Higgs-otic Inflation and String Theory
Luis E. Ibanez, Fernando Marchesano, Irene Valenzuela

TL;DR
This paper presents a string theory-based model where the Higgs field drives inflation, linking the inflaton to the MSSM Higgs and achieving observable predictions consistent with current experiments.
Contribution
It introduces a novel string theory realization of Higgs-driven inflation using D-brane positions and fluxes, connecting particle physics and cosmology in a unified framework.
Findings
Achieves 50-60 e-folds of inflation with r>0.07
Provides a calculable inflaton potential from string theory
Links electroweak symmetry breaking with inflationary dynamics
Abstract
We propose that inflation is driven by a (complex) neutral Higgs of the MSSM extension of the SM, in a chaotic-like inflation setting. The SUSY breaking soft term masses are of order GeV, which is identified with the inflaton mass scale and is just enough to stabilise the SM Higgs potential. The fine-tuned SM Higgs has then a mass around 126 GeV, in agreement with LHC results. We point out that the required large field excursions of chaotic inflation may be realised in string theory with the (complex) inflaton/Higgs identified with a continuous Wilson line or D-brane position. We show specific examples and study in detail a IIB orientifold with D7-branes at singularities, with SM gauge group and MSSM Higgs sector. In this case the inflaton/Higgs fields correspond to D7-brane positions along a two-torus transverse to them. Masses and monodromy are induced by closed…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
