In this study, we propose a dynamical model for the evolution of velocity gradients in compressible turbulent flows with vibrational non-equilibrium effects, using physics-assisted deep neural networks. Such models provide a powerful framework for understanding the nonlinear physics associated with small-scale structures. In compressible flows, the influence of thermodynamic fields on velocity-gradient dynamics is represented through the thermodynamic gradient field (TGF) tensor. The TGF tensor is one of the primary unclosed terms in the velocity-gradient evolution equations. The TGF tensor comprises contributions from the pressure-Hessian tensor, rho bold italic upper H ρ H ρ H , and the baroclinic tensor, bold italic upper B B B . Accordingly, the proposed framework incorporates closures for both bold italic upper H H H and bold italic upper B B B tensor dynamics. Building upon existing phenomenological closures for the bold italic upper H H H tensor governing mechanisms, we develop a neural-network-based closure for the inviscid mechanism responsible for generating the bold italic upper B B B tensor. Unlike the other recently used tensor bases, the presented work employs a novel tensor basis allowing for the inclusion of non-symmetric features in the model. The framework also incorporates a data-driven closure for vibrational non-equilibrium effects. The resulting framework combines phenomenological and data-driven representations of various bold italic upper H H H and bold italic upper B B B tensors governing mechanisms, termed as the hybrid enhanced homogenised Euler equation (H-EHEE) model. Model predictions are evaluated across a range of turbulent Mach numbers and compared against direct numerica
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Shikha et al. (2026) studied this question.
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