Numerical Inside View of Hypermassive Remnant Models for GW170817 supplemental data
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This archive contains gravitational waveform data discussed in the article Wolfgang Kastaun, Frank Ohme, "Numerical Inside View of Hypermassive Remnant Models for GW170817" (2021) It was extracted from numerical simulations using the SFHO EOS and the chirp mass inferred for GW170817, using two mass ratios 1 and 0.9. Both the raw numerical waveform and a hybridized waveform are provided. The data format is described in the README file.
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Zenodo创建时间：
2021-03-01
