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Lorenz gauge gravitational self-force calculations of eccentric binaries using a frequency domain procedure

2014
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Physical Review D
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We present an algorithm for calculating the metric perturbations and gravitational self-force for extreme-mass-ratio inspirals (EMRIs) with eccentric orbits. The massive black hole is taken to be Schwarzschild and metric perturbations are computed in Lorenz gauge. The perturbation equations are solved as coupled systems of ordinary differential equations in the frequency domain. Accurate local behavior of the metric is attained through use of the method of extended homogeneous solutions and

doi:10.1103/physrevd.90.104031
fatcat:quaewsbicnecpeqtddbocohkiu