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The major source of ground-based gravitational wave detectors, the inspiral and merger of comparable mass binary black holes (BBH), consists of a slow quasicircular inspiral, a merger to form a single remnant hole, and the quasinormal ringing of that
Externí odkaz:
http://arxiv.org/abs/2312.15885
Autor:
Price, Richard, Price, Sally
Publikováno v:
NWIG: New West Indian Guide / Nieuwe West-Indische Gids, 2024 Jan 01. 98(1/2), 93-129.
Externí odkaz:
https://www.jstor.org/stable/27297095