15–19 Jun 2026
UC Irvine
America/New_York timezone

RTE–cNSF: A Hybrid Physics–ML Architecture for Accurate Photon Timing in JUNO

16 Jun 2026, 11:00
15m
The Interdisciplinary Science and Engineering Building (UC Irvine)

The Interdisciplinary Science and Engineering Building

UC Irvine

419 Physical Sciences Quad, Irvine, CA 92697

Speaker

Qiyu Yan (University of Chinese Academy of Sciences)

Description

Accurate photon timing in large liquid-scintillator neutrino detectors requires precise modeling of complex optical processes. These include complex scattering, absorption and re-emission, boundary effects, steel-frame shadowing, and multi-path reverberation. These effects draw a complex picture that is yet intractable for analytic methods and too detector-specific to learn end-to-end. We present a hybrid physics--ML architecture, RTE--cNSF, designed for the JUNO detector, which combines a physics-based radiative transfer equation (RTE) solver with a conditional neural spectral field (cNSF) to model these processes.

The architecture enforces a strict first-hit handoff boundary: the RTE handles light propagation inside the liquid scintillator up to the acrylic boundary, while a frozen cNSF --- trained on filtered GEANT4 tracks --- captures all subsequent water-buffer physics. Exploiting the SO(2) symmetry of individual PMTs, the neural model operates on a compact, three-parameter local invariant space, preventing the leakage of source-specific information into the boundary model.

The spatial integration is trifurcated into three topologically disjoint pipelines: a target-driven Fermat path solved analytically via 1D auto-differentiation (JAX) with a symmetry-reduced Jacobian; a diffuse direct-light channel sampled over a 2D Sobol sequence with an orthogonality veto mask; and a scattered-light channel over a 5D boundary manifold. The resulting optical delay kernel is assembled by convolving the spatially integrated flux with the cNSF timing distribution, the scintillator emission profile, chromatic dispersion, and the PMT transit-time spread via FFT, preserving full differentiability for parameter inference.

This work aims to provide a computationally efficient and physically accurate model for photon timing in the JUNO detector, enabling improved calibration, event reconstruction, and ultimately enhancing the sensitivity of neutrino measurements.

Contribution types Standard talk (20min + 5min Q/A)

Authors

Benda Xu (Tsinghua University) Qiyu Yan (University of Chinese Academy of Sciences) Shengqi Chen (Tsinghua University)

Presentation materials