SAIFR:4496

Post-Newtonian observables for aligned-spin binaries from gravitational self-force and Compton amplitudes

(2024). Post-Newtonian observables for aligned-spin binaries from gravitational self-force and Compton amplitudes. ICTP South American Institute for Fundamental Research. https://scivideos.org/ictp-saifr/4496

Post-Newtonian observables for aligned-spin binaries from gravitational self-force and Compton amplitudes. ICTP South American Institute for Fundamental Research, Aug. 14, 2024, https://scivideos.org/ictp-saifr/4496 

          @misc{ scivideos_SAIFR:4496,
            doi = {},
            url = {https://scivideos.org/ictp-saifr/4496},
            author = {},
            keywords = {ICTP-SAIFR, IFT, UNESP},
            language = {en},
            title = {Post-Newtonian observables for aligned-spin binaries from gravitational self-force and Compton amplitudes},
            publisher = { ICTP South American Institute for Fundamental Research},
            year = {2024},
            month = {aug},
            note = {SAIFR:4496 see, \url{https://scivideos.org/ictp-saifr/4496}}
          }
Fabian Bautista
Talk numberSAIFR:4496
Source RepositoryICTP – SAIFR
Collection
Talk Type Conference
Subject

Abstract

Accurate modeling of compact binaries is essential for gravitational-wave detection and parameter estimation, with spin being an importante effect to include in waveform models. In this seminar, I will show how to derive new post-Newtonian (PN) results for the conservative aligned-spin dynamics at next-to-next-to-leading order for the spin3 and spin4 contributions, in addition to the next-to-leading order (NLO) spin5 and spin6 contributions. One approach we follow is the Tutti Frutti method, which relates PN and gravitational self-force (GSF) results through the redshift and spin-precession invariants, by making use of the simple dependence of the scattering angle on the binary mass ratio. However, an ambiguity arises at the NLO spin5 contribution, due to transcendental functions of the Kerr spin in the redshift; this is also the order at which Compton amplitudes calculations are affected by spurious poles. Therefore, we discuss an additional approach to determine the NLO spin5 and spin6 dynamics: using on-shell Compton amplitudes dictated by homogeneous solutions of the Teukolsky equation, the later solved non-perturbative in terms of the Nekrasov-Shatashvili Function.