Stellar Mass Black Hole Formation and Multimessenger Signals from Three-dimensional Rotating Core-collapse Supernova Simulations
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https://zenodo.org/record/13743760
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资源简介：
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]
创建时间：
2024-09-11
