Particle Physics with High Energy Neutrinos

Details Particle Physics with High Energy Neutrinos Particle Physics with High Energy Neutrinos

1994-10-26

arxiv.org/abs/hep-ph/9410384v1

Phys.Rept.258:173-236,1995; ERRATUM-ibid.271:355-356,1996

Physics

High Energy Physics

High Energy Physics - Phenomenology

To be published by Physics Reports. Latex file, 66 pages. One large "uufiled" postscript file containing 18 figures included.

Scientific paper

10.1016/0370-1573(95)00003-Y

The topic of this review is the particle astrophysics of high energy neutrinos. High energy is defined as $E_{\nu} > 100$~MeV. Main topics include: -- atmospheric neutrinos and muons from $\pi$, $K$ and charm decay. They probe uncharted territory in neutrino oscillations and constitute both the background and calibration of high energy neutrino telescopes, -- sources of high energy neutrino beams: the galactic plane, the sun, X-ray binaries, supernova remnants and interactions of extra-galactic cosmic rays with background photons, -- an extensive review of the mechanisms by which active galaxies may produce high energy particle beams, -- high energy neutrino signatures of cold dark matter and, -- a brief review of detection techniques (water and ice Cherenkov detectors, surface detectors, radio- and acoustic detectors, horizontal airshower arrays) and the instruments under construction.

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