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.
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页数：13
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