Table of Contents
Fetching ...

N=4 gauged supergravity and a IIB orientifold with fluxes

Riccardo D'Auria, Sergio Ferrara, Silvia Vaula'

TL;DR

This work analyzes a four-dimensional $N=4$ gauged supergravity, obtained by gauging translational isometries of the scalar manifold, as an effective description of the super-Higgs phases in Type-IIB orientifold compactifications with 3-form fluxes. It employs a dual, $GL(6,\mathbb{R})\times SL(2,\mathbb{R})$-covariant formulation to gauge a flat subgroup, derives the fermion shifts and the scalar potential, and shows the potential is semidefinite nonnegative with a Minkowski minimum when $F^{-IJK}=0$, revealing a no-scale structure. The paper computes the gravitino and vector spectra in the extremum, clarifies how the $N=4\to N=3,2,1,0$ breakings arise from flux components, and identifies the corresponding moduli spaces for each residual supersymmetry. It also connects these results to string compactifications with fluxes and discusses how adding D3-branes or comparing to Scherk–Schwarz reductions would modify the matter content and moduli while preserving the no-scale framework.

Abstract

We analyze the properties of a spontaneously broken D=4, N=4 supergravity without cosmological constant, obtained by gauging translational isometries of its classical scalar manifold. This theory offers a suitable low energy description of the super-Higgs phases of certain Type-IIB orientifold compactifications with 3-form fluxes turned on. We study its N=3,2,1,0 phases and their classical moduli spaces and we show that this theory is an example of no-scale extended supergravity.

N=4 gauged supergravity and a IIB orientifold with fluxes

TL;DR

This work analyzes a four-dimensional gauged supergravity, obtained by gauging translational isometries of the scalar manifold, as an effective description of the super-Higgs phases in Type-IIB orientifold compactifications with 3-form fluxes. It employs a dual, -covariant formulation to gauge a flat subgroup, derives the fermion shifts and the scalar potential, and shows the potential is semidefinite nonnegative with a Minkowski minimum when , revealing a no-scale structure. The paper computes the gravitino and vector spectra in the extremum, clarifies how the breakings arise from flux components, and identifies the corresponding moduli spaces for each residual supersymmetry. It also connects these results to string compactifications with fluxes and discusses how adding D3-branes or comparing to Scherk–Schwarz reductions would modify the matter content and moduli while preserving the no-scale framework.

Abstract

We analyze the properties of a spontaneously broken D=4, N=4 supergravity without cosmological constant, obtained by gauging translational isometries of its classical scalar manifold. This theory offers a suitable low energy description of the super-Higgs phases of certain Type-IIB orientifold compactifications with 3-form fluxes turned on. We study its N=3,2,1,0 phases and their classical moduli spaces and we show that this theory is an example of no-scale extended supergravity.

Paper Structure

This paper contains 7 sections, 87 equations.