Inelastic exponentiation and classical gravitational scattering at one loop

Author:

Georgoudis AlessandroORCID,Heissenberg CarloORCID,Vazquez-Holm IngridORCID

Abstract

Abstract We calculate the inelastic 2 → 3 one-loop amplitude for the scattering of two point-like, spinless objects with generic masses involving the additional emission of a single graviton. We focus on the near-forward, or classical, limit. Our results include the leading and subleading orders in the soft-region expansion, which captures all non-analytic contributions in the transferred momentum and in the graviton’s frequency. This allows us to check the first constraint arising from the inelastic exponentiation put forward in refs. [1–3], and to calculate the 2 → 3 one-loop matrix element of the N-operator, linked to the S-matrix by S = eiN, showing that it is real, classical and free of infrared divergences. We discuss how our results feature in the calculation of the $$ \mathcal{O} $$ O (G3) corrections to the asymptotic waveform.

Publisher

Springer Science and Business Media LLC

Subject

Nuclear and High Energy Physics

Reference106 articles.

1. P.H. Damgaard, L. Plante and P. Vanhove, On an exponential representation of the gravitational S-matrix, JHEP 11 (2021) 213 [arXiv:2107.12891] [INSPIRE].

2. A. Cristofoli et al., The Uncertainty Principle and Classical Amplitudes, arXiv:2112.07556 [INSPIRE].

3. P. Di Vecchia, C. Heissenberg, R. Russo and G. Veneziano, Classical Gravitational Observables from the Eikonal Operator, arXiv:2210.12118 [INSPIRE].

4. LIGO Scientific et al. collaborations, GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run, arXiv:2111.03606 [INSPIRE].

5. A. Buonanno et al., Snowmass White Paper: Gravitational Waves and Scattering Amplitudes, in the proceedings of the 2021 Snowmass Summer Study, (2022) [arXiv:2204.05194] [INSPIRE].

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