Authors: Karan R.Takkhi
Dark matter is considered to be responsible for the unexpectedly high velocities exhibited by the galactic components within the galactic disc and by the galaxies situated within rich galaxy clusters. The velocities are high and the total light output due to visible matter alone cannot account for all the mass and gravity for the overall observed stability. The presence of additional matter in the form of dark matter is required to explain the gravitational stability at such high velocities. I present a theory based on the study of certain characteristics responsible for causing the galaxy rotation problem. Solution to the mentioned problem has been discussed by considering the baryonic matter distribution only. The orbital stability of galaxies at high velocities within rich galaxy clusters has also been taken into account. The theory provides a credible solution without considering dark matter and also without modifying the laws of gravity.
Comments: 8 pages, 6 figures, 2 tables
Unique-IP document downloads: 64 times
Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary. In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution. Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.
Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.