All-orders moduli for type II flux backgrounds
George R. Smith, David Tennyson, Daniel Waldram

TL;DR
This paper develops an exact method using generalised geometry to determine the bulk moduli of type II string theory flux backgrounds, accounting for finite flux, higher-derivative corrections, and obstructions, with implications for the tadpole conjecture.
Contribution
It introduces a spectral sequence approach that precisely counts infinitesimal deformations of SU(3)-structure flux backgrounds, extending beyond linear approximations and including higher-order effects.
Findings
Spectral sequence reproduces naive superpotential expectations.
All obstructions vanish due to a Tian–Todorov-like lemma.
Perturbative higher-order effects do not bypass the tadpole bound.
Abstract
We investigate the old problem of determining the exact bulk moduli of generic -structure flux backgrounds of type II string theory. Using techniques from generalised geometry, we show that the infinitesimal deformations are counted by a spectral sequence in which the vertical maps are either de Rham or Dolbeault differentials (depending on the type of the exceptional complex structure (ECS)) and the horizontal maps are linear maps constructed from the flux and intrinsic torsion. Our calculation is exact, covering all possible supergravity -structure flux backgrounds including those which are not conformally Calabi--Yau, and goes beyond the usual linear approximation in three important ways: (i) we allow for finite flux; (ii) we consider perturbative higher-derivative corrections to the supergravity action; and (iii) we consider obstructions arising from…
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Taxonomy
TopicsSeismic Imaging and Inversion Techniques
