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Atmospheric and astrophysical neutrinos above 1 TeV interacting in IceCube
Vise andre og tillknytning
2015 (engelsk)Inngår i: Physical Review D, ISSN 1550-7998, E-ISSN 1550-2368, Vol. 91, nr 2, s. 022001-Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

The IceCube Neutrino Observatory was designed primarily to search for high-energy (TeV-PeV) neutLrinos produced in distant astrophysical objects. A search for. greater than or similar to 100 TeV neutrinos interacting inside the instrumented volume has recently provided evidence for an isotropic flux of such neutrinos. At lower energies, IceCube collects large numbers of neutrinos from the weak decays of mesons in cosmic-ray air showers. Here we present the results of a search for neutrino interactions inside IceCube's instrumented volume between 1 TeV and 1 PeV in 641 days of data taken from 2010-2012, lowering the energy threshold for neutrinos from the southern sky below 10 TeV for the first time, far below the threshold of the previous high-energy analysis. Astrophysical neutrinos remain the dominant component in the southern sky down to a deposited energy of 10 TeV. From these data we derive new constraints on the diffuse astrophysical neutrino spectrum, Phi(v) = 2.06(-0.3)(+0.4) x 10(-18) (E-v = 10(5) GeV)-2.46 +/- 0.12GeV-1 cm(-2) sr(-1) s(-1) for 25 TeV < E-v < 1.4 PeV, as well as the strongest upper limit yet on the flux of neutrinos from charmed-meson decay in the atmosphere, 1.52 times the benchmark theoretical prediction used in previous IceCube results at 90% confidence.

sted, utgiver, år, opplag, sider
2015. Vol. 91, nr 2, s. 022001-
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Identifikatorer
URN: urn:nbn:se:uu:diva-244487DOI: 10.1103/PhysRevD.91.022001ISI: 000347924700001OAI: oai:DiVA.org:uu-244487DiVA, id: diva2:790317
Tilgjengelig fra: 2015-02-24 Laget: 2015-02-17 Sist oppdatert: 2019-05-21bibliografisk kontrollert

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Boersma, David J.Botner, OlgaEuler, SebastianHallgren, AllanHeros, Carlos Perez de losStröm, RickardTaavola, HenricUnger, Elisabeth
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