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      Neutrino Interactions at Ultrahigh Energies

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          Abstract

          We report new calculations of the cross sections for deeply inelastic neutrino-nucleon scattering at neutrino energies between \(10^{9}\ev\) and \(10^{21}\ev\). We compare with results in the literature and assess the reliability of our predictions. For completeness, we briefly review the cross sections for neutrino interactions with atomic electrons, emphasizing the role of the \(W\)-boson resonance in \(\bar{\nu}_{e}e\) interactions for neutrino energies in the neighborhood of \(6.3\pev\). Adopting model predictions for extraterrestrial neutrino fluxes from active galactic nuclei, gamma-ray bursters, and the collapse of topological defects, we estimate event rates in large-volume water \v{C}erenkov detectors and large-area ground arrays.

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          Interactions of Ultrahigh-Energy Neutrinos

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            Progress and Prospects in Neutrino Astrophysics

            The neutrino deficits observed in four solar neutrino experiments, relative to the theoretical predictions, have led to fresh insights into neutrino and solar physics. Neutrino emission from distant, energetic astronomical systems may form the basis for a new field of astronomy. Additional experiments are needed to test explanations of the solar neutrino deficits and to allow the detection of more distant sources.
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              Author and article information

              Journal
              06 July 1998
              Article
              10.1103/PhysRevD.58.093009
              hep-ph/9807264
              a20d4d6a-ff2c-4185-b0c5-ec542f06d674
              History
              Custom metadata
              FERMILAB-PUB-98/087-T
              Phys.Rev.D58:093009,1998
              32 pages, 11 figures, uses RevTeX and boxedeps
              hep-ph astro-ph

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