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On the gravitational stability of baryonic gas clouds in the background of dark matter

โœ Scribed by David Tsiklauri

Publisher
Elsevier Science
Year
2000
Tongue
English
Weight
54 KB
Volume
5
Category
Article
ISSN
1384-1076

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## Abstract We start from the assumption that the gravitational source strength of matter becomes weaker if the matter density is greater than a certain value and is equal to zero for matter densities greater than another value. We give a phenomenological description of this assumption. One consequ