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Aligned Natural Inflation in String Theory

Cody Long, Liam McAllister, Paul McGuirk

TL;DR

This work addresses the challenge of achieving large-field inflation with trans-Planckian axion excursions in string theory by embedding the Kim–Nilles–Peloso decay-constant alignment mechanism into type IIB Calabi–Yau orientifold compactifications. The authors show that gaugino condensation on magnetized or multiply-wrapped D7-branes can generate two non-perturbative axion couplings whose near-alignment yields an enhanced effective decay constant f_{eff} ~ f/δ when the alignment condition f_{A1}/f_{A2} = f_{B1}/f_{B2} (or its near variant) is satisfied, with the potential written in the standard KNP form. They provide explicit expressions for the non-perturbative superpotential and gauge-kinetic functions, derive the resulting aligned-axion potentials, and present toy examples demonstrating large f_{eff} in controlled regimes, while noting substantial hurdles in full moduli stabilization and matching the scalar power spectrum. The results offer a concrete string-theoretic route to large-field natural inflation and suggest that combining multiple alignment mechanisms or kinetic-alignment ideas could improve robustness and allow parametric control within stabilized compactifications.

Abstract

We propose a scenario for realizing super-Planckian axion decay constants in Calabi-Yau orientifolds of type IIB string theory, leading to large-field inflation. Our construction is a simple embedding in string theory of the mechanism of Kim, Nilles, and Peloso, in which a large effective decay constant arises from alignment of two smaller decay constants. The key ingredient is gaugino condensation on magnetized or multiply-wound D7-branes. We argue that, under very mild assumptions about the topology of the Calabi-Yau, there are controllable points in moduli space with large effective decay constants.

Aligned Natural Inflation in String Theory

TL;DR

This work addresses the challenge of achieving large-field inflation with trans-Planckian axion excursions in string theory by embedding the Kim–Nilles–Peloso decay-constant alignment mechanism into type IIB Calabi–Yau orientifold compactifications. The authors show that gaugino condensation on magnetized or multiply-wrapped D7-branes can generate two non-perturbative axion couplings whose near-alignment yields an enhanced effective decay constant f_{eff} ~ f/δ when the alignment condition f_{A1}/f_{A2} = f_{B1}/f_{B2} (or its near variant) is satisfied, with the potential written in the standard KNP form. They provide explicit expressions for the non-perturbative superpotential and gauge-kinetic functions, derive the resulting aligned-axion potentials, and present toy examples demonstrating large f_{eff} in controlled regimes, while noting substantial hurdles in full moduli stabilization and matching the scalar power spectrum. The results offer a concrete string-theoretic route to large-field natural inflation and suggest that combining multiple alignment mechanisms or kinetic-alignment ideas could improve robustness and allow parametric control within stabilized compactifications.

Abstract

We propose a scenario for realizing super-Planckian axion decay constants in Calabi-Yau orientifolds of type IIB string theory, leading to large-field inflation. Our construction is a simple embedding in string theory of the mechanism of Kim, Nilles, and Peloso, in which a large effective decay constant arises from alignment of two smaller decay constants. The key ingredient is gaugino condensation on magnetized or multiply-wound D7-branes. We argue that, under very mild assumptions about the topology of the Calabi-Yau, there are controllable points in moduli space with large effective decay constants.

Paper Structure

This paper contains 9 sections, 60 equations, 3 figures.

Figures (3)

  • Figure 1: Three branes wrapping locally volume minimizing representatives of the same homology class.
  • Figure 2: Two branes multiply wrapping the same cycle the same number of times.
  • Figure 3: The 2-axion potential \ref{['eq:example_pot']}. Darker regions correspond to higher points in the potential. Inflation can be accommodated along the super-Planckian trajectory indicated by the arrow. The very slight tilt of the trajectory is a consequence of a very slight shift in the position of the minimum for $\psi^{1}$ as $\psi^{2}$ evolves.