In this work, we study the â€˜scalar channelâ€™ of the emission of Hawking radiation from a (4+n)-dimensional, rotating black hole on the brane. We numerically solve both the radial and angular part ofâ€¦ (More)

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 newâ€¦ (More)

We study in detail the scalar-field Hawking radiation emitted into the bulk by a higher-dimensional, rotating black hole. We numerically compute the angular eigenvalues, and solve the radial equationâ€¦ (More)

Barry Wardell, 2 Chad R. Galley, AnÄ±l ZenginoÄŸlu, Marc Casals, Sam R. Dolan, and Adrian C. Ottewill School of Mathematical Sciences and Complex & Adaptive Systems Laboratory, University Collegeâ€¦ (More)

Linear field perturbations of a black hole are described by the Green function of the wave equation that they obey. After Fourier decomposing the Green function, its two natural contributions areâ€¦ (More)

Recent works have included the effect of rotation on simulations of black hole events at the LHC, showing that the angular momentum of the black hole cannot be ignored and it makes a non-trivialâ€¦ (More)

Field perturbations of a curved background space-time obey a wave equation, for which the retarded Green function is a fundamental object. It is known that the Green function diverges when the twoâ€¦ (More)