Measurement of the multi-TeV neutrino cross section with IceCube using Earth absorption

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I CECUBE collaboration, Nature 551 (2017) 596 [1711.08119]

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IceCube Collaboration, I., Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., et al. Measurement of the multi-TeV neutrino cross section with IceCube us- ing Earth absorption. Nature, 551:596–600 (2017). doi:10.1038/nature24459. URL http://arxiv.org/abs/1711.08119

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IceCube Collaboration, “Measurement of the multi-TeV neutrino cross section with IceCube using Earth absorption,” Nature 551 (2017) 596–600, arXiv:1711.08119 [hep-ex]

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09972. [12] R. Abbasi et al. (IceCube), Science380, adc9818 (2023), 2307.04427. [13] A. Schneider, B. Skrzypek, C. A. Arg¨ uelles, and J. M. Conrad, Phys. Rev. D104, 092015 (2021), 2106.01508. [14] P. Di Bari, P. O. Ludl, and S. Palomares-Ruiz, JCAP11, 044 (2016), 1606.06238. [15] M. Tzanov et al. (NuTeV), Phys. Rev. D74, 012008 (2006), hep-ex/0509010. [16] M. G. Aartsen et al. (IceCube), Nature551, 596 (2017), 1711.08119. [17] R. Abbasi et al. (IceCube), Phys. Rev. D104, 022001 (2021), 2011.03560. [18] R. Abbasi et al. (IceCube), Phys. Rev. D111, 112001 (2025), 2502.13299. [19] R. Mammen Abraham et al. (FASER), Phys. Rev. Lett. 133, 021802 (2024), 2403.12520. [20] R. Mammen Abraham et al. (FASER) (2024), 2412.

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09972. [12] R. Abbasi et al. (IceCube), Science380, adc9818 (2023), 2307.04427. [13] A. Schneider, B. Skrzypek, C. A. Arg¨ uelles, and J. M. Conrad, Phys. Rev. D104, 092015 (2021), 2106.01508. [14] P. Di Bari, P. O. Ludl, and S. Palomares-Ruiz, JCAP11, 044 (2016), 1606.06238. [15] M. Tzanov et al. (NuTeV), Phys. Rev. D74, 012008 (2006), hep-ex/0509010. [16] M. G. Aartsen et al. (IceCube), Nature551, 596 (2017), 1711.08119. [17] R. Abbasi et al. (IceCube), Phys. Rev. D104, 022001 (2021), 2011.03560. [18] R. Abbasi et al. (IceCube), Phys. Rev. D111, 112001 (2025), 2502.13299. [19] R. Mammen Abraham et al. (FASER), Phys. Rev. Lett. 133, 021802 (2024), 2403.12520. [20] R. Mammen Abraham et al. (FASER) (2024), 2412

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This goal was achieved in less than three years of data collection, with a result that described an approximately isotropic high-energy neutrino flux that can be described by a power law of the typeϕν∝Φ 0E−γ ν. With the increase in the observatory's exposure time, other important advances were made, such as the measurement of the neutrino-target cross section [275-277], the identification of the first sources of these neutrinos [15,16,199], and, more recently, the description of the astrophysical neutrino flux with a broken power law [205,206]. Beyond the discoveries and measurements of Standard Model processes, Ice- Cube's experimental results have motivated the search for various processes beyond the Standard Model in the production [278-280], propagation [281-286] and interaction of