TY - CONF
T1 - The Character of Three-Dimensional Core-Collapse Simulation Results
AU - Burrows, Adam
AU - Coleman, Matthew
N1 - Publisher Copyright:
© The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).
PY - 2022/2/24
Y1 - 2022/2/24
N2 - 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.
AB - 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.
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U2 - 10.1051/epjconf/202226007001
DO - 10.1051/epjconf/202226007001
M3 - Paper
AN - SCOPUS:85183916347
T2 - 16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021
Y2 - 21 September 2021 through 25 September 2021
ER -