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| Paper: |
Radiation Hydrodynamics of Core-Collapse Supernovae: The “Key” Asset for a
Self-consistent Modelling of These Events |
| Volume: |
453, Advances in Computational Astrophysics: Methods, Tools, and Outcome |
| Page: |
377 |
| Authors: |
Pumo, M. L.; Zampieri, L. |
| Abstract: |
We have developed a specifically tailored relativistic, radiation-hydrodynamics Lagrangian
code, that enables us to simulate the evolution of the main observables (light curve,
evolution of photospheric velocity and temperature) in core-collapse supernova (CC-SN) events.
The code features, some simulations as well as the implications of our results in connection with
a possible “standardization” of the hydrogen-rich CC-SNe are briefly discussed.
The possible role of this code in the development of a “CC-SNe Laboratory” for describing
the evolution of a CC-SN event in a “self-consistent” way (from the main sequence up to the
post-explosive phases) from a model/data comparison of light curves and spectra is also addressed. |
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