High post-Newtonian order gravitational self-force analytical results for eccentric equatorial orbits around a Kerr black hole

被引：26

作者：

Bini, Donato ^{[1
]}

Damour, Thibault ^{[2
]}

Geralico, Andrea ^{[1
]}

机构：

[1] CNR, Ist Applicazioni Calcolo M Picone, I-00185 Rome, Italy

[2] Inst Hautes Etud Sci, 35 Route Chartres, F-91440 Bures Sur Yvette, France

来源：

PHYSICAL REVIEW D | 2016年 / 93卷 / 12期

关键词：

EQUATION;

D O I：

10.1103/PhysRevD.93.124058

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the first analytic computation of the Detweiler-Barack-Sago gauge-invariant redshift function for a small mass in eccentric equatorial orbit around a spinning black hole. Our results give the redshift contributions that mix eccentricity and spin effects, through second order in eccentricity, second order in spin parameter, and the eight-and-a-half post-Newtonian order.

引用

页数：13

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