Researchers Use Quantum Computer to Classify Neutrino Events
Researchers Classify Neutrino Events With A Quantum Computer
Researchers achieved testing accuracy near 80% with neural projected quantum kernels and approximately 70% with quantum convolutional neural networks in classifying events detected by neutrino telescopes using a quantum computer, according to a study published August 21, 2026, in Quantum Science and Technology, Number 4. Led by Pablo Rodriguez-Grasa at the University of the Basque Country UPV/EHU, the team demonstrated this capability by investigating how quantum machine learning can handle high-energy physics datasets on current hardware.
The Tech TL;DR:
- Breakthrough Metric: Achieved testing accuracy near 80% using neural projected quantum kernels (NPQK) and ~70% with quantum convolutional neural networks (QCNNs).
- Hardware Validation: Successfully executed on both quantum simulators and the IBM Strasbourg quantum processor, validating real-world performance above 1 TeV.
- Data Engineering: Utilized a moment-of-inertia-based encoding scheme to reduce data dimensionality while preserving physical characteristics for limited qubit counts.
Overcoming High-Energy Physics Data Bottlenecks Through Moment-of-Inertia Encoding
Processing astronomical datasets from neutrino telescopes like IceCube has historically strained computational architectures due to massive feature spaces. Traditional graph neural networks hit infrastructure limits when processing the sheer volume of telemetry. To bypass this bottleneck, Rodriguez-Grasa and colleagues introduced a moment-of-inertia-based encoding scheme. Described in their study published August 21, 2026, in Quantum Science and Technology, Number 4, this preprocessing strategy maps the underlying physics and geometry of neutrino interactions into a lower-dimensional space. By shrinking the feature space, the team made the classification workload manageable for existing near-term quantum hardware.
Evaluating NPQK Versus QCNN Architectures on Hardware
The research evaluated two distinct quantum machine learning models to separate muon tracks from hadronic and electromagnetic showers—a fundamental distinction required to determine incoming neutrino flavors. The neural projected quantum kernel (NPQK) approach achieved testing accuracy near 80%, running directly on simulators and the IBM Strasbourg quantum processor. Meanwhile, the quantum convolutional neural network (QCNN) approach reached approximately 70% accuracy across a wide energy range during simulated tests.
Testing algorithms on physical QPUs introduces significant noise and decoherence challenges compared to ideal simulation environments. The deployment on the IBM Strasbourg quantum processor confirmed that model performance remained stable above 1 TeV, matching simulation benchmarks closely.
# Conceptual feature mapping pipeline for high-energy telemetry
import numpy as np
def moment_of_inertia_encoding(event_tensor):
# Reduce dimensionality while preserving spatial geometry
moments = np.sum(event_tensor * np.square(np.arange(event_tensor.shape[0])), axis=0)
normalized_features = moments / np.linalg.norm(moments)
return normalized_features
# Feed compressed feature vector into quantum kernel evaluation
Practical Implications for Astrophysics Data Pipelines
According to the findings published in Quantum Science and Technology, this deployment marks a foundational step in applying quantum machine learning directly to astrophysical data analysis. By bypassing pure simulation and executing on physical hardware, the methodology proves resilient against hardware noise constraints.

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