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Selected 3D Flash-X Checkpoints for the Long-Time Evolution of a 9.6 Solar-Mass Core-Collapse Supernova Model

    Sudarshan Neopane | University of Tennessee, Knoxville
    Michael Sandoval | Oak Ridge National Laboratory
    William Raphael Hix | Oak Ridge National Laboratory
    James Austin Harris | Oak Ridge National Laboratory
    Otis Messer | Oak Ridge National Laboratory
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Description

This dataset contains selected 3D Flash-X checkpoint files from the long-time evolution of a low-energy core-collapse supernova explosion of a 9.6 Msun zero-metallicity, low-mass iron-core progenitor. The checkpoints span the shock-breakout phase through the young-remnant phase, ending at approximately 3 yr after core bounce. The dataset is intended for follow-up analysis and post-processing, especially radiation-transport calculations using the hydrodynamic and compositional structure of the ejecta. For a full description of the numerical setup, physical assumptions, limitations, and interpretation of the simulation, users should refer to the associated paper.

Funding Information

DOE Contract Number

AC05-00OR22725

Originating Research Organization

Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)

Other Contributing Organizations

National Science Foundation

Sponsoring Organization

Office of Science (SC)

Related Works

Details

Release Date

July 8, 2026

Subject

79 ASTRONOMY AND ASTROPHYSICS

Keywords

Core-Collapse Supernovae, hydrodynamics

Dataset

Dataset Type

ND Numeric Data

Software

Visit, yt, h5py, hdf5

Cite This Dataset:

Neopane, S., Sandoval, M., Hix, W., Harris, J., Messer, O., Lentz, E. (2026). Selected 3D Flash-X Checkpoints for the Long-Time Evolution of a 9.6 Solar-Mass Core-Collapse Supernova Model. Oak Ridge National Laboratory. https://doi.org/10.13139/OLCF/3367469.

Acknowledgements

This research used resources of the Oak Ridge Leadership Computing Facility at the Oak Ridge National Laboratory, which is supported by the Advanced Scientific Computing Research programs in the Office of Science of the U.S. Department of Energy under Contract No. DE-AC05-00OR22725.