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Naked Singularity Censoring with Anisotropic Apparent Horizon

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arxiv 2401.02003 v1 pith:PMAKMZNW submitted 2024-01-03 gr-qc math-phmath.APmath.DGmath.MP

classification gr-qcmath-phmath.APmath.DGmath.MP
keywords anisotropicinitialnakedsingularityapparentapproachchristodouloufield
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abstract

Employing the Einstein-scalar field system, we demonstrate an approach for proving high co-dimensional nonlinear instability of naked-singularity solutions as constructed by Christodoulou in [18]. We further investigate the censorship of Christodoulou's naked singularity and show that a tiny anisotropic perturbation arising from the outgoing characteristic initial data would lead to the emergence of an anisotropic apparent horizon, which covers and censors the naked singularity. Our approach advances the hyperbolic short-pulse method by not requiring the aid of additional large parameters, by permitting the use of initial perturbations for the shear tensor and the derivative of scalar field to be with finite $BV$ and $C^0$ norms, and by allowing the initial perturbation to be arbitrarily small in scale-critical norms. New elliptic arguments based on non-perturbative methods are also developed.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Interior instability of naked singularities of a scalar field

    gr-qc 2025-08 conditional novelty 8.0 of 10

    Nonlinear interior perturbations below a regularity threshold make k-self-similar scalar-field naked singularities collapse into trapped surfaces and black holes.

  2. Scalar perturbations to naked singularities of perfect fluid

    gr-qc 2025-05 conditional novelty 6.0 of 10

    Small scalar-field perturbations make trapped surfaces form before the naked singularity in spherical perfect-fluid collapse, proving these background solutions are unstable.

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