{
  "abstract": "Gravitational observables for binary systems exhibit a simple polynomial dependence on the masses m 1 , m 2 of the two scattering objects when they are written in terms of the appropriate kinematic variables in the post-Minkowskian (PM) regime. We point out that this property, combined with particle interchange symmetry, allows one to reconstruct the leading and subleading PM waveforms from their probe limit, m 1 ≫ m 2 . As an application, focusing on their re-expansion in the small-velocity or post-Newtonian (PN) regime, we calculate the probe-limit waveforms up to 10PN, and then exploit this observation to deduce from them the waveforms for generic masses in the center-of-mass frame up to 5PN. To this end, we employ both the amplitude-based waveform integrands and the tail formula. This combined approach simplifies substantially the PN expansion of the full subleading PM waveform.",
  "abstract_shown": true,
  "affiliations": [
    "Institut de Physique Théorique, CEA Saclay, CNRS, Université Paris-Saclay, Gif-sur-Yvette, Cedex, F-91191, France",
    "IPHT - Institut de Physique Théorique - UMR CNRS 3681 (Institut de Physique Théorique Orme des Merisiers batiment 774 Point courrier 136 CEA/DSM/IPhT CEA/Saclay F-91191 Gif-sur-Yvette Cedex - France)",
    "School of Mathematical Sciences, Queen Mary University of London, Mile End Road, London, E1 4NS, United Kingdom"
  ],
  "article_type": null,
  "arxiv": null,
  "author_total": 2,
  "authors": [
    {
      "affs": [
        0,
        1
      ],
      "name": "Carlo Heissenberg",
      "orcid": "0000-0001-5775-9526"
    },
    {
      "affs": [
        2
      ],
      "name": "Rodolfo Russo",
      "orcid": "0000-0003-4732-6369"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/68z58zr1h5dh7.bib",
  "cited_by": 9,
  "doi": "10.1016/j.nuclphysb.2026.117538",
  "fulltext_url": null,
  "id": "68z58zr1h5dh7",
  "issns": [
    "0550-3213",
    "1873-1562"
  ],
  "landing_url": "https://doi.org/10.1016/j.nuclphysb.2026.117538",
  "language": "en",
  "licence": "CC-BY",
  "licence_label": "CC BY",
  "licence_source": "journal",
  "licence_url": "https://creativecommons.org/licenses/by/4.0/",
  "metadata_licence": null,
  "native_subjects": [
    [
      "openalex",
      "3103|Pulsars and Gravitational Waves Research"
    ]
  ],
  "openalex": "W4416964982",
  "pdf_url": null,
  "pmcid": null,
  "pmid": null,
  "published": "2026-06-01",
  "publisher": "Elsevier BV",
  "ris": "https://research.draconitic.com/paper/68z58zr1h5dh7.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T13:26:43Z",
      "native_id": "W4416964982",
      "source": "openalex",
      "url": "https://doi.org/10.1016/j.nuclphysb.2026.117538"
    }
  ],
  "subjects": [
    {
      "field": "astronomy",
      "origin": "openalex:3103|Pulsars and Gravitational Waves Research",
      "subfield": "high-energy-astrophysics"
    }
  ],
  "title": "Reconstructing the gravitational waveform from its probe limit",
  "title_text": "Reconstructing the gravitational waveform from its probe limit",
  "type": "peer-reviewed",
  "updated_at": "2026-11-06T13:20:25Z",
  "url": "https://research.draconitic.com/paper/68z58zr1h5dh7",
  "venue": "Nuclear Physics B",
  "versions": []
}