A Kolmogorov-Zakharov Spectrum in $AdS$ Gravitational Collapse
H. P. de Oliveira, Leopoldo A. Pando Zayas, E. L. Rodrigues

TL;DR
This paper demonstrates that gravitational collapse in asymptotically AdS spacetimes exhibits turbulence characterized by a Kolmogorov-Zakharov spectrum, revealing universal features of black hole formation.
Contribution
It provides the first evidence of turbulence and a Kolmogorov-Zakharov spectrum in spherically symmetric AdS gravitational collapse.
Findings
Power spectrum of Ricci scalar follows a ^{-s} law with sb1 0.1
Turbulent regime emerges after initial nonlinear evolution
Universal spectral behavior observed in 4 and 5 dimensions
Abstract
We study black hole formation during the gravitational collapse of a massless scalar field in asymptotically spacetimes for . We conclude that spherically symmetric gravitational collapse in asymptotically spaces is turbulent and characterized by a Kolmogorov-Zakharov spectrum. Namely, we find that after an initial period of weakly nonlinear evolution, there is a regime where the power spectrum of the Ricci scalar evolves as with the frequency, , and .
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