A waveform of the predicted gravitational wave signal from the collapse of a rotating 300M star
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Amplitude waveform of the gravitational waves extracted from a 2D axisymmetric simulation of the collapse of a 300 solar mass rotating star. The simulation is performed using the CoCoNuT-FMT code with general relativistic gravity. Data is given in plain text format, and as a numpy array for convenience. Columns are time (units of seconds) and gravitational wave amplitude A^{E2}_{20} (units of cm; see Mueller, Janka, Marek [2013, ApJ] for a mathematical definition).
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Zenodo创建时间：
2026-04-09
