ROTATION CURVES OF GALAXIES - MISSING MASS OR MISSING PHYSICS

Authors
Citation
V. Krishan, ROTATION CURVES OF GALAXIES - MISSING MASS OR MISSING PHYSICS, Pramana, 49(1), 1997, pp. 147-154
Citations number
16
Categorie Soggetti
Physics
Journal title
ISSN journal
03044289
Volume
49
Issue
1
Year of publication
1997
Pages
147 - 154
Database
ISI
SICI code
0304-4289(1997)49:1<147:RCOG-M>2.0.ZU;2-U
Abstract
The rotation curves of galaxies are modelled using very special proper ties of an hydrodynamically turbulent fluid possessing helicity fluctu ations. The development of correlations among these fluctuations leads to the formation of organized structures characterized by a new flat branch of the spatial energy spectrum in addition to the well known Ko lmogorov spectrum. It is proposed that the flat nature of the rotation curves of galaxies may be a result of the energy cascading processes occuring in turbulent galactic atmospheres. Thus, in this model, there is no need of invoking dark matter to account for the flat rotation c urves of galaxies.