/ Astrophysics astro-ph/0301543


Cold dark matter as cosmic evolution of galaxies in relative units


Gusev, A.A. (Dubna, JINR) ; Pervushin, Victor N. (Dubna, JINR) ; Vinitsky, S.I. (Dubna, JINR) ; Zorin, A.G. (Dubna, JINR)

Published in: Astrophysics / Astrofiz.
Year: 2004 / 2004
Vol.: 47 / 47
Page No: 242-247 / 283-288

Abstract: The Kepler problem is considered in a space with the Friedmann--Lemaitre--Robertson--Walker metrics of the expanding universe. The covariant differential of the Friedmann coordinates (X=a(t)x) is considered as a possible mechanism of the formation of galaxies and clusters of galaxies. The cosmic evolution leads to decreasing energy of particles, causing free particles to be captured in bound states. In this approach the evolution of the universe plays the role usually inscribed to Cold Dark Matter.

Web-Page: http://www.adsabs.harvard.edu/abs/2004Ap.....47..242G; http://dx.doi.org/10.1023/B:ASYS.0000031839.43141.d2

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