Dimuons in Neutrino Telescopes: New Predictions and First Search in IceCube

TL;DR

This paper introduces a new class of neutrino events called dimuons, provides theoretical calculations for their production, and performs an initial search using IceCube data, highlighting their potential for astrophysics and particle physics research.

Contribution

It offers the first detailed calculations of dimuon production cross sections and detection prospects, along with the first observational search in IceCube data, including an analysis of candidate events.

Findings

IceCube could detect ~130 dimuons in current data

IceCube-Gen2 could detect ~620 dimuons in 10 years

Initial candidate events were found but later identified as reconstruction errors

Abstract

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 $\simeq 130$ dimuons ($\simeq 6$ from WBP) in its current data and that IceCube-Gen2, with a higher threshold but a larger exposure, could detect $\simeq 620$ dimuons ($\simeq 30$ 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.