Phenomenology of Production and Decay of Spinning Extra-Dimensional Black Holes at Hadron Colliders
James A. Frost, Jonathan R. Gaunt, Marco O.P. Sampaio, Marc Casals,, Sam R. Dolan, M. Andrew Parker, and Bryan R. Webber

TL;DR
This paper introduces CHARYBDIS2, a Monte Carlo simulation tool for modeling the production and decay of spinning black holes in theories with extra dimensions at hadron colliders, emphasizing spin effects and decay dynamics.
Contribution
It provides a comprehensive simulation including spin-down phases, angular momentum loss, and decay termination options, advancing the modeling of black hole phenomenology in collider experiments.
Findings
Enhanced modeling of black hole spin effects
Feasibility analysis of observing spinning black holes
Improved decay and production process simulations
Abstract
We present results of CHARYBDIS2, a new Monte Carlo simulation of black hole production and decay at hadron colliders in theories with large extra dimensions and TeV-scale gravity. The main new feature of CHARYBDIS2 is a full treatment of the spin-down phase of the decay process using the angular and energy distributions of the associated Hawking radiation. Also included are improved modelling of the loss of angular momentum and energy in the production process as well as a wider range of options for the Planck-scale termination of the decay. The new features allow us to study the effects of black hole spin and the feasibility of its observation in such theories.
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