We study stars in the brane-world by employing the principle of minimal geometric deformation and find that brane-world black hole metrics with a tidal charge can be consistently recovered in a suitable limit. This procedure allows us to determine the tidal charge as a function of the ADM mass of the black hole (and brane tension). A minimum mass for semiclassical microscopic black holes can then be derived, with a relevant impact for the description of black hole events at the LHC. © 2012 Elsevier B.V.
CITATION STYLE
Casadio, R., & Ovalle, J. (2012). Brane-world stars and (microscopic) black holes. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 715(1–3), 251–255. https://doi.org/10.1016/j.physletb.2012.07.041
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