SCHWARZSCHILD-DE SITTER AND MECHANICAL APPROACHES COMPARISON WITH RESPECT TO DARK MATTER HALOS

We compare the Schwarzschild-de Sitter approach to deriving mass and potential distributions and corresponding parameters associated with dark matter halos for clusters of galaxies with the mechanical one, taking into account cosmological effects, in particular, dark energy influence.

Bibliographic Details
Main Authors: R. Brilenkov, M. Eingorn, A. Zhuk
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2013-11-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/82545