Publication Date:
2017-09-02
Description:
Author(s): Kazuki Sakai, Ken-ichi Oohara, Hiroyuki Nakano, Masato Kaneyama, and Hirotaka Takahashi It is known that a quasinormal mode (QNM) of a remnant black hole dominates a ringdown gravitational wave (GW) in a binary black hole (BBH) merger. To study properties of the QNMs, it is important to determine the time when the QNMs appear in a GW signal as well as to calculate its frequency and amp... [Phys. Rev. D 96, 044047] Published Thu Aug 31, 2017
Keywords:
General relativity, alternative theories of gravity
Print ISSN:
0556-2821
Electronic ISSN:
1089-4918
Topics:
Physics