D3/D7 Inflationary Model and M-theory
Keshav Dasgupta, Carlos Herdeiro, Shinji Hirano, Renata Kallosh
TL;DR
The paper presents a D3/D7 inflationary scenario in Type IIB string theory with a constant worldvolume flux on the D7, realized as an $N=2$ $P$-term inflation potential. Inflation proceeds along a Coulomb-like de Sitter valley with the inflaton given by the D3–D7 separation, and ends in a waterfall to a Minkowski vacuum described by a D3/D7 bound state identified with a non-linear (non-commutative) Abelian instanton; the nonzero cosmological constant is tied to resolving the small-instanton singularity via the noncommutative parameter. The construction is embedded in a compactified Type IIB setup on $K3 imes T^2/ ext{Z}_2$ with orientifolds, and lifted to M-theory on a four-fold with G-fluxes, analyzing both Coulomb and Higgs branches, their SUSY properties, and higher-order corrections. The work connects cosmological dynamics to brane/flux configurations, noncommutative instanton physics, and anomaly-consistent M-theory compactifications, offering a path toward a fully string/M-theory realization of hybrid inflation with a geometric origin for the cosmological constant.
Abstract
A proposal is made for a cosmological D3/D7 model with a constant magnetic flux along the D7 world-volume. It describes an N=2 gauge model with Fayet-Iliopoulos terms and the potential of the hybrid P-term inflation. The motion of the D3-brane towards D7 in a phase with spontaneously broken supersymmetry provides a period of slow-roll inflation in the de Sitter valley, the role of the inflaton being played by the distance between D3 and D7-branes. After tachyon condensation a supersymmetric ground state is formed: a D3/D7 bound state corresponding to an Abelian non-linear (non-commutative) instanton. In this model the existence of a non-vanishing cosmological constant is associated with the resolution of the instanton singularity. We discuss a possible embedding of this model into a compactified M-theory setup.
