collaborators

8 papers

math.NA2026

Entropy stable finite difference schemes for One-Fluid Two-Temperature Euler Non-equilibrium Hydrodynamics

Chetan Singh, Harish Kumar

In this work, we consider the One-Fluid Two-Temperature Euler (OFTT-Euler) equations used for modeling non-equilibrium hydrodynamics. The model comprises a system of nonlinear hype…

math.NA2026

Admissible Lax-Wendroff Flux Reconstruction Method with Automatic Differentiation on Adaptive Curved Meshes for Relativistic Hydrodynamics

Sujoy Basak, Arpit Babbar, Harish Kumar +1

The relativistic hydrodynamics (RHD) equations can give rise to solutions which have shocks, contact discontinuities, and other sharp structures, which interact and evolve over tim…

physics.plasm-ph2026

Entropy stable numerical schemes for divergence diminishing Chew, Goldberger & Low equations for plasma flows

Chetan Singh, Harish Kumar, Deepak Bhoriya +1

Chew, Goldberger & Low (CGL) equations are a set of hyperbolic PDEs with non-conservative products used to model the plasma flows, when the assumption of local thermodynamic equili…

math.NA2025

Constraints Preserving Lax-Wendroff Flux Reconstruction for Relativistic Hydrodynamics with General Equations of State

Sujoy Basak, Arpit Babbar, Harish Kumar +1

In the realm of relativistic astrophysics, the ideal equation of state with a constant adiabatic index provides a poor approximation due to its inconsistency with relativistic kine…

astro-ph.IM2025

Physical Constraint Preserving Higher Order Finite Volume Schemes for Divergence-Free Astrophysical MHD and RMHD

Dinshaw S. Balsara, Deepak Bhoriya, Chetan Singh +3

Higher order finite volume schemes for magnetohydrodynamics (MHD) and relativistic magnetohydrodynamics (RMHD) are very valuable because they allow us to carry out astrophysical si…

math.NA2025

Chew, Goldberger & Low Equations: Eigensystem Analysis and Applications to One-Dimensional Test Problems

Chetan Singh, Deepak Bhoriya, Anshu Yadav +2

Chew, Goldberger & Low (CGL) equations describe one of the simplest plasma flow models that allow anisotropic pressure, i.e., pressure is modeled using a symmetric tensor described…