Einasto profile explained

The Einasto profile (or Einasto model) is a mathematical function that describes how the density

\rho of a spherical stellar system varies with distance r from its center. Jaan Einasto introduced his model at a 1963 conference in Alma-Ata, Kazakhstan.^[1]

The Einasto profile possesses a power law logarithmic slope of the form:$$\backslash gamma(r)\; \backslash equiv\; -\backslash frac\; \backslash propto\; r^$$which can be rearranged to give$$\backslash rho(r)\; \backslash propto\; \backslash exp\; .$$The parameter

\alpha controls the degree of curvature of the profile. This can be seen by computing the slope on a log-log plot:$$\backslash frac\; \backslash propto\; -r^\; .$$

The larger

\alpha , the more rapidly the slope varies with radius (see figure). Einasto's law can be described as a generalization of a power law, \rho\propto r ^{-N} , which has a constant slope on a log-log plot.

Einasto's model has the same mathematical form as Sersic's law, which is used to describe the surface brightness (i.e. projected density) profile of galaxies, except that the Einasto model describes a spherically symmetric density distribution in 3 dimensions, whereas the Sersic law describes a circularly symmetric surface density distribution in two dimensions.

Einasto's model has been used to describe many types of system, including galaxies,^[2] and dark matter halos.^{[3] [4]}

See also

• NFW profile

External links

• Spherical galaxy models with power-law logarithmic slope. A comprehensive paper that derives many properties of stellar systems obeying Einasto's law.

Notes and References

1. [Jaan Einasto|J. Einasto]
2. J. Einasto and U. Haud (1989), Galactic models with massive corona. I - Method. II - Galaxy Astron. Astrophys. 223, 89
3. Navarro. Julio. Julio Navarro. etal. The inner structure of ΛCDM haloes - III. Universality and asymptotic slopes. Monthly Notices of the Royal Astronomical Society. April 2004. 349. 3. 1039–1051. 10.1111/j.1365-2966.2004.07586.x. free . astroph/0311231. 2004MNRAS.349.1039N.
4. Merritt . David . David Merritt . Graham . Alister . etal . 2006 . Empirical Models for Dark Matter Halos . The Astronomical Journal . 132 . 6 . 2685–2700 . astro-ph/0509417 . 10.1086/508988 . 2006AJ....132.2685M. 14511019 .