Rotation Curves of Galaxies by Fourth Order Gravity
A. Stabile, G. Scelza

TL;DR
This paper explores how Fourth Order Gravity, combined with dark matter, can explain galactic rotation curves, offering an alternative to dark matter dominance and comparing theoretical predictions with observational data.
Contribution
It introduces a systematic analysis of galactic rotation curves within Fourth Order Gravity, considering both with and without dark matter, and compares results to classical General Relativity.
Findings
Fourth Order Gravity modifies gravitational potential with Yukawa terms.
Rotation curves can be higher or lower than GR depending on Lagrangian terms.
Large-distance behavior shows Keplerian decline even with dark matter.
Abstract
We investigate the radial behavior of galactic rotation curves by a Fourth Order Gravity adding also the Dark Matter component. The Fourth Order Gravity is a Lagrangian containing the Ricci scalar, the Ricci and Riemann tensor, but the rotation curves are depending only on two free parameters. A systematic analysis of rotation curves, in the Newtonian Limit of theory, induced by all galactic sub-structures of ordinary matter is shown. This analysis is presented for Fourth Order Gravity with and without Dark Matter. The outcomes are compared with respect to classical outcomes of General Relativity. The gravitational potential of point-like mass is the usual potential corrected by two Yukawa terms. The rotation curve is higher or also lower than curve of General Relativity if in the Lagrangian the Ricci scalar square is dominant or not with respect to the contribution of the Ricci tensor…
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