Planet-sized Detectors for Ultra-high Energy Neutrinos & Cosmic Rays

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dc.creatorGorham, Peter W.
dc.date2004-11-17
dc.date.accessioned2026-07-07T02:15:54Z
dc.date.available2026-07-07T02:15:54Z
dc.descriptionExtragalactic astronomy with photons ends at ~0.1 PeV, but we know there are astrophysical sources for seven more decades of energy beyond this. To probe the highest energy sources and particles in the universe, new messengers, such as neutrinos, and detectors with planet-sized areas are required. This note provides a glimpse of the possibilities.
dc.description2 pages, 1 figure; white paper submitted for inclusion in the NASA Advanced Planning Office's Capability Roadmap Public Workshop, Nov. 30, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0411510
dc.identifierhttp://arxiv.org/abs/astro-ph/0411510
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8591
dc.subjectAstrophysics
dc.titlePlanet-sized Detectors for Ultra-high Energy Neutrinos & Cosmic Rays
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