Models of Black Hole Production at LHC

Abstract

The purpose of this paper is to discuss about the different models for black hole production at the future Large Hadron Collider. In traditional scenarios the Planck scale is fundamental, and the weak scale is derived from it via some dynamical mechanism. Recently, several authors are exploring an alternative viewpoint where the weak scale is the fundamental scale of nature and the 4‐dimensional Planck scale is to be derived from that [1]. These scenarios include large or warped extra dimensions, propagation of matter and gauge degrees of freedom on brane worlds, and a fundamental Planck scale of O(TeV). If the scale of quantum gravity is near TeV we will have a copious production of mini black holes at the Large Hadron Collider [2] and Cosmic rays interactions in the atmosphere [3]. We discussed as well other line of semi‐classical models from analog gravity in nonlinear electrodynamics that can be tested as well at LHC. The possibles consequences of these models for high energy experimental physics are discussed.