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Neutrino Telescopes
High Energy Astrophysical Phenomena · Submitted 3 Jan 2011
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Several neutrino telescopes of different sizes and capabilities are presently taking data and projects to further increase their size and sensitivity are underway.In this contribution we review the present status of neutrino telescopes based on the cherenkov ligh detection technique, their recent results and the plans to increase their sensitivity.
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The abstract, sentence by sentence
The observation of high energy cosmic neutrinos can shed light on the astrophysical sites and mechanisms involved in the acceleration of protons and nuclei to the high energies observed at Earth by cosmic ray detectors. More generally, high energy neutrinos can be a key instrument in the multimessenger study of the high energy sky. Several neutrino telescopes of different sizes and capabilities are presently taking data and projects to further increase their size and sensitivity are underway.In this contribution we review the present status of neutrino telescopes based on the cherenkov ligh detection technique, their recent results and the plans to increase their sensitivity.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | The observation of high energy cosmic neutrinos can shed light on the astrophysical sites and mechanisms involved in the acceleration of protons and nuclei to the high energies observed at Earth by cosmic ray detectors. | background 1.00 | 0.04 | 0.10 | hedged possibility 0.93 |
| s1 | More generally, high energy neutrinos can be a key instrument in the multimessenger study of the high energy sky. | background 0.99 | 0.04 | 0.08 | hedged possibility 0.58 |
| s2 | Several neutrino telescopes of different sizes and capabilities are presently taking data and projects to further increase their size and sensitivity are underway.In this contribution we review the present status of neutrino telescopes based on the cherenkov ligh detection technique, their recent results and the plans to increase their sensitivity. | contribution 0.98 | 0.17 | 0.15 | asserted 0.98 |
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The paper
Original abstract
The observation of high energy cosmic neutrinos can shed light on the astrophysical sites and mechanisms involved in the acceleration of protons and nuclei to the high energies observed at Earth by cosmic ray detectors. More generally, high energy neutrinos can be a key instrument in the multimessenger study of the high energy sky. Several neutrino telescopes of different sizes and capabilities are presently taking data and projects to further increase their size and sensitivity are underway.In this contribution we review the present status of neutrino telescopes based on the cherenkov ligh detection technique, their recent results and the plans to increase their sensitivity.
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What this paper does with the arXiv papers it cites
What it cites · 3 sentences without a confident label
Uses data or values from 2 papers
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The most stringent upper limit provided by NT200 for a diffuse astrophysical flux of $ν_e + ν_μ + ν_τ$ assuming an E$^-2$ spectrum is E$^2 Φ$=2.9 $×$10$^-7$ GeV cm$^-2$ s$^-1$ in the 20 TeV to 20 PeV energy range [ref] .
Search for a diffuse flux of high-energy neutrinos with the Baikal neutrino telescope NT200 · Neutrino telescopes in lake and sea water · 0.99
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The open blue squares in figure [ref] show the 90% C.L. upper limit for a candidate list of selected sources [ref] .
Search for neutrino point sources with the IceCube Neutrino Observatory · IceCube · 0.91
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