Log-periodic gravitational-wave background beyond Einstein gravity

被引:2
|
作者
Calcagni, Gianluca [1 ]
Kuroyanagi, Sachiko [2 ,3 ]
机构
[1] CSIC, Inst Estruct Mat, Serrano 121, Madrid 28006, Spain
[2] Univ Autonoma Madrid, Inst Fis Teor UAM, CSIC, Madrid 28049, Spain
[3] Nagoya Univ, Dept Phys, Nagoya 4648602, Japan
基金
日本学术振兴会;
关键词
stochastic background; log oscillations; quantum gravity; alternative gravity theories; PERTURBATIONS;
D O I
10.1088/1361-6382/ad1123
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Periodic patterns of logarithmic oscillations can arise in primordial curvature perturbation spectra and in the associated gravitational-wave background via different mechanisms. We show that, in the presence of log oscillations, the spectral shape of the stochastic background has a unique parametrization independent of its physical origin. We also show that this log-periodic modulation can be generated in any scenario beyond Einstein gravity endowed with an approximate discrete scale invariance, a symmetry typical of deterministic fractal spacetimes that could emerge in quantum gravity under certain conditions. We discuss how a log-oscillatory spectral shape arises from concrete inflationary models beyond Einstein gravity and the prospects for detection in Einstein Telescope and other next-generation gravitational-wave observatories. We find that these instruments will be sensitive to log-periodic features if the detection is made with a high signal-to-noise ratio (SNR) and that the error scales as 1/SNR .
引用
收藏
页数:26
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