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Challenging a binary neutron star merger interpretation of GW230529 - Numerical Waveforms

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Zenodo2025-08-14 更新2026-05-26 收录
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https://zenodo.org/doi/10.5281/zenodo.16875324
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The numerical gravitational waveforms for the binary configurations simulated in the paper "Challenging a binary neutron star merger interpretation of GW230529" (Markin:2025oeo  / arXiv:2508.08750). The waveforms are produced using the NR code BAM, packaged in SXS 2019/NRAR format (cf. Appendix A.3 of Boyle:2019kee), and are grouped by the resolution. Ivan Markin and Tim Dietrich gratefully acknowledge support from the Deutsche Forschungsgemeinschaft (DFG) under the project 504148597 (DI 2553/7) and the computing time granted by the Resource Allocation Board and provided on the supercomputer Emmy/Grete at NHR-Nord@Göttingen as part of the NHR infrastructure. The calculations for this research were conducted with computing resources under the project bbp00049.
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2025-08-14
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