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Frequency-domain approach to self-force in hyperbolic scattering

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arxiv 2305.09724 v2 pith:AFL3NIXE submitted 2023-05-16 gr-qc astro-ph.HEhep-th

classification gr-qcastro-ph.HEhep-th
keywords self-forcefrequency-domainmethodscatteringexistingaccountactingangle
verification ladder T0 review T1 audit T2 compute T3 formal
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We develop a frequency-domain method for calculating the self-force acting on a scalar charge on a fixed scattering geodesic in Schwarzschild spacetime. Existing frequency-domain methods, which are tailored for bound orbits, are inadequate here for several reasons. One must account for the continuous spectrum in the scattering problem, deal with slowly-convergent radial integrals that are hard to evaluate numerically, and confront the inapplicability of the standard self-force method of "extended homogeneous solutions", which only works for compactly supported sources. We tackle each of these issues in turn, and then present a full numerical implementation, in which we calculate the self-force correction to the scatter angle due to scalar-field back-reaction. We perform a range of internal validation tests, as well as ones based on comparison with existing time-domain results. We discuss the merits and remaining limitations of our method, and outline directions for future work.

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Cited by 2 Pith papers

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  1. Time-domain framework for the Teukolsky equation with a particle source using comoving hyperboloidal coordinates

    gr-qc 2026-06 unverdicted novelty 6.0 of 10

    A time-domain numerical framework for the Teukolsky equation with particle sources in comoving compactified hyperboloidal coordinates that avoids nonphysical growing modes.

  2. Gravitational radiation from hyperbolic orbits: comparison between self-force, post-Minkowskian, post-Newtonian, and numerical relativity results

    gr-qc 2025-12 unverdicted novelty 5.0 of 10

    Self-force calculations of radiated gravitational wave energy from hyperbolic orbits around Schwarzschild black holes agree with post-Minkowskian results for large impact parameters and velocities up to 0.7c, with fur...

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