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Understanding Core-Collapse Supernovae

2004/05/21 by Adam Burrows, Burrows, Adam
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0405427

to be published in the proceedings of the Twelfth Workshop on "Nuclear Astrophysics," a Tribute to an Explosive Astrophysicist, Wolfgang Hillebrandt, on the occasion of his 60th Birthday, held at the Ringberg Castle, Lake Tegernsee, Germany, March 22 - 27, 2004, eds. E. Muller and H.-Th. Janka

arxiv created 2004/05/21 · openalex publication_date 2004/05/21 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

I summarize, in the form of an extended abstract, the ongoing efforts at the University of Arizona (and in collaboration) to understand core-collapse supernovae theoretically. Included are short discussions of 1D (SESAME) and 2D (VULCAN/2D) codes and results, as well as discussions of the possible role of rotation. Highlighted are recent developments in multi-dimensional radiation hydrodynamics and the essential physics of the neutrino-driven mechanism.

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