Nonlinear Effects in Black Hole Ringdown

被引:74
作者
Cheung, Mark Ho-Yeuk [1 ]
Baibhav, Vishal [2 ,3 ]
Berti, Emanuele [1 ]
Cardoso, Vitor [4 ,5 ]
Carullo, Gregorio [6 ]
Cotesta, Roberto [1 ]
Del Pozzo, Walter [7 ]
Duque, Francisco [5 ]
Helfer, Thomas [1 ]
Shukla, Estuti [8 ]
Wong, Kaze W. K. [9 ]
机构
[1] Johns Hopkins Univ, William H Miller III Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USA
[2] Northwestern Univ, Ctr Interdisciplinary Explorat & Res Astrophys CIE, 1800 Sherman Ave, Evanston, IL 60201 USA
[3] Northwestern Univ, Dept Phys & Astron, 1800 Sherman Ave, Evanston, IL 60201 USA
[4] Niels Bohr Int Acad, Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
[5] Univ Lisboa UL, Inst Super Tecn IST, Dept Fis, CENTRA, Ave Rovisco Pais 1, P-1049001 Lisbon, Portugal
[6] Friedrich Schiller Univ Jena, Theoret Phys Inst, Frobelstieg 1, D-07743 Jena, Germany
[7] Univ Pisa, Dipartimento Fis Enrico Fermi, I-56127 Pisa, Italy
[8] Penn State Univ, Inst Gravitat & Cosmos, Dept Phys, University Pk, PA 16802 USA
[9] Flatiron Inst, Ctr Computat Astrophys, New York, NY 10010 USA
基金
美国国家科学基金会; 欧盟地平线“2020”;
关键词
EXTREME GRAVITY TESTS; GRAVITATIONAL-WAVES; PERTURBATIONS; RELATIVITY;
D O I
10.1103/PhysRevLett.130.081401
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We report evidence for nonlinear modes in the ringdown stage of the gravitational waveform produced by the merger of two comparable-mass black holes. We consider both the coalescence of black hole binaries in quasicircular orbits and high-energy, head-on black hole collisions. The presence of nonlinear modes in the numerical simulations confirms that general-relativistic nonlinearities are important and must be considered in gravitational-wave data analysis.
引用
收藏
页数:6
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