Stellar Mass Black Hole Formation and Multimessenger Signals from Three-dimensional Rotating Core-collapse Supernova Simulations
Authors/Creators
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1.
National Tsing Hua University
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2.
University of Basel
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3.
Michigan State University
Description
Gravitational waveforms from Pan et al. (2021) .
They are the 40 solar mass model from Woosley & Heger 2007 with different
initial rotational speeds:
Model NR: Omega_0 = 0.0 rad/sec
Model SR: Omega_0 = 0.5 rad/sec
Model 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 different
mode 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 the
quadruple 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]
Files
Files
(76.7 MB)
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Additional details
References
- Pan, K.-C., Liebendörfer, M., Couch, S.M., et al. 2021, ApJ, 914, 140. doi:10.3847/1538-4357/abfb05