Critical phenomena in gravitational collapse (Physics Reports)
Carsten Gundlach

TL;DR
This paper reviews the critical phenomena observed in gravitational collapse within general relativity, highlighting the universal properties, mathematical analogies to phase transitions, and the rich phenomenology near black hole formation thresholds.
Contribution
It provides a comprehensive overview of critical phenomena in gravitational collapse, including their mathematical understanding, universality, and specific features in general relativity.
Findings
Critical solutions exhibit universality near black hole thresholds.
Black hole mass scales as $(p-p_*)^gamma$ in scale-invariant cases.
Critical phenomena are shown to be generic in gravitational collapse.
Abstract
In general relativity black holes can be formed from regular initial data that do not contain a black hole already. The space of regular initial data for general relativity therefore splits naturally into two halves: data that form a black hole in the evolution and data that do not. The spacetimes that are evolved from initial data near the black hole threshold have many properties that are mathematically analogous to a critical phase transition in statistical mechanics. Solutions near the black hole threshold go through an intermediate attractor, called the critical solution. The critical solution is either time-independent (static) or scale-independent (self-similar). In the latter case, the final black hole mass scales as along any one-parameter family of data with a regular parameter such that is the black hole threshold in that family. The critical…
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