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    Radial fall: The gravitational waveform up to the second-and-half post-Newtonian order

    Donato Bini1 and Giorgio Di Russo2

    Phys. Rev. D 114, 064068 – Published 21 September, 2026

    DOI: https://doi.org/10.1103/6x3q-pdz4

    Abstract

    We consider an application of the multipolar post-Minkowskian formalism to the case of a two-body system in radial fall. We compute, within the post-Newtonian approximation, the associated gravitational waveform reaching the 2.5 post-Newtonian accuracy level. At this level the presence of a radiation-reaction force manifests, modifying the fall with a corresponding bremsstrahlung radiation. We evaluate then all emissions: energy, angular momentum (vanishing identically), and linear momentum. We also evaluate the (nonlocal) inertial forces contributions appearing (at the next PN order, 4.5PN) in the center-of-mass due to the losses paving the way for future more accurate computations.

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    See Also

    Gravitational waveform from radial infall at the third-and-half post-Newtonian order

    Giorgio Di Russo and Donato Bini
    Phys. Rev. D 114, 064069 (2026)

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