Small Black Holes on Branes: Is the horizon regular or singular ?
D. Karasik, C. Sahabandu, P. Suranyi, L. C. R. Wijewardhana

TL;DR
This paper examines whether small black holes on branes in the Randall-Sundrum model have regular horizons or naked singularities, using perturbative expansions and weak field approximations.
Contribution
It demonstrates that first-order solutions suggest a singular horizon, while a regular horizon solution involves half-integer powers in the mass expansion.
Findings
First-order weak field solution indicates a singular horizon.
A regular horizon solution involves half-integer powers of mass.
Perturbative approach reveals the nature of the horizon in brane black holes.
Abstract
We investigate the following question: Consider a small mass, with (the ratio of the Schwarzschild radius and the bulk curvature length) much smaller than 1, that is confined to the TeV brane in the Randall-Sundrum I scenario. Does it form a black hole with a regular horizon, or a naked singularity? The metric is expanded in and the asymptotic form of the metric is given by the weak field approximation (linear in the mass). In first order of we show that the iteration of the weak field solution, which includes only integer powers of the mass, leads to a solution that has a singular horizon. We find a solution with a regular horizon but its asymptotic expansion in the mass also contains half integer powers.
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