- Aartsen, MG
- Hill, GC
- Kyriacou, A
- Robertson, S
- Wallace, A
- Whelan, BJ
- Ackermann, M
- Bernardini, E
- Blot, S
- Bradascio, F
- Bretz, HP
- Brostean-Kaiser, J
- Franckowiak, A
- Jacobi, E
- Karg, T
- Kintscher, T
- Kunwar, S
- Nahnhauer, R
- Satalecka, K
- Spiering, C
- Stachurska, J
- Stasik, A
- Strotjohann, NL
- Terliuk, A
- Usner, M
- Van Santen, J
- Adams, J
- Bagherpour, H
- Aguilar, JA
- Ansseau, I
- Heereman, D
- Meagher, K
- Meures, T
- O'Murchadha, A
- Pinat, E
- Raab, C
- Ahlers, M
- Koskinen, DJ
- Larson, MJ
- Medici, M
- Rameez, M
- Ahrens, M
- Bohm, C
- Dumm, JP
- Finley, C
- Flis, S
- Hultqvist, K
- Walck, C
- Zoll, M
- Al Samarai, I
- Bron, S
- Carver, T
- Christov, A
- Montaruli, T
- Altmann, D
- Anton, G
- Gl'senkamp, T
- Katz, U
- Kittler, T
- Tselengidou, M
- Andeen, K
- Plum, M
- Anderson, T
- DeLaunay, JJ
- Dunkman, M
- Eller, P
- Huang, F
- Keivani, A
- Lanfranchi, JL
- Pankova, DV
- Te'ic, G
- Turley, CF
- Weiss, MJ
- Arg'elles, C
- Axani, S
- Collin, GH
- Conrad, JM
- Moulai, M
- Auffenberg, J
- Brenzke, M
- Glauch, T
- Haack, C
- Kalaczynski, P
- Koschinsky, JP
- Leuermann, M
- R'del, L
- Reimann, R
- Rongen, M
- S'lzer, T
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- Schumacher, L
- Stettner, J
- et al.
Neutrinos interact only very weakly, so they are extremely penetrating. The theoretical neutrino-nucleon interaction cross-section, however, increases with increasing neutrino energy, and neutrinos with energies above 40 teraelectronvolts (TeV) are expected to be absorbed as they pass through the Earth. Experimentally, the cross-section has been determined only at the relatively low energies (below 0.4 TeV) that are available at neutrino beams from accelerators. Here we report a measurement of neutrino absorption by the Earth using a sample of 10,784 energetic upward-going neutrino-induced muons. The flux of high-energy neutrinos transiting long paths through the Earth is attenuated compared to a reference sample that follows shorter trajectories. Using a fit to the two-dimensional distribution of muon energy and zenith angle, we determine the neutrino-nucleon interaction cross-section for neutrino energies 6.3-980 TeV, more than an order of magnitude higher than previous measurements. The measured cross-section is about 1.3 times the prediction of the standard model, consistent with the expectations for charged- and neutral-current interactions. We do not observe a large increase in the cross-section with neutrino energy, in contrast with the predictions of some theoretical models, including those invoking more compact spatial dimensions or the production of leptoquarks. This cross-section measurement can be used to set limits on the existence of some hypothesized beyond-standard-model particles, including leptoquarks.