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Aligned natural inflation in string theory

Cody Long, Liam McAllister, and Paul McGuirk
Phys. Rev. D 90, 023501 – Published 10 July 2014

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.

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  • Received 13 May 2014

DOI:https://doi.org/10.1103/PhysRevD.90.023501

© 2014 American Physical Society

Authors & Affiliations

Cody Long*, Liam McAllister, and Paul McGuirk

  • Department of Physics, Cornell University, Ithaca, New York 14853, USA

  • *cel89@cornell.edu
  • mcallister@cornell.edu
  • mcguirk@cornell.edu

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Issue

Vol. 90, Iss. 2 — 15 July 2014

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Images

  • Figure 1
    Figure 1

    Three branes wrapping locally volume minimizing representatives of the same homology class.

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  • Figure 2
    Figure 2

    Two branes multiply wrapping the same cycle the same number of times.

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  • Figure 3
    Figure 3

    The 2-axion potential (54). 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 ψ1 as ψ2 evolves.

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