1201.6145 (R. Casadio et al.)
R. Casadio, J. Ovalle
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 are consistently recovered in a suitable limit. This procedure allows us
to determine the tidal charge as a function of the black hole ADM mass (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.
View original:
http://arxiv.org/abs/1201.6145
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