A nearly cylindrically symmetric source in the Brans-Dicke gravity as the generator of the rotational curves of the galaxies
S. Mittmann dos Santos, J. M. Hoff da Silva, M. E. X. Guimar\~aes, J., L. Neto

TL;DR
This paper proposes a nearly cylindrically symmetric solution within Brans-Dicke gravity to explain the observed flat rotation curves of galaxies, addressing a longstanding astrophysical puzzle.
Contribution
It introduces a novel cylindrical symmetric model in Brans-Dicke gravity as a potential explanation for galaxy rotation curves.
Findings
Model reproduces the observed velocity increase in galaxies
Provides an alternative to dark matter explanations
Suggests scalar-tensor theories can account for galactic dynamics
Abstract
Observation shows that the velocities of stars grow by approximately 2 to 3 orders of magnitude when the distances from the centers of the galaxies are in the range of kpc to kpc, before they begin to tend to a constant value. Up to know, the reason for this behavior is still a matter for debate. In this work, we propose a model which adequately describes this unusual behavior using a (nearly) cylindrical symmetrical solution in the framework of a scalar-tensor-like (the Brans-Dicke model) theory of gravity.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Solar and Space Plasma Dynamics
