Classical ultra-relativistic scattering in ADD
arXiv:0903.3019 · doi:10.1088/1126-6708/2009/05/074
Abstract
The classical differential cross-section is calculated for high-energy small-angle gravitational scattering in the factorizable model with toroidal extra dimensions. The three main features of the classical computation are: (a) It involves summation over the infinite Kaluza-Klein towers but, contrary to the Born amplitude, it is finite with no need of an ultraviolet cutoff. (b) It is shown to correspond to the non-perturbative saddle-point approximation of the eikonal amplitude, obtained by the summation of an infinite number of ladder graphs of the quantum theory. (c) In the absence of extra dimensions it reproduces all previously known results.
12 pages, minor changes
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- Physics searches at the LHC
- Transplanckian bremsstrahlung and black hole production
- Gravitational bremsstrahlung in ultra-planckian collisions
- Classical ultrarelativistic bremsstrahlung in extra dimensions
- Scalar Bremsstrahlung in Gravity-Mediated Ultrarelativistic Collisions
- Vector Bremsstrahlung by Ultrarelativistic Collisions in Higher Dimensions