Black hole and brane production in TeV gravity: A review
Marco Cavaglia
TL;DR
This review synthesizes the theoretical framework and phenomenology of black hole and brane production in TeV-scale gravity with large extra dimensions, spanning string/M-theory compactifications and warped geometries. It analyzes semiclassical BH and brane production cross sections, decay channels, and potential collider and ultra-high-energy cosmic ray signatures, while cataloging current collider and astrophysical constraints. The work highlights scenarios where brane production can compete with or dominate BH formation, such as asymmetric compactifications, fat branes, and warped models, and discusses cosmological implications of brane relics and early-universe brane gas. Despite substantial progress, the authors emphasize theoretical uncertainties in brane dynamics and call for deeper studies of brane formation, decay, and distinctive experimental signatures to distinguish BHs from branes at high energies.
Abstract
In models with large extra dimensions particle collisions with center-of-mass energy larger than the fundamental gravitational scale can generate non-perturbative gravitational objects such as black holes and branes. The formation and the subsequent decay of these super-Planckian objects would be detectable in particle colliders and high energy cosmic ray detectors, and have interesting implications in cosmology and astrophysics. In this paper we present a review of black hole and brane production in TeV-scale gravity.
