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Synapse
April 24, 2026

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

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Authors

MSMagdeline Mohlao SeabiAMAzwinndini Muronga

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Overview

Numerical and analytical models demonstrate shock wave behavior in core-collapse supernovae, indicating important astrophysical implications.

Key Points

  • The research aims to model shock waves influenced by magnetic fields in astrophysical scenarios.
  • Developed numerical and analytical models for shock waves
  • Examined shock dynamics under varying magnetic field conditions
  • Generated benchmark solutions to validate shock wave behavior
  • Demonstrated distinct shock wave properties in the presence of magnetic fields
  • Provided insights into hydro-dynamic and magnetohydrodynamic interactions
  • Established foundational knowledge for future astrophysics applications

Cite This Study

Seabi et al. (2026) studied this question.

synapsesocial.com/papers/69eb0a94553a5433e34b4a02https://doi.org/10.1051/epjconf/202636414006/pdf
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