Sound Speed Resonance of the Stochastic Gravitational-Wave Background

被引:36
|
作者
Cai, Yi-Fu [1 ,2 ,3 ]
Lin, Chunshan [4 ]
Wang, Bo [1 ,2 ,3 ]
Yan, Sheng-Feng [1 ,2 ,3 ]
机构
[1] Univ Sci & Technol China, Sch Phys Sci, Dept Astron, Hefei 230026, Anhui, Peoples R China
[2] Univ Sci & Technol China, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China
[3] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Anhui, Peoples R China
[4] Jagiellonian Univ, Fac Phys Astron & Appl Comp Sci, PL-30348 Krakow, Poland
基金
中国博士后科学基金;
关键词
PARTICLES; EQUATIONS;
D O I
10.1103/PhysRevLett.126.071303
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We propose a novel mechanism to test time variation of the propagation speed of gravitational waves (GWs) in light of GWs astronomy. As the stochastic GWs experience the whole history of cosmic expansion, they encode potential observational evidence of such variation. We report that, one feature of a varying GWs speed is that the energy spectrum of GWs will present resonantly enhanced peaks if the GWs speed oscillates in time at high-energy scales. Such oscillatory behavior arises in a wide class of modified gravity theories. The amplitude of these peaks can be at reach by current and forthcoming GWs instruments, hence making the underlying theories falsifiable. This mechanism reveals that probing the variation of GWs speed can be a promising way to search for new physics beyond general relativity.
引用
收藏
页数:6
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