Phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes
暂无分享,去创建一个
[1] Lawrence E. Kidder,et al. Multipolar effective-one-body waveforms for precessing binary black holes: Construction and validation , 2020, Physical Review D.
[2] D. Keitel,et al. Let's twist again: computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes , 2020 .
[3] M. Colleoni,et al. Setting the cornerstone for a family of models for gravitational waves from compact binaries: The dominant harmonic for nonprecessing quasicircular black holes , 2020, 2001.11412.
[4] M. Colleoni,et al. Multimode frequency-domain model for the gravitational wave signal from nonprecessing black-hole binaries , 2020, 2001.10914.
[5] P. Schmidt,et al. Validity of common modeling approximations for precessing binary black holes with higher-order modes , 2020, 2001.10936.
[6] G. Pratten,et al. Multipolar effective one body waveform model for spin-aligned black hole binaries , 2020, 2001.09082.
[7] F. Ohme,et al. Including higher order multipoles in gravitational-wave models for precessing binary black holes , 2019, Physical Review D.
[8] L. Haegel,et al. Predicting the properties of black-hole merger remnants with deep neural networks , 2019, Classical and Quantum Gravity.
[9] S. Marsat,et al. Fourier-domain modulations and delays of gravitational-wave signals , 2018, 1806.10734.
[10] P. Schmidt,et al. Numerical Relativity Injection Infrastructure , 2017, 1703.01076.
[11] B. Iyer,et al. Post-Newtonian prediction for the (2,2) mode of the gravitational wave emitted by compact binaries , 2012, 1210.2339.