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pro vyhledávání: '"Watarai, Daiki"'
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Watarai, Daiki
In a binary merger with a small mass ratio, as the secondary body approaches the innermost stable circular orbit (ISCO) of the primary black hole, the motion transitions from the adiabatic inspiral to the plunge governed by the geodesic equation. The
Externí odkaz:
http://arxiv.org/abs/2408.16747
Electromagnetic observations reveal that almost all galaxies have supermassive black holes (SMBHs) at their centers, but their properties, especially their spins, are not fully understood. Some of the authors have recently shown [Oshita and Tsuna (20
Externí odkaz:
http://arxiv.org/abs/2403.12380
The merger phase of compact binary coalescences is the strongest gravity regime that can be observed. To test the validity of general relativity (GR) in strong gravitational fields, we propose a gravitational waveform parameterized for deviations fro
Externí odkaz:
http://arxiv.org/abs/2309.14061
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