The Role of Angular Momentum and Cosmic Censorship in the (2+1)-Dimensional Rotating Shell Collapse
Robert B. Mann, John J. Oh, and Mu-In Park

TL;DR
This paper investigates how angular momentum influences gravitational collapse in 3D Einstein gravity, revealing that it does not generally prevent the formation of naked singularities, challenging cosmic censorship.
Contribution
It provides a detailed analysis of rotating shell collapse in 3D gravity, showing that angular momentum alone cannot prevent naked singularity formation across various equations of state.
Findings
Shells can form BTZ black holes, Kerr-dS spacetimes, or horizonless geometries.
Angular momentum barrier prevents curvature singularity formation in pressureless shells.
Collapse to naked singularities is possible with non-zero pressure shells, regardless of angular momentum.
Abstract
We study the gravitational collapse problem of rotating shells in three-dimensional Einstein gravity with and without a cosmological constant. Taking the exterior and interior metrics to be those of stationary metrics with asymptotically constant curvature, we solve the equations of motion for the shells from the Darmois-Israel junction conditions in the "co-rotating" frame. We study various collapse scenarios with "arbitrary" angular momentum for a variety of geometric configurations, including anti-de Sitter, de Sitter, and flat spaces. We find that the collapsing shells can form a BTZ black hole, a three-dimensional Kerr-dS spacetime, and an horizonless geometry of point masses under certain initial conditions. For pressureless dust shells, the curvature singularity is "not" formed due to the angular momentum barrier near the origin. However when the shell pressure is nonvanishing,…
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