Can we detect quantum gravity with compact binary inspirals?

被引：6

作者：

Jenkins, Alexander C. ^{[1
]}

Pithis, Andreas G. A. ^{[1
]}

Sakellariadou, Mairi ^{[1
]}

机构：

[1] Univ London, Kings Coll London, Phys Dept, Theoret Particle Phys & Cosmol Grp, London WC2R 2LS, England

来源：

PHYSICAL REVIEW D | 2018年 / 98卷 / 10期

关键词：

GRAVITATIONAL COLLAPSE; NONRENORMALIZABILITY; SINGULARITIES;

D O I：

10.1103/PhysRevD.98.104032

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Treating general relativity as an effective field theory, we compute the leading-order quantum corrections to the orbits and gravitational-wave emission of astrophysical compact binaries. These corrections are independent of the (unknown) nature of quantum gravity at high energies, and generate a phase shift and amplitude increase in the observed gravitational-wave signal. Unfortunately (but unsurprisingly), these corrections are undetectably small, even in the most optimistic observational scenarios.

引用

页数：7

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