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In this work, we construct a five-dimensional spherically-symmetric, chargedand asymptotically Anti-de Sitter black hole with its singularity beingpoint-like and strictly localised on our brane. In addition, the induced branegeometry is described by a Reissner-Nordstr\"{o}m-(A)dS line-element. Weperform a careful classification of the horizons, and demonstrate that all ofthem are exponentially localised close to the brane thus exhibiting a pancakeshape. The bulk gravitational background is everywhere regular, and reduces toan AdS$_5$ spacetime right outside the black-hole event horizon. This geometryis supported by an anisotropic fluid with only two independent components, theenergy density $\rho_E$ and tangential pressure $p_2$. All energy conditionsare respected close to and on our brane, but a local violation takes placewithin the event horizon regime in the bulk. A tensor-vector-scalarfield-theory model is built in an attempt to realise the necessary bulk matter,however, in order to do so, both gauge and scalar degrees of freedom need toturn phantom-like at the bulk boundary. The study of the junction conditionsreveals that no additional matter needs to be introduced on the brane for itsconsistent embedding in the bulk geometry apart from its constant, positivetension. We finally compute the effective gravitational equations on the brane,and demonstrate that the Reissner-Nordstr\"{o}m-(A)dS geometry on our brane iscaused by the combined effect of the five-dimensional geometry and bulk matterwith its charge being in fact a tidal charge.

Analytic and exponentially localized brane-world Reissner-Nordstr\"{o}m-AdS solution: a top-down approach