A 3D Simulation of a Type II-P Supernova: From Core Bounce to beyond Shock Breakout

A 3D Simulation of a Type II-P Supernova: From Core Bounce to beyond Shock Breakout

In order to better connect core-collapse supernova (CCSN) theory with its observational signatures, we have developed a simulation pipeline from the onset of the core collapse to beyond shock breakout from the stellar envelope. Using this framework, we present a 3D simulation study from 5 s to over...

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Bibliographic Details
Main Authors: David Vartanyan, Benny T.-H. Tsang, Daniel Kasen, Adam Burrows, Tianshu Wang, Lizzy Teryoshin
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Supernova dynamics
Astrophysical fluid dynamics
Hydrodynamical simulations
Type II supernovae
Radiative transfer
Massive stars
Online Access:https://doi.org/10.3847/1538-4357/adb1e4
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https://doi.org/10.3847/1538-4357/adb1e4

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