Analytic and exponentially localized braneworld Reissner-Nordström-AdS solution: A top-down approach

In this work, we construct a five-dimensional spherically symmetric, charged and asymptotically anti--de Sitter black hole with its singularity being pointlike strictly localized on our brane. addition, the induced brane geometry is described by Reissner-Nordstr\"om-(A)dS line element. We perform careful classification of horizons, demonstrate that all them are exponentially close to thus exhibiting pancake shape. The bulk gravitational background everywhere regular, reduces an ${\mathrm{AdS}}_{5}$ spacetime right outside event horizon. This supported anisotropic fluid only two independent components, energy density ${\ensuremath{\rho}}_{E}$ tangential pressure ${p}_{2}$. All conditions respected brane, but local violation takes place within horizon regime in bulk. A tensor-vector-scalar field-theory model built attempt realize necessary matter, however, order do so, both gauge scalar degrees freedom need turn phantomlike at boundary. study junction reveals no additional matter needs be introduced for consistent embedding apart from constant, positive tension. finally compute effective equations caused combined effect charge fact tidal charge.