English

Strong Dynamics and Natural Inflation

High Energy Physics - Theory 2018-10-10 v1 Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology

Abstract

We continue our investigation of the 4d effective field theory for closed string axions in Type II compactifications with D-branes. The inclusion of St\"uckelberg couplings for the axions requires the presence of chiral fermions at D-brane intersections, whose interactions at strong non-Abelian gauge coupling induce mass terms for the axions and scalar chiral condensate excitations, dubbed infladrons. The set-up allows for a realization of natural-like inflation with a closed string axion as inflaton and a flattened scalar potential due to the back-reaction of the more massive infladrons. We further point out that this large field inflationary model is not compromised by axionic wormhole corrections.

Keywords

Cite

@article{arxiv.1807.00620,
  title  = {Strong Dynamics and Natural Inflation},
  author = {Gary Shiu and Wieland Staessens},
  journal= {arXiv preprint arXiv:1807.00620},
  year   = {2018}
}

Comments

6 pages, 2 figures

R2 v1 2026-06-23T02:48:03.621Z