Thermal Radiation Transport with Tensor Trains

Abstract We present a novel tensor network algorithm to solve the time-dependent, gray thermal radiation transport equation. The method invokes a tensor train (TT) decomposition for the specific intensity. The efficiency of this approach is dictated by the rank of the decomposition. When the solution is “low rank,” the memory footprint of the specific intensity solution vector may be significantly compressed. The algorithm, following a step-then-truncate approach of a traditional discrete ordinates method, operates directly on the compressed state vector, thereby enabling large speedups for low-rank solutions. To achieve these speedups, we rely on a recently developed rounding approach based on the Gram-SVD. We detail how familiar S N algorithms for (gray) thermal transport can be mapped to this TT framework and present several numerical examples testing both the optically thick and thin regimes. The TT framework finds low-rank structure and supplies up to ≃60× speedups and ≃1000× compressions for problems demanding large angle counts, thereby enabling previously intractable S N calculations and supplying a promising avenue to mitigate ray effects.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-07-14
DOI
https://doi.org/10.3847/1538-4357/adda3f
Citations
3
Primary Topic
Tensor decomposition and applications
Type
article
Field-Weighted Citation Impact
4.60
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article

Thermal Radiation Transport with Tensor Trains

Jonah Miller, Alex Arkady Gorodetsky, Luke F. Roberts, Joshua C. Dolence et al.
3 citations
The Astrophysical Journal
Tensor decomposition and applications
4.60
article

Thermal Radiation Transport with Tensor Trains

Jonah Miller, Alex Arkady Gorodetsky, Luke F. Roberts, Joshua C. Dolence, Chad Meyer, Patrick D. Mullen, Aditya Deshpande
article en
3 citations

Abstract

Abstract We present a novel tensor network algorithm to solve the time-dependent, gray thermal radiation transport equation. The method invokes a tensor train (TT) decomposition for the specific intensity. The efficiency of this approach is dictated by the rank of the decomposition. When the solution is “low rank,” the memory footprint of the specific intensity solution vector may be significantly compressed. The algorithm, following a step-then-truncate approach of a traditional discrete ordinates method, operates directly on the compressed state vector, thereby enabling large speedups for low-rank solutions. To achieve these speedups, we rely on a recently developed rounding approach based on the Gram-SVD. We detail how familiar S N algorithms for (gray) thermal transport can be mapped to this TT framework and present several numerical examples testing both the optically thick and thin regimes. The TT framework finds low-rank structure and supplies up to ≃60× speedups and ≃1000× compressions for problems demanding large angle counts, thereby enabling previously intractable S N calculations and supplying a promising avenue to mitigate ray effects.

The Astrophysical JournalVol. 988(1)
Los Alamos National Laboratory (US), University of Michigan (US), Computational Physics (United States) (US)
Openalex Percentile: Top 5%
Tensor decomposition and applications
4.60
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