Resummed spinning waveforms from five-point amplitudes
Abstract We compute the classical tree-level five-point amplitude for the two-to-two scattering of spinning celestial objects with the emission of a graviton. Using this five-point amplitude, we then turn to the computation of the leading-order time-domain gravitational waveform. The method we descr...
Váldodahkkit: | Andreas Brandhuber, Graham R. Brown, Gang Chen, Joshua Gowdy, Gabriele Travaglini |
---|---|
Materiálatiipa: | Artihkal |
Giella: | English |
Almmustuhtton: |
SpringerOpen
2024-02-01
|
Ráidu: | Journal of High Energy Physics |
Fáttát: | |
Liŋkkat: | https://doi.org/10.1007/JHEP02(2024)026 |
Geahča maid
-
Spinning waveforms in cubic effective field theories of gravity
Dahkki: Andreas Brandhuber, et al.
Almmustuhtton: (2024-12-01) -
Spinning binary dynamics in cubic effective field theories of gravity
Dahkki: Andreas Brandhuber, et al.
Almmustuhtton: (2024-08-01) -
An eikonal-inspired approach to the gravitational scattering waveform
Dahkki: Alessandro Georgoudis, et al.
Almmustuhtton: (2024-03-01) -
Gravitational Bremsstrahlung in black-hole scattering at O G 3 $$ \mathcal{O}\left({G}^3\right) $$ : linear-in-spin effects
Dahkki: Lara Bohnenblust, et al.
Almmustuhtton: (2024-11-01) -
Dynamics of spinning binary at 2PM
Dahkki: Gang Chen, et al.
Almmustuhtton: (2024-12-01)