Collider Signals of Gravitational Fixed Points
arXiv:0707.3182 · doi:10.1088/1126-6708/2007/12/009
Abstract
Recent studies have shown that the poor perturbative behavior of General Relativity in the ultraviolet regime may be ameliorated by the existence of a non-Gaussian fixed point which renders the theory asymptotically safe and possibly non-perturbatively renormalizable. This results in a running of the (effective) gravitational coupling such that gravity becomes weaker at high energies. We parameterize this effective coupling with a form factor and study its consequences at the LHC and ILC in models with large extra dimensions or warped extra dimensions. We find significant effects in the processes of Kaluza-Klein (KK) graviton exchange or resonant KK graviton production in both the Drell-Yan reaction as well as in . On the otherhand, processes leading to KK graviton emission show qualitatively less sensitivity to the presence of a form factor. In addition, we examine tree-level perturbative unitarity in gravity-mediated scattering and find that this form factor produces a far better behaved amplitude at large center of mass energies.
33 pages
References in corpus (6)
- Tests of the Gravitational Inverse-Square Law below the Dark-Energy Length Scale
- Particle Physics Implications of a Recent Test of the Gravitational Inverse Square Law
- Non-Local Modification of Gravity and the Cosmological Constant Problem
- Newtonian limit of Extended Theories of Gravity
- Quantum Gravity Through Non-Perturbative Renormalization Group and Improved Black Hole
- A Stringy Composite Graviton and the Cosmological Constant Problem