Structure and evolution of shock waves in the presence of magnetic fields for heavy-ion collisions and astrophysics applications

This study presents a numerical and analytical model of hydro-dynamic and magnetohydrodynamic piston-driven shock waves, developed to generate benchmark solutions for shock dynamics in the presence and absence of magnetic fields in core-collapse supernovae environments.

Authors

Publication Details

Journal
Springer Link (Chiba Institute of Technology)
Published
2026-04-17
DOI
https://doi.org/10.1051/epjconf/202636414006/pdf
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
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article

Structure and evolution of shock waves in the presence of magnetic fields for heavy-ion collisions and astrophysics applications

Azwinndini Muronga, Magdeline Mohlao Seabi
Springer Link (Chiba Institute of Technology)
Gamma-ray bursts and supernovae
article

Structure and evolution of shock waves in the presence of magnetic fields for heavy-ion collisions and astrophysics applications

Azwinndini Muronga, Magdeline Mohlao Seabi
article en

Abstract

This study presents a numerical and analytical model of hydro-dynamic and magnetohydrodynamic piston-driven shock waves, developed to generate benchmark solutions for shock dynamics in the presence and absence of magnetic fields in core-collapse supernovae environments.

Springer Link (Chiba Institute of Technology)
Openalex Percentile: Top 8%
Gamma-ray bursts and supernovae
DOISourceOpenAlex
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Structure and evolution of shock waves in the presence of magnetic fields for heavy-ion collisions and astrophysics applications — Azwinndini Muronga, Magdeline Mohlao Seabi · Springer Link (Chiba Institute of Technology) (2026) | TGRS Research Map | TGRS