Extreme gravity tests with gravitational waves from compact binary coalescences: (I) inspiral-merger

被引:192
|
作者
Berti, Emanuele [1 ]
Yagi, Kent [2 ]
Yunes, Nicolas [3 ]
机构
[1] Univ Mississippi, Dept Phys & Astron, University, MS 38677 USA
[2] Univ Virginia, Dept Phys, Charlottesville, VA 22904 USA
[3] Montana State Univ, Dept Phys, eXtreme Grav Inst, Bozeman, MT 59717 USA
基金
美国国家科学基金会;
关键词
Modified gravity; Gravitational waves; Compact binary systems; ROTATING BLACK-HOLE; MODIFIED DISPERSION-RELATIONS; PREFERRED-FRAME THEORIES; RELATIVISTIC GRAVITY; GENERAL-RELATIVITY; EQUIVALENCE PRINCIPLE; CONSERVATION-LAWS; SCALAR THEORIES; MASSIVE BODIES; CAUCHY-PROBLEM;
D O I
10.1007/s10714-018-2362-8
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The observation of the inspiral and merger of compact binaries by the LIGO/Virgo collaboration ushered in a new era in the study of strong-field gravity. We review current and future tests of strong gravity and of the Kerr paradigm with gravitational-wave interferometers, both within a theory-agnostic framework (the parametrized post-Einsteinian formalism) and in the context of specific modified theories of gravity (scalar-tensor, Einstein-dilaton-Gauss-Bonnet, dynamical Chern-Simons, Lorentz-violating, and extra dimensional theories). In this contribution we focus on (i) the information carried by the inspiral radiation, and (ii) recent progress in numerical simulations of compact binary mergers in modified gravity.
引用
收藏
页数:45
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