Interactions of cosmic neutrinos with nucleons in the RS model

Abstract

We consider the scattering of the brane fields due to t-channel massive graviton exchanges in the Randall-Sundrum model. The eikonal amplitude is analytically calculated and both differential and total neutrino-nucleon cross sections are estimated. The event rate of quasi-horizontal air showers induced by cosmic neutrinos, which can be detected at the Pierre Auger Observatory, is presented for two different fluxes of cosmogenic neutrinos.

23 pages, LaTeX2e, 11 eps figures

References in corpus (1)

• The Impact of Heavy Nuclei on the Cosmogenic Neutrino Flux

Cited by in corpus (9)

• The Jem-Euso Mission
• Exotic Neutrino Interactions at the Pierre Auger Observatory
• LHC bounds on large extra dimensions
• RS model with a small curvature and two-photon production at the LHC
• Virtual gravitons and brane field scattering in the RS model with a small curvature
• 5-dimensional Quantum Gravity Effects in Exclusive Double Diffractive Events
• Probe of the Randall-Sundrum-like model with the small curvature via light-by-light scattering at the LHC
• Probing Quantum Gravity with Elastic Interactions of Ultra-High-Energy Neutrinos
• RS model with a small curvature and gravity effects in e+e- annihilation into leptons at the LC