Radiative classical gravitational observables at O ( G 3 ) from scattering amplitudes
Radiative classical gravitational observables at O ( G 3 ) from scattering amplitudes
复制标题
来自散射振幅的 O ( G 3 ) 处的辐射经典引力可观测量
DOI:
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发表时间:
2021
期刊:
影响因子:
--
通讯作者:
M. Zeng
中科院分区:
文献类型:
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作者:
Enrico Herrmann;Julio Parra;M. Zeng
We compute classical gravitational observables for the scattering of two spinless black holes in general relativity and N=8 supergravity in the formalism of Kosower, Maybee, and O’Connell (KMOC). We focus on the gravitational impulse with radiation reaction and the radiated momentum in black hole scattering at O(G3) to all orders in the velocity. These classical observables require the construction and evaluation of certain loop-level quantities which are greatly simplified by harnessing recent advances from scattering amplitudes and collider physics. In particular, we make use of generalized unitarity to construct the relevant loop integrands, employ reverse unitarity, the method of regions, integration-by-parts (IBP), and (canonical) differential equations to simplify and evaluate all loop and phase-space integrals to obtain the classical gravitational observables of interest to two-loop order. The KMOC formalism naturally incorporates radiation effects which enables us to explore these classical quantities beyond the conservative two-body dynamics. From the impulse and the radiated momentum, we extract the scattering angle and the radiated energy. Finally, we discuss universality of the impulse in the high-energy limit and the relation to the eikonal phase.
影响因子:
5.4
作者:
D. Kosower;Ben Maybee;D. O’Connell
通讯作者:
D. Kosower;Ben Maybee;D. O’Connell
影响因子:
8.6
作者:
Abbott, B. P.;Abbott, R.;Zweizig, J.
通讯作者:
Zweizig, J.