论文标题
在下午2点搜索Kerr
Searching for Kerr in the 2PM amplitude
论文作者
论文摘要
旋转物体的经典散射由重型颗粒的纺纱形形式形式很好地描述。使用这些变量,我们得出了无虚拟的,全旋转相反的康普顿幅度(将物理杆分解为最小的,全旋转的三分三分幅度,参考\ cite {arkani-hamed:2017jhn}),以qED,qcd,qccd,qcd,grattity的经典限制。固化的振幅可能会通过接触术语进行变形,这是我们可以通过在第二次后 - 康科夫斯基(下午2点)下施加旋转结构之间的关系来解决的绝大多数贡献。对于QED和重力,这留下了适度数量的未连接系数参数化接触期变形,而QCD幅度则是唯一确定的。我们的重力康普顿振幅使我们能够将旋转2pm散射的最新散射推向两个物体的自旋矢量中的任何顺序。我们在此处和辅助文件\ texttt {2 pmspin8aux.nb}中介绍结果,最高为旋转矢量中的第八阶。有趣的是,尽管康普顿振幅中剩余的系数剩下的系数,但在旋转结构之间施加了上述关系,但唯一地固定了下午2点振幅的一些高旋转部分。
The classical scattering of spinning objects is well described by the spinor-helicity formalism for heavy particles. Using these variables, we derive spurious-pole-free, all-spin opposite-helicity Compton amplitudes (factorizing on physical poles to the minimal, all-spin three-point amplitudes of ref. \cite{Arkani-Hamed:2017jhn}) in the classical limit for QED, QCD, and gravity. The cured amplitudes are subject to deformations by contact terms, the vast majority of whose contributions we can fix by imposing a relation between spin structures -- motivated by lower spin multipoles of black hole scattering -- at the second post-Minkowskian (2PM) order. For QED and gravity, this leaves a modest number of unfixed coefficients parametrizing contact-term deformations, while the QCD amplitude is uniquely determined. Our gravitational Compton amplitude allows us to push the state-of-the-art of spinning-2PM scattering to any order in the spin vectors of both objects; we present results here and in the auxiliary file \texttt{2PMSpin8Aux.nb} up to eighth order in the spin vectors. Interestingly, despite leftover coefficients in the Compton amplitude, imposing the aforementioned relation between spin structures uniquely fixes some higher-spin parts of the 2PM amplitude.