Galactic rotation curves of spiral galaxies and dark matter in f(R,T) gravity theory
Gayatri Mohan, Umananda Dev Goswami

TL;DR
This paper explores whether the flat rotation curves of spiral galaxies can be explained without dark matter by using $f( ext{R},T)$ gravity theory, deriving field equations, and fitting observational data.
Contribution
It introduces a specific $f( ext{R},T)$ gravity model that accounts for galactic rotation curves without dark matter, supported by observational data fitting.
Findings
The model nearly explains galaxy rotation curves without dark matter.
Theoretical predictions match observed velocities for nineteen galaxies.
Dark matter may not be necessary in this gravity framework.
Abstract
Galactic rotation curve is a powerful indicator of the state of the gravitational field within a galaxy. The flatness of these curves indicates the presence of dark matter in galaxies and their clusters. In this paper, we focus on the possibility of explaining the rotation curves of spiral galaxies without postulating the existence of dark matter in the framework of gravity, where the gravitational Lagrangian is written by an arbitrary function of , the Ricci scalar and of , the trace of energy-momentum tensor . We derive the gravitational field equations in this gravity theory for the static spherically symmetric spacetime and solve the equations for metric coefficients using a specific model that has minimal coupling between matter and geometry. The orbital motion of a massive test particle moving in a stable circular orbit is considered…
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Solar and Space Plasma Dynamics
