Gravitational waveform from radial infall of a particle into a Schwarzschild black hole computed to 3.5 post-Newtonian order.
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NLO angular impulse for Kerr black holes computed to all orders in spin via KMOC formalism and leading singularities, with consistency checks and potential extraction.
Outlines a Schwinger-Keldysh path-integral framework that derives worldline equations of motion and computes weak-field gravitational waveforms independently for unspecified relativistic orbits.
citing papers explorer
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Gravitational waveform from radial infall at the third-and-half Post-Newtonian order
Gravitational waveform from radial infall of a particle into a Schwarzschild black hole computed to 3.5 post-Newtonian order.
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NLO Angular Impulse and Leading Singularities to all orders in spin for Kerr Black Holes
NLO angular impulse for Kerr black holes computed to all orders in spin via KMOC formalism and leading singularities, with consistency checks and potential extraction.
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Weak-field waveforms for generic relativistic orbits
Outlines a Schwinger-Keldysh path-integral framework that derives worldline equations of motion and computes weak-field gravitational waveforms independently for unspecified relativistic orbits.