Abstract
In theories of gravitation in which dimensional parameters are dynamically induced, one can have non-topological-soliton solutions. This article reviews related topics connected with such solutions.
The existence of such solutions in curved spacetime can give rise to halos of gravity (g-) balls with the “gravitational constant” having different values inside and outside the ball.
Such g-balls can have quite an interesting bearing on the dark matter problem over galactic and cluster scales. We describe the origin of such solutions and speculate on related problems in Cosmology. Such objects would naturally occur in a large class of induced gravity models in which we have scalar fields non minimally coupled to the scalar curvature.
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Lohiya, D. Non-topological solitons in non-minimally coupled scalar fields: theory and consequences. Astrophys Space Sci 232, 1–22 (1995). https://doi.org/10.1007/BF00627539
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DOI: https://doi.org/10.1007/BF00627539