Corpus ID: 237416648

Modeling Core-Collapse Supernovae Gravitational-Wave Memory in Laser Interferometric Data

@inproceedings{Richardson2021ModelingCS,
  title={Modeling Core-Collapse Supernovae Gravitational-Wave Memory in Laser Interferometric Data},
  author={Colter Richardson and Michele Zanolin and H Andresen and M. J. Szczepa'nczyk and Kiranjyot Gill and Annop Wongwathanarat Embry-Riddle Aeronautical University and Max-Planck-Institute for Extraterrestrial Physics and University of Central Florida and Harvard University and Max Planck Institute for Astrophysics},
  year={2021}
}
We study the properties of the gravitational wave (GW) emission between 10−5 Hz and 50 Hz (which we refer to as low-frequency emission) from core-collapse supernovae, in the context of studying such signals in laser interferometric data as well as performing multi-messenger astronomy. We pay particular attention to the GW linear memory, which is when the signal amplitude does not return to zero after the GW burst. Based on the long term simulation of a core-collapse supernova of a solar… Expand

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