collaborators

8 papers

cs.LG2026

A Hyperbolic Neural Closure for M1 Radiation Transfer

Bongseok Kim, Jiahao Zhang, Johannes Krotz +3

In radiation transfer simulations, an M1 method achieves substantial computational savings by replacing the full angular transport equation with a low-order moment system. Because…

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…

astro-ph.SR2026

Two-Dimensional Kelvin-Helmholtz Instability with Anisotropic Pressure

Shishir Biswas, Masaru Nakanotani, Dinshaw S. Balsara +2

The Kelvin-Helmholtz (KH) instability occurs in multiple heliospheric (solar-wind stream interfaces, planetary magnetospheres, cometary tails, heliopause flanks) and interstellar (…

math.NA2025

An Alternative Finite Difference WENO-like Scheme with Physical Constraint Preservation for Divergence-Preserving Hyperbolic Systems

Dinshaw S. Balsara, Deepak Bhoriya, Chi-Wang Shu

Alternative finite difference Weighted Essentially Non-Oscillatory (AFD-WENO) schemes allow us to very efficiently update hyperbolic systems even in complex geometries. Recent inno…

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…