Advances in Theoretical and Mathematical Physics

Volume 27 (2023)

Number 3

Twistor sigma models for quaternionic geometry and graviton scattering

Pages: 623 – 681

DOI: https://dx.doi.org/10.4310/ATMP.2023.v27.n3.a1

Authors

Tim Adamo (School of Mathematics and Maxwell Institute for Mathematical Sciences, University of Edinburgh, Scotland, United Kingdom)

Lionel Mason (Mathematical Institute, University of Oxford, United Kingdom)

Atul Sharma (Center for the Fundamental Laws of Nature, and the Black Hole Initiative, Harvard University, Cambridge, Massachusetts, U.S.A.)

Abstract

We reformulate the twistor construction for hyper- and quaternion-Kähler manifolds, introducing new sigma models that compute scalar potentials for the geometry. These sigma models have the twistor space of the quaternionic manifold as their target and encode finite non-linear perturbations of the flat structures. In the hyperkähler case our twistor sigma models compute both Plebanski fundamental forms (including the Kähler potential), while in the quaternion-Kähler setting the twistor sigma model computes the Kähler potential for the hyperkähler structure on non-projective twistor space.

In four-dimensions, one of the models provides the generating functional of tree-level MHV graviton scattering amplitudes; perturbations of the hyperkähler structure corresponding to positive helicity gravitons. The sigma model’s perturbation theory gives rise to a sum of tree diagrams observed previously in the literature, and their summation via a matrix tree theorem gives a firstprinciples derivation of Hodges’ formula for MHV graviton amplitudes directly from general relativity. We generalise the twistor sigma model to higher-degree (defined in the first case with a cosmological constant), giving a new generating principle for the full tree-level graviton S-matrix.

Published 6 June 2024