Post-Newtonian dynamics of spinning black hole binaries in Einstein-scalar-Gauss-Bonnet gravity

被引：2

作者：

Almeida, Gabriel Luz ^{[1
]}

Zhou, Shuang-Yong ^{[2
]}

机构：

[1] Univ Sci & Technol China, Interdisciplinary Ctr Theoret Study, Hefei 230026, Anhui, Peoples R China

[2] Peng Huanwu Ctr Fundamental Theory, Hefei 230026, Anhui, Peoples R China

来源：

PHYSICAL REVIEW D | 2024年 / 110卷 / 12期

基金：

中国国家自然科学基金;

关键词：

ROTATING RELATIVISTIC STARS; EQUATIONS; FIELD; EXPANSIONS;

D O I：

10.1103/PhysRevD.110.124016

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We explore the post-Newtonian dynamics of spinning black hole (BH) binaries in Einstein-scalar-GaussBonnet (ESGB) gravity, a theory that modifies general relativity by introducing a massless scalar field coupled nonminimally to gravity via the Gauss-Bonnet term. By employing an effective field theory (EFT) approach, we extend the Routhian formalism to incorporate spin effects in scalar interactions. In this formalism, we derive for the first time the effective two-body potential for spinning BHs up to the third post-Newtonian (3PN) order in generic ESGB gravity theories. This potential is expressed in terms of the sensitivities of the BHs, which are then obtained through a matching procedure using analytic BH solutions derived here within a slow-rotation approximation, accurate to seventh order in the Gauss-Bonnet coupling and fifth order in the BH spin. We also examine the thermodynamic properties of these rotating solutions, which, as shown in previous work, yield important insights into the inspiral phase evolution in ESGB gravity.

引用

页数：25

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