Dark Matter near gravitating bodies
H. B. Tran Tan, V. V. Flambaum, J. C. Berengut

TL;DR
This paper demonstrates that dark matter density and current are significantly enhanced near massive astronomical objects like neutron stars and black holes, potentially making dark matter interactions observable.
Contribution
It reveals that gravitational fields of dense bodies can amplify dark matter effects, a novel insight into dark matter behavior near extreme objects.
Findings
Dark matter density increases near neutron stars and black holes.
Enhanced dark matter effects could be detectable observationally.
Gravitational interactions influence dark matter distribution significantly.
Abstract
In this paper, we show that in the vicinity of certain astronomical bodies, e.g., a Neutron Star, a Black Hole, there exist significant enhancements of Dark Matter's density and current, due to its interaction with the gravitational field of the bodies. This enhancement implies that the effects of Dark Matter - Normal Matter interactions are enhanced and hence might be observable.
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Taxonomy
TopicsRelativity and Gravitational Theory · Radioactive Decay and Measurement Techniques · Dark Matter and Cosmic Phenomena
