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We present a novel machine learning (ML)-based method to accelerate conservative-to-primitive inversion, focusing on hybrid piecewise polytropic and tabulated equations of state. Traditional root-finding techniques are computationally expensive, particularly for large-scale relativistic hydrodynamics simulations. To address this, we employ feedforward neural networks (
Details
Relativistic effects;
Neutrons;
Neutron stars;
Artificial neural networks;
Supercomputers;
Numerical analysis;
Hydrodynamics;
Theory of relativity;
Machine learning;
Performance evaluation;
Numerical methods;
Data points;
Simulation;
Datasets;
Graphics processing units;
Equations of state;
Neural networks;
Optimization;
Inference;
Variables;
Spacetime;
Methods;
Algorithms;
Fluid mechanics;
Parameter estimation
; Haas, Roland 2
; Huerta, E A 3
1 Department of Physics, University of Illinois Urbana-Champaign, Urbana, IL 61801, USA, National Center for Supercomputing Applications, University of Illinois Urbana-Champaign, Urbana, IL 61801, USA
2 Department of Physics, University of Illinois Urbana-Champaign, Urbana, IL 61801, USA, National Center for Supercomputing Applications, University of Illinois Urbana-Champaign, Urbana, IL 61801, USA, Department of Physics an Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1, Canada
3 Department of Physics, University of Illinois Urbana-Champaign, Urbana, IL 61801, USA, Data Science and Learning Division, Argonne National Laboratory, Lemont, IL 60439, USA, Department of Computer Science, The University of Chicago, Chicago, IL 60637, USA