Classical observables from the exponential representation of the gravitational S-matrix

被引:0
|
作者
Poul H. Damgaard
Elias Roos Hansen
Ludovic Planté
Pierre Vanhove
机构
[1] University of Copenhagen,Niels Bohr International Academy, Niels Bohr Institute
[2] Theoretical Physics Department,undefined
[3] CERN,undefined
[4] Institut de Physique Theorique,undefined
[5] Université Paris-Saclay,undefined
[6] CEA,undefined
[7] CNRS,undefined
关键词
Classical Theories of Gravity; Scattering Amplitudes; Effective Field Theories;
D O I
暂无
中图分类号
学科分类号
摘要
By combining the KMOC-formalism with the exponential representation of the scattering matrix we show that the two-body scattering angle is given by the corresponding matrix element of the exponential representation. This holds to all orders in the Post-Minkowskian expansion of gravity when restricted to the conservative sector. Once gravitational radiation is taken into account new terms correcting this relationship appear starting at fourth Post-Minkowskian order. A systematic expansion of the momentum kick is provided to any order, thus illustrating the iterative structure that partly recycles terms from lower orders in the Post-Minkowskian expansion. We provide explicit results for this computation to fourth Post-Minkowskian order, the first complete calculation at this order based on scattering amplitudes.
引用
收藏
相关论文
共 50 条