A new radiation-hydrodinamics code to study core-collapse supernova events

2011/09/08 by M. L. Pumo, Pumo, M. L., L. Zampieri +1
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #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.1109.1791

3 pages, 5 figures, Proceedings of the meeting "GIANT 2010", Catania (Sicily, Italy), March 29-31 2010, to appear on special issue of report LNS (ISSN 182 1561)

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 core-collapse supernova events, 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 these events. The code features, some testcase simulations and the possible applications of the code are briefly discussed.

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