Interactions of cosmic neutrinos with nucleons in the RS model

2004/12/24 by A. V. Kisselev · 1 citation
Physics and Astronomy · #Astronomy #Astrophysics #Black Holes and Theoretical Physics #COSMIC cancer database #Cosmic neutrino background #Cosmic ray #Cosmology and Gravitation Theories #Neutrino #Neutrino detector #Neutrino oscillation #Nuclear physics #Nucleon #Particle physics #Particle physics theoretical and experimental studies #Physics #astro-ph #hep-ph

paper · pdf · doi:10.1140/epjc/s2005-02284-y

published as Eur.Phys.J.C42:217-225,2005 · 23 pages, LaTeX2e, 11 eps figures

arxiv created 2004/12/24 · openalex publication_date 2005/06/07 · arxiv updated 2011/09/13 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

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.

Citations

• Kaluza-Klein states from large extra dimensions
• Gravireggeons in extra dimensionsand interaction of ultra-high energy cosmic neutrinos with nucleons
• Large Mass Hierarchy from a Small Extra Dimension
• An Alternative to Compactification
• High energy astrophysical neutrinos: The upper bound is robust

Cited by

• Exotic neutrino interactions at the Pierre Auger Observatory