Sequential Monte Carlo with Cross-validated Neural Networks for Complexity of Hyperbolic Black Hole Solutions in 4D
Armin Hatefi, Ehsan Hatefi

TL;DR
This paper introduces a novel Bayesian Sequential Monte Carlo method combined with neural networks to accurately estimate complex, multi-modal solutions of hyperbolic black hole equations in 4D, accounting for measurement errors.
Contribution
It develops a new probabilistic framework using SMC and neural networks for solving highly nonlinear, multi-modal equations in gravitational physics, incorporating measurement errors and cross-validation.
Findings
Confirmed known solutions in the literature.
Identified all possible solutions considering measurement errors.
Enhanced prediction of critical functions for multiple solutions.
Abstract
This paper investigates the self-similar solutions of the Einstein-axion-dilaton configuration from type IIB string theory and the global SL(2,R) symmetry. We consider the Continuous Self Similarity (CSS), where the scale transformation is controlled by an SL(2, R) boost or hyperbolic translation. The solutions stay invariant under the combination of space-time dilation with internal SL(2,R) transformations. We develop a new formalism based on Sequential Monte Carlo (SMC) and artificial neural networks (NNs) to estimate the self-similar solutions to the equations of motion in the hyperbolic class in four dimensions. Due to the complex and highly nonlinear patterns, researchers typically have to use various constraints and numerical approximation methods to estimate the equations of motion; thus, they have to overlook the measurement errors in parameter estimation. Through a Bayesian…
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