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Physics Capabilities of the IceCube DeepCore Detector

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arxiv 0907.2263 v1 pith:XQ43FQTB submitted 2009-07-14 astro-ph.IM astro-ph.HE

classification astro-ph.IMastro-ph.HE
keywords icecubeneutrinodetectorsensitivityexperimentsfullstringsadditional
verification ladder T0 review T1 audit T2 compute T3 formal

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IceCube-DeepCore is a compact Cherenkov detector located in the clear ice of the bottom center of the IceCube Neutrino Telescope. Its purpose is to enhance the sensitivity of IceCube for low neutrino energies (< 1 TeV) and to lower the detection threshold of IceCube by about an order of magnitude to below 10 GeV. The detector is formed by 6 additional strings of 360 high quantum efficiency phototubes together with the 7 central IceCube strings. The improved sensitivity will provide an enhanced sensitivity to probe a range of parameters of dark matter models not covered by direct experiments. It opens a new window for atmospheric neutrino oscillation measurements of muon neutrino disappearance or tau neutrino appearance in an energy region not well tested by previous experiments, and enlarges the field of view of IceCube to a full sky observation when searching for potential neutrino sources. The first string was succesfully installed in January 2009, commissioning of the full detector is planned early 2010.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 24 citations worldwide. Full citation record

  1. Constraining primordial black holes and primordial curvature power spectrum with extragalactic muon neutrino

    astro-ph.CO 2026-07 conditional novelty 4.0 of 10

    Neutrino flux from WIMP annihilation in PBH-seeded UCMHs yields f_PBH ≲ 4×10^{-5} (strongest) and P_R ≲ 10^{-1.65} at k∼3×10^{12} Mpc^{-1}.

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