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Hamiltonian Neural Networks approach to fuzzball geodesics

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arxiv 2502.20881 v3 pith:OSYOFBB4 submitted 2025-02-28 hep-th cs.LGgr-qc

classification hep-thcs.LGgr-qc
keywords equationshnnssolvedatafuzzballgeodesicshamiltonhamiltonian
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The recent increase in computational resources and data availability has led to a significant rise in the use of Machine Learning (ML) techniques for data analysis in physics. However, the application of ML methods to solve differential equations capable of describing even complex physical systems is not yet fully widespread in theoretical high-energy physics. Hamiltonian Neural Networks (HNNs) are tools that minimize a loss function defined to solve Hamilton equations of motion. In this work, we implement several HNNs trained to solve, with high accuracy, the Hamilton equations for a massless probe moving inside a smooth and horizonless geometry known as D1-D5 circular fuzzball. We study both planar (equatorial) and non-planar geodesics in different regimes according to the impact parameter, some of which are unstable. Our findings suggest that HNNs could eventually replace standard numerical integrators, as they are equally accurate but more reliable in critical situations.

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Cited by 2 Pith papers

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  1. Operator Learning in Lattice QCD: Spectral Reconstruction

    hep-lat 2026-07 conditional novelty 7.0 of 10

    DeepONet ensembles trained on GP mock data reconstruct O(3) smeared spectral densities from lattice correlators with lower total uncertainty than HLT, consistent with the analytic result.

  2. Machine Learning the 6d Supergravity Landscape

    hep-th 2025-05 conditional novelty 6.0 of 10

    An autoencoder and two neural classifiers, trained only on anomaly Gram matrices, provide automated clustering, outlier detection, and consistency predictions for millions of 6d supergravity building blocks.

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