SCHWARZSCHILD-DE SITTER AND MECHANICAL APPROACHES COMPARISON WITH RESPECT TO DARK MATTER HALOS
dc.contributor.author | Brilenkov, R. D. | |
dc.contributor.author | Eingorn, Maxim V. | |
dc.contributor.author | Zhuk, Oleksandr I. | |
dc.date.accessioned | 2014-03-29T02:01:35Z | |
dc.date.available | 2014-03-29T02:01:35Z | |
dc.date.issued | 2013 | |
dc.description | Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2013 . – Vol.26/2 | uk |
dc.description.abstract | 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. | uk |
dc.identifier.citation | Odessa Astronomical Publications | uk |
dc.identifier.uri | https://dspace.onu.edu.ua/handle/123456789/4787 | |
dc.language.iso | en | uk |
dc.publisher | Astroprint | uk |
dc.relation.ispartofseries | ;vol. 26, issue 2, p. 179 | |
dc.subject | Schwarzschild-de Sitter | uk |
dc.subject | mass | uk |
dc.subject | potential distributions | uk |
dc.subject | dark matter | uk |
dc.subject | clusters of galaxies | uk |
dc.subject | dark energy influence | uk |
dc.title | SCHWARZSCHILD-DE SITTER AND MECHANICAL APPROACHES COMPARISON WITH RESPECT TO DARK MATTER HALOS | uk |
dc.type | Article | uk |
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