Burkert profile

E820923

The Burkert profile is a cored dark matter halo density model commonly used in astrophysics to describe the flat central density distributions inferred from galaxy rotation curves.

All labels observed (1)

Label Occurrences
Burkert profile canonical 1

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf astrophysical model ⓘ
dark matter halo density profile ⓘ
addresses core–cusp problem ⓘ
appliesTo dwarf spheroidal galaxies ⓘ
late-type spiral galaxies ⓘ
assumes spherical symmetry ⓘ
asymptoticBehavior ρ(r) ∝ r⁻³ at large radii ⓘ
category dark matter phenomenology ⓘ
galactic structure models ⓘ
centralDensity ρ₀ ⓘ
centralSlope 0 ⓘ
comparedWith Einasto profile ⓘ
isothermal sphere profile ⓘ
contrastsWith Navarro–Frenk–White profile ⓘ
cuspy dark matter halo profiles ⓘ
coreDensityRadiusProduct approximately constant across galaxies (empirical claim) ⓘ
densityExpression ρ(x) = ρ₀ / [(1 + x)(1 + x²)] ⓘ
describes cored dark matter halo ⓘ
flat central density distribution ⓘ
dimensionlessRadius x = r/r₀ ⓘ
fits rotation curves of dwarf galaxies ⓘ
rotation curves of low surface brightness galaxies ⓘ
hasCore constant-density core ⓘ
hasCoreRadius r₀ ⓘ
hasDensityCore non-singular center ⓘ
hasFunctionalForm ρ(r) = ρ₀ / [(1 + r/r₀)(1 + (r/r₀)²)] ⓘ
hasParameter r₀ ⓘ
ρ₀ ⓘ
implies approximately flat rotation curves in inner regions ⓘ
introducedBy Andreas Burkert ⓘ
introducedIn 1995 ⓘ
massProfile M(r) = 4π ∫₀ʳ ρ(r′) r′² dr′ ⓘ
mathematicalForm two-parameter density profile ⓘ
motivatedBy galaxy rotation curves ⓘ
namedAfter Andreas Burkert ⓘ
outerSlope -3 ⓘ
publication Burkert 1995, Astrophysical Journal Letters ⓘ
relatedConcept cored halo ⓘ
dark matter distribution in galaxies ⓘ
halo core radius ⓘ
usedFor deriving dark matter halo masses ⓘ
fitting observed rotation curves ⓘ
mass modeling of galaxies ⓘ
usedIn astrophysics ⓘ
dark matter halo modeling ⓘ
empirical scaling relations of dark matter halos ⓘ
galaxy dynamics ⓘ

How these facts were elicited

Referenced by (1)

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

Einasto density profile → comparedWith → Burkert profile ⓘ