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IceCube-Gen2: A Vision for the Future of Neutrino Astronomy in Antarctica
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arxiv 1412.5106 v2 pith:SVWU77M6 submitted 2014-12-16 astro-ph.HE astro-ph.IMhep-ex
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abstract
The recent observation by the IceCube neutrino observatory of an astrophysical flux of neutrinos represents the "first light" in the nascent field of neutrino astronomy. The observed diffuse neutrino flux seems to suggest a much larger level of hadronic activity in the non-thermal universe than previously thought and suggests a rich discovery potential for a larger neutrino observatory. This document presents a vision for an substantial expansion of the current IceCube detector, IceCube-Gen2, including the aim of instrumenting a $10\,\mathrm{km}^3$ volume of clear glacial ice at the South Pole to deliver substantial increases in the astrophysical neutrino sample for all flavors. A detector of this size would have a rich physics program with the goal to resolve the sources of these astrophysical neutrinos, discover GZK neutrinos, and be a leading observatory in future multi-messenger astronomy programs.
Forward citations
Cited by 3 Pith papers
Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record
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Can Quasi-periodic Eruptions Produce Detectable High Energy Neutrinos?
astro-ph.HE 2025-09 conditional novelty 6.0 of 10
Quasi-periodic eruptions could accelerate protons to tens of TeV, but their 10-year neutrino fluences and IceCube event rates are too low for individual detection except for very nearby sources.
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Fundamental physics with high-energy cosmic neutrinos today and in the future
astro-ph.HE 2019-07 unverdicted novelty 2.0 of 10
High-energy astrophysical neutrinos enable stringent tests of physics beyond the Standard Model at energies and baselines unreachable by other means.
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A White Paper on The Multi-Messenger Science Landscape in India
astro-ph.HE 2025-05 unverdicted novelty 1.0 of 10
No new scientific result is presented; the document reviews multi-messenger science and recommends a national coordination center linking Indian gravitational wave, electromagnetic, cosmic ray, and neutrino facilities.
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