We investigate possible signatures of black hole events at the LHC in the
hypothesis that such objects will not evaporate completely, but leave a stable
remnant. For the purpose of defining a reference scenario, we have employed the
publicly available Monte Carlo generator CHARYBDIS2, in which the remnant's
behavior is mostly determined by kinematic constraints and conservation of some
quantum numbers, such as the baryon charge. Our findings show that electrically
neutral remnants are highly favored and a significantly larger amount of
missing transverse momentum is to be expected with respect to the case of
complete decay.Comment: LaTeX, 13 pages, 2 tables, 5 figures, references added and typos
corrected. To appear in EPJ