Black holes at future colliders and beyond

One of the most dramatic consequences of low-scale (∼ 1 TeV) quantum gravity in models with large or warped extra dimension(s) is copious production of mini black holes at future colliders and in ultra-high-energy cosmic ray collisions. Hawking radiation of these black holes is expected to be constrained mainly to our three-dimensional world and results in rich phenomenology. In this topical review we discuss the current status of astrophysical observations of black holes and selected aspects of mini black hole phenomenology, such as production at colliders and in cosmic rays, black hole decay properties, Hawking radiation as a sensitive probe of the dimensionality of extra space, as well as an exciting possibility of finding new physics in the decays of black holes. PACS numbers: 04.50.+h, 04.70.Dy, 11.10.Kk, 13.85.Qk, 13.85.Rm, 14.80.-j Submitted to: Institute of Physics Publishing J. Phys. G: Nucl. Phys. Black holes at future colliders and beyond 2