Late-Time Evolution of Charged Gravitational Collapse and Decay of Charged Scalar Hair - III. Nonlinear Analysis
Shahar Hod, Tsvi Piran

TL;DR
This paper investigates the nonlinear evolution of charged scalar fields during gravitational collapse, confirming decay patterns and mass-inflation phenomena, and validating analytical predictions about charged hair decay rates.
Contribution
It provides the first nonlinear analysis confirming decay rates of charged scalar hair and the occurrence of mass-inflation in charged black holes, supporting previous analytical conjectures.
Findings
Oscillatory inverse power-law tails confirmed
Decay of charged hair is slower than neutral
Mass-inflation occurs along the Cauchy horizon
Abstract
We study the nonlinear gravitational collapse of a charged massless scalar-field. We confirm the existence of oscillatory inverse power-law tails along future timelike infinity, future null infinity and along the future outer-horizon. The nonlinear dumping exponents are in excellent agreement with the analytically predicted ones. Our results prove the analytic conjecture according to which a charged hair decays slower than a neutral one and also suggest the occurrence of mass-inflation along the Cauchy horizon of a dynamically formed charged black-hole.
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