| State-of-the-art |
| COLLAPSE |
Stellar core collapse from pre-supernova models
including (some) of the following:
B-fields, GR, microphysics, 3D, v-transport |
| OUTFLOW |
| Ad-hoc model of the central engine |
hypercreating-BH + initial B
(strenght + topology) |
| Jet injection conditions |
| Jet propagation: AMR, (ideal) (G)R(M)HD,
estimate flow conditions at transparency |
| RADIATION |
| Assumed ejecta structure, kinematic models, analytic or
simplified emission models |
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- Magneto-rotational core collapse from pre-supernova models in full (time- evolving) GR, including microphysics, and (simplified) !-transport.
- Collapse followed beyond BH-formation, until a hyper-accreting BH forms.
- B-field consistently computed from the evolution of the pre-supernova core.
- Propagation of the jet in GRRMHD until it reaches transparency.
- Consistent calculation of the observational signature (radiation).
Extensions: 3D, improved !-transport, more emission processes (IC), etc.
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