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dc.contributor.authorGeorgoudis, A
dc.contributor.authorHeissenberg, C
dc.contributor.authorRusso, R
dc.date.accessioned2024-06-13T15:42:10Z
dc.date.available2024-04-26
dc.date.available2024-06-13T15:42:10Z
dc.date.issued2024-05-20
dc.identifier.issn2470-0010
dc.identifier.urihttps://qmro.qmul.ac.uk/xmlui/handle/123456789/97437
dc.description.abstractWe consider the frequency-domain leading order and next-to-leading order post-Minkowskian waveforms obtained from the tree-level and one-loop amplitudes describing the scattering of two massive scalar objects and the emission of one graviton. We explicitly calculate their post-Newtonian (PN) limit obtaining an expansion up to the third subleading PN order in all ingredients: the tree-level amplitude, the odd and even parts of the real one-loop kernel, and the Compton or “rescattering” cuts, thus reaching 3PN precision for the latter. We provide explicit expressions for the multipole decomposition of these results in the center-of-mass frame and compare them with the results obtained from the classical multipolar post-Minkowskian method. We find perfect agreement between the two, once the Bondi-Metzner-Sachs supertranslation frame is properly adjusted and the infrared divergences due to rescattering are suitably subtracted in dimensional regularization. This shows that the approach proposed in Georgoudis et al. [An eikonal-inspired approach to the gravitational scattering waveform, J. High Energy Phys. 03 (2024) 089] can be applied beyond the soft-regime ensuring the agreement between amplitude-based and multipolar post-Minkowskian results for generic frequencies.en_US
dc.format.extent106020 - 106020
dc.publisherAmerican Physical Society (APS)en_US
dc.relation.ispartofPhysical Review D
dc.rightsPublished by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
dc.titlePost-Newtonian multipoles from the next-to-leading post-Minkowskian gravitational waveformen_US
dc.typeArticleen_US
dc.rights.holder© The Author(s) 2024. Published by the American Physical Society
dc.identifier.doi10.1103/physrevd.109.106020
pubs.issue10en_US
pubs.notesNot knownen_US
pubs.publication-statusPublisheden_US
pubs.volume109en_US
dcterms.dateAccepted2024-04-26
rioxxterms.funderDefault funderen_US
rioxxterms.identifier.projectDefault projecten_US
qmul.funderAmplitudes, strings & duality::Science and Technology Facilities Council [2006-2012]en_US
qmul.funderAmplitudes, strings & duality::Science and Technology Facilities Council [2006-2012]en_US
qmul.funderAmplitudes, strings & duality::Science and Technology Facilities Council [2006-2012]en_US
qmul.funderAmplitudes, strings & duality::Science and Technology Facilities Council [2006-2012]en_US


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