Evolution of the main observables in core-collapse supernova events: a radiation-hydrodynamical modelling

2011/09/08 by M. L. Pumo, Pumo, M. L., L. Zampieri +1
Physics and Astronomy · #Astro and Planetary Science #FOS: Physical sciences #Gamma-ray bursts and supernovae #Pulsars and Gravitational Waves Research #Solar and Stellar Astrophysics (astro-ph.SR) #astro-ph.SR

paper · pdf · doi:10.48550/arxiv.1109.1770

4 pages, 2 figures, Proceedings of the "54° congresso della Societa' Astronomica Italiana", Napoli, May 4-7, 2010, to appear in Mem. S.A.It. Suppl

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

Abstract

With the aim of clarifying the nature of the supernova events from stars having initial (at the main sequence) masses larger than ∼ 8-10 M_\odot, we have developed a specifically tailored radiation hydrodynamics Lagrangian code, that enables us to simulate the evolution of the main observables (light curve, evolution of photospheric velocity and temperature) in these events. The code features and some test-case simulations as well as the possible applications of the code are briefly discussed.

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