MPI for Astrophysics
|Title (1st Abstract)||
The first few month of a supernova remnant
Max-Planck-Institute for Astrophysics
H.-T. Janka, A. Wongwathanarat
6. Jets and Asymmetries in SNe and their Remnants
We perform long-term, hydrodynamical simulations of supernova remnants in 3 dimensions. Continuing the simulations of A.Wongwathanarat “3D long-time CCSN simulations: from shock revival to shock break-out” we follow the evolution of the shock and the ejecta during the first few month after the explosion. The explosion is simulated with a ray-by-ray gray neutrino transport approximation and the so called Yin-Yang grid (an axis-free spherical polar coordinates grid).