Most simulations for my research rely on my own multi-D hydrodynamics code. The code is built based on the 1D prototype developed by my former graduate classmate Mr. Ka-Wing Wong. After I picked up the code, I extend to multi-D, and insert all necessary physics for modeling supernova. 

The code uses the 5th order WENO scheme for spatial discretization and 3rd order 5-step NSSP Runge-Kutta scheme for time discretization. 

The code includes physics and has been used for simulations for:

• Type Ia supernova

• Electron capture supernova

• Collapsar

• Dark matter admixed stellar objects

• Stellar pulsation

Collaboration using our code for scientific research is warmly welcome. Contact for further details. 

(Github Under construction)

Standard shocktube test for the Riemann solver of the hydro code. 

Gresho vortex test for testing the code advection

Spherical blast test demonstrating the code capturing perfect symmetry

Kelvin-Helmholtz instability test showing the spiraling flow inside "eyes".