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

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

2004-11-17

arxiv.org/abs/astro-ph/0411510v1

Astronomy and Astrophysics

Astrophysics

2 pages, 1 figure; white paper submitted for inclusion in the NASA Advanced Planning Office's Capability Roadmap Public Worksh

Scientific paper

Extragalactic 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.

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