Abstract

We identify the low-energy K\"ahler potential of warped F-theory/IIB flux compactifications whose light spectrum includes universal, K\"ahler, axionic and mobile D3-brane moduli. The derivation is based on four-dimensional local superconformal symmetry and holomorphy of brane instanton contributions and it reproduces and generalises previous partial results. We compute the resulting kinetic terms, which show their explicit dependence on the warping. The K\"ahler potential satisfies the no-scale condition and produces, at leading order in the large volume expansion, a specific correction to the unwarped K\"ahler potential.

Highlights

  • Background structureLet us review the structure of warped F-theory/IIB compactifications, by using the type IIB description of these vacua [3,4,5,6]

  • We identify the low-energy Kahler potential of warped F-theory/IIB flux compactifications whose light spectrum includes universal, Kahler, axionic and mobile D3-brane moduli

  • The derivation is based on four-dimensional local superconformal symmetry and holomorphy of brane instanton contributions and it reproduces and generalises previous partial results

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Summary

Background structure

Let us review the structure of warped F-theory/IIB compactifications, by using the type IIB description of these vacua [3,4,5,6]. These vacua have an Einstein frame metric of the form ds210 = e2Dds2R1,3 + e−2Dds2X (2.1). Where ds2R1,3 is the flat Minkowski four-dimensional metric, the internal space X is Kahler and the warping e2D is generically non-constant along the internal directions. The R-R F5 is non-trivial and its form is directly linked to the warping by. Where the volume form dvolX is computed by using the internal Kahler metric ds2X .2.

Kahler potential from warped volume
The conformal Kahler potential
The conformal compensator and the Kahler potential
Universal modulus and Kahler potential
Decoding the Kahler potential
Decoding the moduli dependence
Chiral fields and Kahler potential
A comment on D3-brane instantons
Warped kinetic terms and no-scale condition
Large moduli limit
Including axions
Closed string axionic chiral fields
Wilson lines
Kahler metric and no-scale structure
A Derivatives of geometric moduli
Useful preliminary formulas
Derivatives in absence of axionic chiral fields
Derivatives in presence of axionic chiral fields
B A simple example
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