BMS Supertranslation Symmetry Implies Faddeev-Kulish Amplitudes
Sangmin Choi, Ratindranath Akhoury
TL;DR
This work shows that infrared-finite scattering amplitudes in perturbative gravity emerge when one imposes conservation of the BMS supertranslation charges. By constructing eigenstates of the soft graviton charge and analyzing how graviton clouds dress external particles, the authors prove that any charge-conserving amplitude is equivalent to a Faddeev-Kulish amplitude, effectively moving soft clouds across the scattering operator without changing IR properties. They demonstrate clouds weakly commute with the S-matrix and establish the precise equality M = M_c = M_FK, linking asymptotic symmetries to IR finiteness. The analysis is applied to decoherence studies, arguing that while a naive tracing over soft degrees can yield decoherence, the properly dressed FK framework yields IR-finite density matrices with well-defined diagonal elements. The results suggest a deep connection between asymptotic symmetries and the infrared structure of gravity, with potential extensions to QED and QCD.
Abstract
We show explicitly that, among the scattering amplitudes constructed from eigenstates of the BMS supertranslation charge, the ones that conserve this charge, are equal to those constructed from Faddeev-Kulish states. Thus, Faddeev-Kulish states naturally arise as a consequence of the asymptotic symmetries of perturbative gravity and all charge conserving amplitudes are infrared finite. In the process we show an important feature of the Faddeev-Kulish clouds dressing the external hard particles: these clouds can be moved from the incoming states to the outgoing ones, and vice-versa, without changing the infrared finiteness properties of S matrix elements. We also apply our discussion to the problem of the decoherence of momentum configurations of hard particles due to soft boson effects.
