Sufficient conditions are given for a unique outer horizon to cloak a negative-mass Schwarzschild timelike naked singularity when non-negative localized anisotropic matter is added.
In this sense, horizon formation emerges from a competition between the negative bare core and the cu- mulative growth of the exterior matter layer
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Classical Dressing of Timelike Naked Singularities
Sufficient conditions are given for a unique outer horizon to cloak a negative-mass Schwarzschild timelike naked singularity when non-negative localized anisotropic matter is added.