UNIGE document Scientific Article
previous document  unige:114702  next document
add to browser collection

Measurements using the inelasticity distribution of multi-TeV neutrino interactions in IceCube

CollaborationWith : Al Samarai, Imen / Barbano, Anastasia / Bron, Stéphanie / Carver, Tessa / Montaruli, Teresa
Published in Physical review. D. Particles and fields. 2019, vol. 99, no. 3
Collection Open Access - SCOAP3
Abstract Inelasticity, the fraction of a neutrino's energy transferred to hadrons, is a quantity of interest in the study of astrophysical and atmospheric neutrino interactions at multi-TeV energies with IceCube. In this work, a sample of contained neutrino interactions in IceCube is obtained from five years of data and classified as 2650 tracks and 965 cascades. Tracks arise predominantly from charged-current νμ interactions, and we demonstrate that we can reconstruct their energy and inelasticity. The inelasticity distribution is found to be consistent with the calculation of Cooper-Sarkar et al. across the energy range from ∼1 to ∼100 TeV. Along with cascades from neutrinos of all flavors, we also perform a fit over the energy, zenith angle, and inelasticity distribution to characterize the flux of astrophysical and atmospheric neutrinos. The energy spectrum of diffuse astrophysical neutrinos is described well by a power law in both track and cascade samples, and a best-fit index γ=2.62±0.07 is found in the energy range from 3.5 TeV to 2.6 PeV. Limits are set on the astrophysical flavor composition and are compatible with a ratio of (<mfrac>13</mfrac>∶<mfrac>13</mfrac>∶<mfrac>13</mfrac>)⊕. Exploiting the distinct inelasticity distribution of νμ and ν¯μ interactions, the atmospheric νμ to ν¯μ flux ratio in the energy range from 770 GeV to 21 TeV is found to be 0.77−0.25+0.44 times the calculation by Honda et al. Lastly, the inelasticity distribution is also sensitive to neutrino charged-current charm production. The data are consistent with a leading-order calculation, with zero charm production excluded at 91% confidence level. Future analyses of inelasticity distributions may probe new physics that affects neutrino interactions both in and beyond the Standard Model.
arXiv: 1808.07629
Full text
(ISO format)
ICECUBE COLLABORATION. Measurements using the inelasticity distribution of multi-TeV neutrino interactions in IceCube. In: Physical Review. D, 2019, vol. 99, n° 3. doi: 10.1103/PhysRevD.99.032004 https://archive-ouverte.unige.ch/unige:114702

275 hits



Deposited on : 2019-03-04

Export document
Format :
Citation style :