrophysics
cosmology
generalizes Sérsic profile
hasParameter Einasto density profile self-linksurface differs
surface form: Einasto index

scale density
scale radius
shape parameter
mathematicalForm exponential of a power of radius
namedAfter Jaan Einasto
originatedIn 1970s
property finite central density
non-power-law inner slope
relatedConcept Sérsic index
dark matter halo profile
halo mass–concentration relation
similarTo Sérsic profile
usedFor describing galaxy rotation curve mass models
fitting N-body simulation halos
modeling dark matter distribution
modeling stellar distribution
usedIn analysis of halo concentration
cosmological N-body simulations
dynamical modeling of galaxies
strong lensing mass models
weak lensing mass models
usedToInfer dark matter fraction in galaxies
total mass distribution from kinematics

How these facts were elicited

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Instruction
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# Requirements
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Input
Subject: Einasto density profile
Description of subject: The Einasto density 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.

Referenced by (3)

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

Jaan Einasto notableConcept Einasto density profile
Einasto profile relatedConcept Einasto density profile
this entity surface form: Sérsic profile
Einasto density profile hasParameter Einasto density profile self-linksurface differs
this entity surface form: Einasto index