Convergence to a self-similar solution in general relativistic gravitational collapse
Tomohiro Harada, Hideki Maeda

TL;DR
This paper demonstrates that in spherical gravitational collapse of a perfect fluid with specific equations of state, solutions tend to a self-similar form near singularities, providing insights into cosmic censorship and critical phenomena.
Contribution
It shows that generic collapse converges to a known self-similar solution, with implications for cosmic censorship and critical phenomena in gravitational collapse.
Findings
Collapse converges to the Larson-Penston self-similar solution near singularities.
Naked singularities can form, challenging cosmic censorship.
Critical phenomena with a specific exponent are predicted in Newtonian collapse.
Abstract
We study the spherical collapse of a perfect fluid with an equation of state by full general relativistic numerical simulations. For , it has been known that there exists a general relativistic counterpart of the Larson-Penston self-similar Newtonian solution. The numerical simulations strongly suggest that, in the neighborhood of the center, generic collapse converges to this solution in an approach to a singularity and that self-similar solutions other than this solution, including a ``critical solution'' in the black hole critical behavior, are relevant only when the parameters which parametrize initial data are fine-tuned. This result is supported by a mode analysis on the pertinent self-similar solutions. Since a naked singularity forms in the general relativistic Larson-Penston solution for , this will be the most serious known…
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