Toward Radio Detection of PeV Neutrinos on the Cubic Kilometer Scale

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dc.creatorFrichter, George M.
dc.creatorRalston, John P.
dc.creatorMcKay, Douglas W.
dc.date1996-06-03
dc.date.accessioned2026-07-07T02:21:19Z
dc.date.available2026-07-07T02:21:19Z
dc.descriptionInteractions of ultrahigh energy neutrinos of cosmological origin in large volumes of radio-transparent South Polar ice can be detected via coherent Cherenkov emission from accompanying electromagnetic showers. A pilot experiment employing buried radio receivers has been successfully deployed at the South Pole and data are now being collected. The physics of coherent radio emission together with the properties of radio-pulse propagation in Antarctic ice clearly distinguishes the radio method from phototube detection. In the context of the proposed km^3-scale neutrino telescope, these two detection modes provide complementary information on UHE neutrino interactions.
dc.description10 pages, procsla.sty, psfig.sty. Conf. Proc. Seventh International Symposium on Neutrino Telescopes, Feb. 27 - Mar. 1, 1996, Venice, Italy
dc.identifierhttps://arxiv.org/abs/astro-ph/9606008
dc.identifierhttp://arxiv.org/abs/astro-ph/9606008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10506
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleToward Radio Detection of PeV Neutrinos on the Cubic Kilometer Scale
dc.typetext

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