arXiv · 2412.14358
The impact of the eccentricity on the collapse of an ellipsoid into a black hole
Abstract
We consider the gravitational collapse of a homogeneous pressureless ellipsoid. We have shown that the minimal size $r$ that the ellipsoid can reach during collapse depends on its initial eccentricity $e_0$ as $r\propto e_0^\nu$, where $\nu \approx 15/8$, and this dependence is very universal. We have estimated the parameters (in particular, the initial eccentricity) of a homogeneous pressureless ellipsoid, whereat it collapses directly into a black hole.
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A. G. Nikiforov, A. N. Baushev, M. V. Barkov. 2024-12-18. The impact of the eccentricity on the collapse of an ellipsoid into a black hole. https://doi.org/10.3390/universe11030095
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