Singularities and self-similarity in gravitational collapse
Tomohiro Harada

TL;DR
This paper explores the role of singularities and self-similar solutions in gravitational collapse, highlighting their significance in understanding cosmic censorship violations and critical phenomena through numerical and theoretical analysis.
Contribution
It provides a unified framework linking self-similar solutions to attractors in gravitational collapse, advancing understanding of singularities and critical phenomena.
Findings
Self-similar solutions act as attractors in gravitational collapse.
Critical phenomena are related to intermediate self-similar behaviour.
Unified view of convergence and critical phenomena via renormalisation group flow.
Abstract
Einstein's field equations in general relativity admit a variety of solutions with spacetime singularities. Numerical relativity has recently revealed the properties of somewhat generic spacetime singularities. It has been found that in a variety of systems self-similar solutions can describe asymptotic or intermediate behaviour of more general solutions in an approach to singularities. The typical example is the convergence to an attractor self-similar solution in gravitational collapse. This is closely related to the cosmic censorship violation in the spherically symmetric collapse of a perfect fluid. The self-similar solution also plays an important role in critical phenomena in gravitational collapse. The critical phenomena are understood as the intermediate behaviour around a critical self-similar solution. We see that the convergence and critical phenomena are understood in a…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory
