Summing up D-instantons in N=2 supergravity

TL;DR

This paper investigates the non-perturbative quantum geometry of the Universal Hypermultiplet in N=2 supergravity, calculating D-instanton contributions and their effects on the moduli space and scalar potential.

Contribution

It derives a unique non-perturbative pre-potential for the UH metric incorporating D-instanton effects, matching the Eisenstein series and proving cluster decomposition.

Findings

The non-perturbative pre-potential matches the Eisenstein series of Green and Gutperle.

The pre-potential interpolates between perturbative and superconformal regions.

Cluster decomposition of D-instantons in curved spacetime is proven.

Abstract

The non-perturbative quantum geometry of the Universal Hypermultiplet (UH) is investigated in N=2 supergravity. The UH low-energy effective action is given by the four-dimensional quaternionic non-linear sigma-model having an U(1)xU(1) isometry. The UH metric is governed by the single real pre-potential that is an eigenfunction of the Laplacian in the hyperbolic plane. We calculate the classical pre-potential corresponding to the standard (Ferrara-Sabharwal) metric of the UH arising in the Calabi-Yau compactification of type-II superstrings. The non-perturbative quaternionic metric, describing the D-instanton contributions to the UH geometry, is found by requiring the SL(2,Z) modular invariance of the UH pre-potential. The pre-potential found is unique, while it coincides with the D-instanton function of Green and Gutperle, given by the order-3/2 Eisenstein series. As a by-product, we prove cluster decomposition of D-instantons in curved spacetime. The non-perturbative UH pre-potential interpolates between the perturbative (large CY volume) region and the superconformal (Landau-Ginzburg) region in the UH moduli space. We also calculate a non-perturbative scalar potential in the hyper-K"ahler limit, when an abelian isometry of the UH metric is gauged in the presence of D-instantons.