0000000000218847

AUTHOR

A. Cuoco

showing 2 related works from this author

Disentangling neutrino-nucleon cross section and high energy neutrino flux with akm3neutrino telescope

2007

The energy--zenith angular event distribution in a neutrino telescope provides a unique tool to determine at the same time the neutrino-nucleon cross section at extreme kinematical regions, and the high energy neutrino flux. By using a simple parametrization for fluxes and cross sections, we present a sensitivity analysis for the case of a km^3 neutrino telescope. In particular, we consider the specific case of an under-water Mediterranean telescope placed at the NEMO site, although most of our results also apply to an under-ice detector such as IceCube. We determine the sensitivity to departures from standard values of the cross sections above 1 PeV which can be probed independently from a…

AstrofísicaPhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesCosmic raySolar neutrino problemAstrophysicslaw.inventionTelescopeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorlawMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationPhysical Review D
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Do observations prove that cosmological neutrinos are thermally distributed?

2005

It is usually assumed that relic neutrinos possess a Fermi-Dirac distribution, acquired during thermal equilibrium in the Early Universe. However, various mechanisms could introduce strong distortions in this distribution. We perform a Bayesian likelihood analysis including the first moments of the three active neutrino distributions as free parameters, and show that current cosmological observations of light element abundances, Cosmic Microwave Background (CMB) anisotropies and Large Scale Structures (LSS) are compatible with very large deviations from the standard picture. We also calculate the bounds on non-thermal distortions which can be expected from future observations, and stress th…

PhysicsNuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectCosmic microwave backgroundDark matterAstrophysics (astro-ph)FOS: Physical sciencesFísicaAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsUniverseCosmologyCosmic neutrino backgroundHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesisNucleosynthesisNeutrinomedia_common
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