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Energy reconstruction methods in the IceCube neutrino telescope
Stockholms universitet, Naturvetenskapliga fakulteten, Fysikum. (Systemfysik)
Stockholms universitet, Naturvetenskapliga fakulteten, Fysikum. Stockholms universitet, Naturvetenskapliga fakulteten, Oskar Klein-centrum för kosmopartikelfysik (OKC).
Stockholms universitet, Naturvetenskapliga fakulteten, Fysikum. Stockholms universitet, Naturvetenskapliga fakulteten, Oskar Klein-centrum för kosmopartikelfysik (OKC).
Stockholms universitet, Naturvetenskapliga fakulteten, Fysikum. Stockholms universitet, Naturvetenskapliga fakulteten, Oskar Klein-centrum för kosmopartikelfysik (OKC).
Vise andre og tillknytning
2014 (engelsk)Inngår i: Journal of Instrumentation, ISSN 1748-0221, E-ISSN 1748-0221, Vol. 9, s. P03009-Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

Accurate measurement of neutrino energies is essential to many of the scientific goals of large-volume neutrino telescopes. The fundamental observable in such detectors is the Cherenkov light produced by the transit through a medium of charged particles created in neutrino interactions. The amount of light emitted is proportional to the deposited energy, which is approximately equal to the neutrino energy for v(e) and v(mu) charged-current interactions and can be used to set a lower bound on neutrino energies and to measure neutrino spectra statistically in other channels. Here we describe methods and performance of reconstructing charged-particle energies and topologies from the observed Cherenkov light yield, including techniques to measure the energies of uncontained muon tracks, achieving average uncertainties in electromagnetic-equivalent deposited energy of similar to 15% above 10 TeV.

sted, utgiver, år, opplag, sider
2014. Vol. 9, s. P03009-
Emneord [en]
Cherenkov detectors, dE/dx detectors, Neutrino detectors, Performance of High Energy Physics Detectors
HSV kategori
Identifikatorer
URN: urn:nbn:se:su:diva-105251DOI: 10.1088/1748-0221/9/03/P03009ISI: 000336123200069OAI: oai:DiVA.org:su-105251DiVA, id: diva2:729117
Merknad

AuthorCount:287;

Tilgjengelig fra: 2014-06-25 Laget: 2014-06-24 Sist oppdatert: 2017-12-05bibliografisk kontrollert

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Bohm, ChristianDanninger, MatthiasFinley, ChadFlis, SamuelHulth, Per-OlofHultqvist, KlasWalck, ChristianWolf, MartinZoll, Marcel
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