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

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