Anti-deSitter gravitational collapse
V. Husain, G. Kunstatter, B. Preston, M. Birukou

TL;DR
This paper develops a formalism for analyzing spherically symmetric scalar field collapse in various dimensions and cosmological constants, and uses it to study critical phenomena in four-dimensional anti-de Sitter spacetime.
Contribution
It introduces a general formalism for scalar collapse in arbitrary dimensions and cosmological constants, and applies it to reveal universal critical behavior in AdS space.
Findings
Critical behavior observed at black hole formation threshold
Critical exponent is independent of the cosmological constant
Formalism applicable to various spacetime dimensions
Abstract
We describe a formalism for studying spherically symmetric collapse of the massless scalar field in any spacetime dimension, and for any value of the cosmological constant . The formalism is used for numerical simulations of gravitational collapse in four spacetime dimensions with negative . We observe critical behaviour at the onset of black hole formation, and find that the critical exponent is independent of .
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