Accelerated motion and the self-force in Schwarzschild spacetime

被引:11
|
作者
Heffernan, Anna [1 ,2 ,3 ]
Ottewill, Adrian C. [2 ]
Warburton, Niels [2 ]
Wardell, Barry [2 ]
Diener, Peter [4 ,5 ]
机构
[1] Univ Florida, Dept Phys, 2001 Museum Rd, Gainesville, FL 32611 USA
[2] Univ Coll Dublin, Sch Math & Stat, Dublin 4, Ireland
[3] ESA, European Space Res & Technol Ctr ESTEC, Adv Concepts Team, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands
[4] Louisiana State Univ, Ctr Computat & Technol, Baton Rouge, LA 70803 USA
[5] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA
基金
欧盟地平线“2020”; 爱尔兰科学基金会; 美国国家科学基金会;
关键词
self-force; gravitational waves source modelling; accelerated motion; black holes; mode-sum; effectives source; GRAVITATIONAL-RADIATION REACTION; GENERAL-RELATIVITY; BLACK-HOLES; BINARY; PARTICLES; COLLAPSE; FIELD;
D O I
10.1088/1361-6382/aad420
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We provide expansions of the Detweiler-Whiting singular field for a particle with a scalar field moving along arbitrary, planar accelerated trajectories in Schwarzschild spacetime. We transcribe these results into mode-sum regularization parameters, computing previously unknown terms that increase the convergence rate of the mode-sum. We test our results by computing the self-force along a variety of accelerated trajectories. For non-uniformly accelerated circular orbits we present results from a new 1+1D discontinuous Galerkin time-domain code which employs an effective source. We also present results for uniformly accelerated circular orbits and accelerated bound eccentric orbits computed within a frequency-domain treatment. Our regularization results will be useful for computing self-consistent self-force inspirals where the particle's worldline is accelerated with respect to the background spacetime.
引用
收藏
页数:30
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