Three-Graviton Amplitude in Berkovits-Vafa-Witten Variables
K. Bobkov, L. Dolan

TL;DR
This paper calculates the three-graviton scattering amplitude in Type IIB superstring theory using a novel six-dimensional supersymmetric formalism, analyzing both flat and curved backgrounds.
Contribution
It introduces a method to compute superstring amplitudes in six-dimensional variables, extending previous approaches to include curved backgrounds like AdS3xS3xK3.
Findings
Computed three-graviton amplitude in flat space R6xK3
Extended calculations to curved AdS3xS3xK3 background with flux
Demonstrated the applicability of Berkovits-Vafa-Witten variables in diverse geometries
Abstract
We compute the three-graviton tree amplitude in Type IIB superstring theory compactified to six dimensions using the manifestly (6d) supersymmetric Berkovits-Vafa-Witten worldsheet variables. We consider two cases of background geometry: the flat space example R6xK3, and the curved example AdS3xS3xK3 with Ramond flux, and compute the correlation functions in the bulk.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Pulsars and Gravitational Waves Research
