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Chimera D-Series Gravitational Wave Emission Sourced from Matter

    Robert Daniel Murphy | University of Tennessee, Knoxville
    Anthony Mezzacappa | University of Tennessee, Knoxville
    Eric J. Lentz | Oak Ridge National Laboratory
    Pedro Marronetti | Physics Division, National Science Foundation
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Description

Gravitational wave data sourced from the the time-dependent fluid quadrupole motion, in the Chimera D-Series three-dimensional core collapse supernova simulations. Data from three models initiated from three different progenitors are presented: D9.6-3D, D15-3D, and D25-3D. Please see the README for more information about the data structure and progenitors.

Funding Information

DOE Contract Number

AC05-00OR22725

Originating Research Organization

The University of Tennessee, Knoxville TN (USA)

Other Contributing Organizations

Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); Physics Division, NSF, Alexandria VA (USA)

Sponsoring Organization

NSF Gravitational Physics; Office of Science (SC)

Project Identifier

AST137

Related Works

Details

DOI

https://doi.org/10.13139/OLCF/2571921

Release Date

August 7, 2025

Subject

ASTRONOMY AND ASTROPHYSICS

Keywords

Gravitational Waves, Core-Collapse Supernovae

Dataset

Dataset Type

ND Numeric Data

Other Contract Number(s)

PHY-2409148; PHY-2110177; PHY-1806692

Cite This Dataset:

Murphy, R., Mezzacappa, A., Lentz, E., Marronetti, P. (2025). Chimera D-Series Gravitational Wave Emission Sourced from Matter. Oak Ridge National Laboratory. https://doi.org/10.13139/OLCF/2571921.

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.