https://doi.org/10.1051/epjconf/202226007001
The Character of Three-Dimensional Core-Collapse Simulation Results
Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08540
* e-mail: burrows@astro.princeton.edu
** e-mail: msbc@astro.princeton.edu
Published online: 24 February 2022
We here in graphical form highlight some of the early phases in the explosion of core-collapse supernovae and the birth of neutron stars. The graphics presented summarizes the results of the almost fifty three-dimensional radiation/hydrodynamic simulations the Princeton group has simulated during the last three years using its state-of-the-art (though still evolving and improving) code Fornax.
© The Authors, published by EDP Sciences, 2022
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
