Gravitational self-force corrections to tidal invariants for particles on circular orbits in a Kerr spacetime

被引:5
作者
Bini, Donato [1 ]
Geralico, Andrea [1 ]
机构
[1] CNR, Ist Applicaz Calcolo M Picone, I-00185 Rome, Italy
关键词
RELATIVISTIC CELESTIAL MECHANICS; TEUKOLSKY EQUATION; ANALYTIC SOLUTIONS; PERTURBATIONS;
D O I
10.1103/PhysRevD.98.064040
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We generalize to the Kerr spacetime existing self-force results on tidal invariants for particles moving along circular orbits around a Schwarzschild black hole. We obtain linear-in-mass-ratio (conservative) corrections to the quadratic and cubic electric-type invariants and the quadratic magnetic-type invariant in series of the rotation parameter up to the fourth order and through the ninth and eighth post-Newtonian orders, respectively. We then analytically compute the associated eigenvalues of both electric and magnetic tidal tensors.
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收藏
页数:12
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[31]   Confirming and improving post-Newtonian and effective-one-body results from self-force computations along eccentric orbits around a Schwarzschild black hole [J].
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Damour, Thibault ;
Geralico, Andrea .
PHYSICAL REVIEW D, 2016, 93 (06)
[32]   Post-Newtonian observables for aligned-spin binaries to sixth order in spin from gravitational self-force and Compton amplitudes [J].
Bautista, Yilber Fabian ;
Khalil, Mohammed ;
Sergola, Matteo ;
Kavanagh, Chris ;
Vines, Justin .
PHYSICAL REVIEW D, 2024, 110 (12)
[33]   Analytic determination of the eight-and-a-half post-Newtonian self-force contributions to the two-body gravitational interaction potential [J].
Bini, Donato ;
Damour, Thibault .
PHYSICAL REVIEW D, 2014, 89 (10)