Gravitational Magnus effect
L. Filipe O. Costa, Rita Franco, Vitor Cardoso

TL;DR
This paper demonstrates the existence of a gravitational Magnus effect, analogous to the fluid dynamics phenomenon, arising from spin-curvature interactions in General Relativity, with potential observable consequences in astrophysical systems.
Contribution
It provides a rigorous derivation of the gravitational Magnus effect from the Mathisson-Papapetrou equations and explores its implications in various astrophysical contexts.
Findings
The effect causes secular orbital precessions detectable by future experiments.
Explicit calculations for dark matter halos, accretion disks, and FLRW spacetime.
Clarification of action-reaction laws in post-Newtonian gravity.
Abstract
It is well known that a spinning body moving in a fluid suffers a force orthogonal to its velocity and rotation axis --- it is called the Magnus effect. Recent simulations of spinning black holes and (indirect) theoretical predictions, suggest that a somewhat analogous effect may occur for purely gravitational phenomena. The magnitude and precise direction of this "gravitational Magnus effect" is still the subject of debate. Starting from the rigorous equations of motion for spinning bodies in General Relativity (Mathisson-Papapetrou equations), we show that indeed such an effect takes place and is a fundamental part of the spin-curvature force. The effect arises whenever there is a current of mass/energy, non-parallel to a body's spin. We compute the effect explicitly for some astrophysical systems of interest: a galactic dark matter halo, a black hole accretion disk, and the…
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