Galactic rotation curves in hybrid metric-Palatini gravity
Salvatore Capozziello, Tiberiu Harko, Tomi S. Koivisto, Francisco S., N. Lobo, Gonzalo J. Olmo

TL;DR
This paper explores how hybrid metric-Palatini gravity can explain galactic rotation curves without dark matter by linking observable velocities and shifts to the scalar field in the theory.
Contribution
It demonstrates that the hybrid metric-Palatini model can reproduce galactic rotation curves and relates physical quantities to observable parameters, enabling potential empirical tests.
Findings
Rotation curves can be explained without dark matter.
Scalar field parameters can be constrained by stellar velocity dispersions.
Observable quantities like Doppler shifts relate directly to the model.
Abstract
Generally, the dynamics of test particles around galaxies, as well as the corresponding mass deficit, is explained by postulating the existence of a hypothetical dark matter. In fact, the behavior of the rotation curves shows the existence of a constant velocity region, near the baryonic matter distribution, followed by a quick decay at large distances. In this work, we consider the possibility that the behavior of the rotational velocities of test particles gravitating around galaxies can be explained within the framework of the recently proposed hybrid metric-Palatini gravitational theory. The latter is constructed by modifying the metric Einstein-Hilbert action with an term in the Palatini formalism. It was shown that the theory unifies local constraints and the late-time cosmic acceleration, even if the scalar field is very light. In the intermediate galactic scale, we show…
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