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RESEARCH PRODUCT
Ultrahigh-energy neutrino flux as a probe of large extra dimensions
Olga MenaSoebur RazzaqueJoseph D. Lykkensubject
High Energy Physics - TheoryAstrofísicaParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxCosmic rayAstrophysics01 natural sciences7. Clean energyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesUltrahigh energy010306 general physicsPhysicsAnnihilation010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysics3. Good healthHigh Energy Physics - PhenomenologySupernovaExtra dimensionsHigh Energy Physics - Theory (hep-th)13. Climate actionLarge extra dimensionHigh Energy Physics::ExperimentNeutrinodescription
A suppression in the spectrum of ultrahigh-energy (UHE, >= 10^{18} eV) neutrinos will be present in extra-dimensional scenarios, due to enhanced neutrino-antineutrino annihilation processes with the supernova relic neutrinos. In the n>4 scenario, being n the number of extra dimensions, neutrinos can not be responsible for the highest energy events observed in the UHE cosmic ray spectrum. A direct implication of these extra-dimensional interactions would be the absence of UHE neutrinos in ongoing and future neutrino telescopes.
year | journal | country | edition | language |
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2007-05-14 | Journal of Cosmology and Astroparticle Physics |