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High-energy neutrino astronomy: detection methods and first achievements

B. Baret 1 V. van Elewyck 2
1 APC - AHE - APC - Astrophysique des Hautes Energies
APC (UMR_7164) - AstroParticule et Cosmologie, Dipartimento di Astronomia, Universita degli Studi di Bologna
Abstract : In the last century, astronomy evolved from optical observation to the multi-wavelength study of celestial objects from radio waves up to x- and γ-rays, leading to a wealth of new discoveries and opening the way to high-energy astroparticle physics. In particular, the recent success of ground-based very-high-energy γ-ray telescopes has opened a new window on the most powerful and violent objects of the Universe, giving a new insight into the physical processes at work in such sources. In the context of high-energy astronomy, neutrinos constitute a unique probe since they escape from their sources, travel undisturbed on virtually cosmological distances and are produced in high-energy hadronic processes. In particular they would allow a direct detection and unambiguous identification of the sites of acceleration of high-energy baryonic cosmic rays, which remain unknown. This report discusses the physics potential of the domain and reviews the experimental techniques relevant for the detection of high-energy (>=TeV) neutrinos. The results obtained by the first generation of such detectors are presented, along with the perspectives opened by new projects and prototypes being currently developed.
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Contributor : Bruny Baret <>
Submitted on : Tuesday, June 19, 2012 - 2:46:24 PM
Last modification on : Friday, October 30, 2020 - 12:04:02 PM

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B. Baret, V. van Elewyck. High-energy neutrino astronomy: detection methods and first achievements. Reports on Progress in Physics, IOP Publishing, 2011, 74, pp.046902. ⟨10.1088/0034-4885/74/4/046902⟩. ⟨in2p3-00709798⟩



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