Pa dl 5974
However, if initial state is not a BH, the inspiral stage could in principle be used to discriminate against a two-BH initial state, since the quadrupole moment, tidal love numbers or absorption of the initial state is different from that of a BH, see e. Inflation is the current paradigm of the early universe. Blanco-Pillado, J. However, this assumption could bring bias that causes systematic errors in the parameter estimation of signals, e. References 1. The domain-wall bubbles or relevant objects can spontaneously nucleate in de Sitter space and be stretched by the inflation to astrophysical scales [ 3 ], see also [ 4 ]. Correspondence to Yu-Tong Wang.
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C 78, Armendariz-Picon, Phys. In right panel of Fig. D 96 8 About this article. The resulting BHs might be candidates for seeding the supermassive objects at the center of galaxies [ 9 ].
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|We show that if such a state is a WH, which is slowly pinching off and eventually will collapse into a BHthe ringdown waveform will exhibit a series of echoes, as pointed out in [ 10 ].
Maselli, P. Cite this article Wang, Y. Brady, D. Wang, Y.
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Thus, it is possible that the primordial WHs, created and enlarged in the inflationary phase, might be slowly pinching till today, and merge with another compact object a neutron star or BH.
Bueno, P. The physics of GW echoes has recently been extensively studied, see also [ 293031 ]. Ringdown waveforms of post-merger objects, which correspond to the static and slowly pinching WHs depicted by Fig.
Pa dl 5974
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D 97 2 We plot the corresponding waveforms in Fig. According to Eq. Cardoso, T. Thus in the frequency domain, we can write Eq.
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Yurtsever, Phys. Thus, it is possible that the primordial WHs, created and enlarged in the inflationary phase, might be slowly pinching till today, and merge with another compact object a neutron star or BH.
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|D 44 Considering the expansion.
Maselli, P. The resulting BHs might be candidates for seeding the supermassive objects at the center of galaxies [ 9 ]. Brown, J. Afshordi, arXiv