Static spherically symmetric scalar-field spacetimes with small scalar charge are linearly unstable to radial perturbations, giving numerical support for cosmic censorship in this class.
The choice n = 3, 4, 5 in (13) ensures the Coulomb asymptotic behavior of the field at spatial infinity
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Penrose hypothesis and instability of naked singularities in static spherically symmetric systems with scalar fields
Static spherically symmetric scalar-field spacetimes with small scalar charge are linearly unstable to radial perturbations, giving numerical support for cosmic censorship in this class.