| Issue |
EPJ Web Conf.
Volume 364, 2026
XXXI International Conference on Ultra-Relativistic Nucleus-Nucleus Collisions “Quark Matter 2025”
|
|
|---|---|---|
| Article Number | 14006 | |
| Number of page(s) | 4 | |
| Section | QCD Matter in Astrophysics | |
| DOI | https://doi.org/10.1051/epjconf/202636414006 | |
| Published online | 17 April 2026 | |
https://doi.org/10.1051/epjconf/202636414006
Structure and evolution of shock waves in the presence of magnetic fields for heavy-ion collisions and astrophysics applications
1 Nelson Mandela University, Faculty of Science, Department of Physics, x43, Summerstrand, Gqe- berha, 6001
2 Nelson Mandela University, x43, Summerstrand, Gqeberha, 6001
3 NITheCS, Stellenbosch, 7600
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Published online: 17 April 2026
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.
© The Authors, published by EDP Sciences, 2026
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