activity
20152025
most citedFlavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

197 citations · 1.1k across the 21 of their papers we have counts for

collaborators
Showing hep-exShow all

11 papers · 1 filter

hep-ex2025

Search for Heavy Neutral Leptons with IceCube DeepCore

R. Abbasi, M. Ackermann, J. Adams +421

The observation of neutrino oscillations has established that neutrinos have non-zero masses. This phenomenon is not explained by the Standard Model of particle physics, but one vi…

hep-ex2024

Measurement of atmospheric neutrino oscillation parameters using convolutional neural networks with 9.3 years of data in IceCube DeepCore

IceCube Collaboration

The DeepCore sub-detector of the IceCube Neutrino Observatory provides access to neutrinos with energies above approximately 5 GeV. Data taken between 2012-2021 (3,387 days) are ut…

hep-ex202238 cited

Graph Neural Networks for Low-Energy Event Classification & Reconstruction in IceCube

R. Abbasi, M. Ackermann, J. Adams +380

IceCube, a cubic-kilometer array of optical sensors built to detect atmospheric and astrophysical neutrinos between 1 GeV and 1 PeV, is deployed 1.45 km to 2.45 km below the surfac…

hep-ex2021

A muon-track reconstruction exploiting stochastic losses for large-scale Cherenkov detectors

R. Abbasi, M. Ackermann, J. Adams +362

IceCube is a cubic-kilometer Cherenkov telescope operating at the South Pole. The main goal of IceCube is the detection of astrophysical neutrinos and the identification of their s…

hep-ex2021

A Convolutional Neural Network based Cascade Reconstruction for the IceCube Neutrino Observatory

R. Abbasi, M. Ackermann, J. Adams +364

Continued improvements on existing reconstruction methods are vital to the success of high-energy physics experiments, such as the IceCube Neutrino Observatory. In IceCube, further…

hep-ex2020

Measurement of the high-energy all-flavor neutrino-nucleon cross section with IceCube

R. Abbasi, M. Ackermann, J. Adams +361

The flux of high-energy neutrinos passing through the Earth is attenuated due to their interactions with matter. The interaction rate is modulated by the neutrino interaction cross…