2011/09/08 by M. L. Pumo, Pumo, M. L., L. Zampieri +1
Physics and Astronomy · #Astro and Planetary Science #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #Gamma-ray bursts and supernovae #Solar and Stellar Astrophysics (astro-ph.SR) #astro-ph.SR
paper · pdf · doi:10.48550/arxiv.1109.1775
2 pages, no figures, Proceedings of the meeting "Advances in Computational Astrophysics: methods, tools and outcomes", Cefalù (Sicily, Italy), June 13-17, 2011, to appear in ASP Conf. Series
arxiv created 2011/09/08 · openalex publication_date 2011/09/08 · arxiv updated 2011/09/09 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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.