Theory-Agnostic Constraints on Black-Hole Dipole Radiation with Multiband Gravitational-Wave Astrophysics

被引:143
作者
Barausse, Enrico [1 ,2 ]
Yunes, Nicolas [3 ]
Chamberlain, Katie [3 ]
机构
[1] Sorbonne Univ, Univ Paris 06, 98 Bis Bd Arago, F-75014 Paris, France
[2] CNRS, UMR 7095, Inst Astrophys Paris, 98 Bis Bd Arago, F-75014 Paris, France
[3] Montana State Univ, Dept Phys, eXtreme Grav Inst, Bozeman, MT 59717 USA
基金
美国国家科学基金会; 欧盟地平线“2020”;
关键词
RELATIVISTIC GRAVITY; SCALAR THEORIES; BINARY; FIELD; PRINCIPLE; TESTS;
D O I
10.1103/PhysRevLett.116.241104
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The aLIGO detection of the black-hole binary GW150914 opens a new era for probing extreme gravity. Many gravity theories predict the emission of dipole gravitational radiation by binaries. This is excluded to high accuracy in binary pulsars, but entire classes of theories predict this effect predominantly ( or only) in binaries involving black holes. Joint observations of GW150914-like systems by aLIGO and eLISA will improve bounds on dipole emission from black-hole binaries by 6 orders of magnitude relative to current constraints, provided that eLISA is not dramatically descoped.
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页数:6
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