4.7 Article

Dimuons in neutrino New and first search in IceCube

Journal

PHYSICAL REVIEW D
Volume 105, Issue 9, Pages -

Publisher

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.105.093005

Keywords

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Funding

  1. Simons Foundation
  2. National Science Foundation [PHY-2012955]

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This article introduces a new method for detecting dimuon events using neutrino telescopes. The authors conducted theoretical and observational research, and proposed potential detection results for the IceCube and IceCube-Gen2 telescopes. However, analysis of the publicly available IceCube data revealed that the previously identified candidate dimuon events were not real dimuons, but rather an internal reconstruction error.
Neutrino telescopes allow powerful probes of high-energy astrophysics and particle physics. Their power is increased when they can isolate different event classes, e.g., by flavor, though that is not the only possibility. Here we focus on a new event class for neutrino telescopes: dimuons, two energetic muons from one neutrino interaction. We make new theoretical and observational contributions. For the theoretical part, we calculate dimuon-production cross sections and detection prospects via deep-inelastic scattering (DIS; where we greatly improve upon prior work) and W-boson production (WBP; where we present first results). We show that IceCube should have ???130 dimuons (???6 from WBP) in its current data and that IceCube-Gen2, with a higher threshold but a larger exposure, could detect ???620 dimuons (???30 from WBP) in 10 years. These dimuons are almost all produced by atmospheric neutrinos. For the observational part, we perform a simple but conservative analysis of IceCube public data, finding 19 candidate dimuon events. Subsequent to our paper appearing, visual inspection of these events by the IceCube Collaboration revealed that they are not real dimuons, but instead arise from an internal reconstruction error that identifies some single muons crossing the dust layer as two separate muons. To help IceCube and the broader community with future dimuon searches, we include the updated full details of our analysis. Together, these theoretical and observational contributions help open a valuable new direction for neutrino telescopes, one especially important for probing high-energy QCD and new physics.

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