Brane-world stars and (microscopic) black holes

• DOI: 10.1016/j.physletb.2012.07.041
• Publication Date: 2012-07-20T17:15:34Z
• Authors: R. Casadio; J. Ovalle
• Keywords: Black hole (networking); Semiclassical physics

We study stars in the brane-world by employing principle of minimal geometric deformation and find that black hole metrics with a tidal charge are consistently recovered suitable limit. This procedure allows us to determine as function ADM mass (and brane tension). A minimum for semiclassical microscopic holes can then be derived, relevant impact description events at LHC.