The Character of Three-Dimensional Core-Collapse Simulation Results

Adam Burrows; Matthew Coleman

doi:10.1051/epjconf/202226007001

The Character of Three-Dimensional Core-Collapse Simulation Results

Adam Burrows
, Matthew Coleman

Department of Physics

Princeton University

Research output: Contribution to conference › Paper › peer-review

1 Scopus citations

Abstract

We here in graphical form highlight some of the early phases in the explosion of core-collapse supernovae and the birth of neutron stars. The graphics presented summarizes the results of the almost fifty three-dimensional radiation/hydrodynamic simulations the Princeton group has simulated during the last three years using its state-of-the-art (though still evolving and improving) code Fornax.

Original language	English
DOIs	https://doi.org/10.1051/epjconf/202226007001
State	Published - 24 Feb 2022
Event	16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021 - Chengdu, China Duration: 21 Sep 2021 → 25 Sep 2021

Conference

Conference	16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021
Country/Territory	China
City	Chengdu
Period	21/09/21 → 25/09/21

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10.1051/epjconf/202226007001

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The Character of Three-Dimensional Core-Collapse Simulation Results

Abstract

Conference

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