Interpretation of galaxy rotation curves from primordial black holes in 4D Einstein-Gauss-Bonnet gravity
M. Bousder

TL;DR
This paper proposes a novel model using 4D Einstein-scalar-Gauss-Bonnet gravity to explain galaxy rotation curves through primordial black holes, linking dark matter phenomena with black hole physics.
Contribution
It introduces a new approach connecting galaxy rotation curves with primordial black holes within 4D Einstein-Gauss-Bonnet gravity, incorporating scalar fields and Gauss-Bonnet coupling.
Findings
Reproduces flat galaxy rotation curves using the model.
Suggests primordial black holes as dark matter candidates within specific mass ranges.
Provides a natural explanation for observed matter and dark matter proportions.
Abstract
We develop a novel approach to the dark matter halos in the context of 4 dimensional Einstein--scalar-Gauss-Bonnet gravity to reproduce the flat rotation curves of galaxies. Moreover, the Gauss-Bonnet coupling describes the interior structure of the galaxies, while there is a presence of a scalar field in the galaxy edges. This can provide an interesting interpretation for the functional coupling . We discuss how this comparison can naturally drive the observed percentages of matter and dark matter in the Universe. The effective mass range\ in our model is , which is in good agreement with the constraints on primordial black holes.
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Galaxies: Formation, Evolution, Phenomena
