Stellar Mass Black Hole Formation and Multimessenger Signals from Three-dimensional Rotating Core-collapse Supernova Simulations (Q6718433)
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Dataset published at Zenodo repository.
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Stellar Mass Black Hole Formation and Multimessenger Signals from Three-dimensional Rotating Core-collapse Supernova Simulations |
Dataset published at Zenodo repository. |
Statements
Gravitational waveforms from Pan et al. (2021) . They are the 40 solar mass model from Woosley Heger 2007 with differentinitial rotational speeds: Model NR: Omega_0 = 0.0 rad/secModel SR: Omega_0 = 0.5 rad/secModel FR: Omega_0 = 1.0 rad/sec /* File content */ They are 5 files for each simulation. Files "data_s40_[model]_d3_[Cross/Plus][Equator/Pole].d" are GW strains for differentmode of polarization [h_plus or h_cross] and viewing angles [equator or pole]. 1st column is time [s] in postbounce.2nd column s the GW strain, assuming d=10 kpc.Files "data_s40_[model]_d3_Idotdot.d" are the second time derivative of thequadruple moments. 1st: postbounce time [s]2nd: Idd_xx [cgs]3rd: Idd_xy = Idd_yx [cgs]4th: Idd_yy = Idd_yy [cgs]5th: Idd_zx = Idd_zx [cgs]6th: Idd_zy = Idd_zy [cgs]7th: Idd_zz = Idd_zz [cgs]
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11 September 2024
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v1.0
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