Transient spiral arms from far out of equilibrium gravitational evolution
David Benhaiem, Michael Joyce, Francesco Sylos Labini

TL;DR
This paper models how out-of-equilibrium gravitational evolution can produce transient spiral structures resembling galaxies, suggesting an alternative explanation for observed galaxy dynamics without dark matter.
Contribution
It introduces a simple idealized model demonstrating that spiral arms can form from non-stationary mass distributions, challenging traditional dark matter or modified gravity explanations.
Findings
Spiral structures can last tens of dynamical times in the model.
Velocity distributions show potential observational signatures.
Radial motions may be detectable at large galactic scales.
Abstract
We describe how a simple class of out of equilibrium, rotating and asymmetrical mass distributions evolve under their self-gravity to produce a quasi-planar spiral structure surrounding a virialized core, qualitatively resembling a spiral galaxy. The spiral structure is transient, but can survive tens of dynamical times, and further reproduces qualitatively noted features of spiral galaxies as the predominance of trailing two-armed spirals and large pitch angles. As our models are highly idealized, a detailed comparison with observations is not appropriate, but generic features of the velocity distributions can be identified to be potential observational signatures of such a mechanism. Indeed, the mechanism leads generically to a characteristic transition from predominantly rotational motion, in a region outside the core, to radial ballistic motion in the outermost parts. Such radial…
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