Prograde spin-up during gravitational collapse
Rico G. Visser, Marc G. Brouwers

TL;DR
This paper introduces a geometric mechanism explaining how collapsing clouds gain prograde rotation, linking initial conditions and external potential to the spin orientation of resulting celestial objects.
Contribution
The study presents a novel geometric model and analytical calculations showing how external shear induces prograde spin-up during collapse, applicable across various astrophysical contexts.
Findings
Prograde spin-up scales quadratically with time during collapse.
The rotational gain depends strongly on the initial cloud size and distance from the potential source.
The mechanism explains the prevalence of prograde rotation in Kuiper belt binaries.
Abstract
Asteroids, planets, stars in some open clusters, as well as molecular clouds appear to possess a preferential spin-orbit alignment, pointing to shared processes that tie their rotation at birth to larger parent structures. We present a new mechanism that describes how collections of particles or 'clouds' gain a prograde rotational component when they collapse or contract while subject to an external, central force. The effect is geometric in origin, as relative shear on curved orbits moves their shared center-of-mass slightly inward and toward the external potential during a collapse, exchanging orbital angular momentum into aligned (prograde) rotation. We perform illustrative analytical and N-body calculations to show that this process of prograde spin-up proceeds quadratically in time () until the collapse nears completion. The total rotational gain…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
