On the flat galactic rotational curves in $f(\mathcal{R})$ gravity
Muhammad Usman

TL;DR
This paper investigates whether f(R) gravity can explain flat galactic rotation curves without dark matter by solving field equations numerically for various matter distributions and relating the results to scalar field models.
Contribution
It provides numerical solutions to f(R) gravity field equations for different galaxy profiles, showing deviations from linear R relations and linking to scalar field dark matter models.
Findings
Modified gravity can produce flat rotation curves without dark matter.
Solutions show significant deviations from linear R for matter distributions.
Scalar dark matter from modified gravity does not cluster like baryonic matter.
Abstract
A mysterious dark matter is supposed to exist in the galactic halos. In this contrast, we discuss the possibility of explaining the flat rotational velocity curves in f(R) gravity by solving field equations numerically in vacuum and for different matter distributions. For a spherically symmetric static space-time (as the galactic environment) we give metric for constant rotational velocity regions. For a constant rotational velocity region, we prove that all values of rotational velocities (most importantly observed rotational velocity ~200-300Km/s) do not lead to an analytic solution of the vacuum field equations. We then obtain numerical solutions of the field equations in vacuum and for three types of mass distributions named: (1) power law density profile, (2) simple model for galaxy with a core and, (3) Navarro, Frank and White (NFW) profile, for M31 and Milky way galaxy. The…
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