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Chimera D-Series Gravitational Wave Emission Sourced from Matter

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

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 Resources

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; DOE Office of Science (SC)

Project Identifier

AST137

Related Resources

Details

DOI

10.13139/OLCF/2571921

Release Date

August 7, 2025

Dataset

Dataset Type

ND Numeric Data

Other Contract Number(s)

PHY-2409148; PHY-2110177; PHY-1806692

Acknowledgements

Users should acknowledge the OLCF in all publications and presentations that speak to work performed on OLCF resources:

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

Category

  • 79 ASTRONOMY AND ASTROPHYSICS

Keywords

  • Gravitational Waves,
  • Core-Collapse Supernovae