Universal constraints on axions from inflation

R. Z. Ferreira, M. S. Sloth

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Abstrakt

We consider the presence of an axion like particle, sigma, with a generic CP violating axial coupling of the form (alpha sigma/f), where F (mu nu) is the gauge field strength of a generic abelian U(1) gauge group, not necessarily associated with the standard electromagnetism, and f is the decay constant of the axion. It has previously been demonstrated that if the axion is identified with the inflaton, such an interaction can lead to measurable cosmological signatures (non-Gaussian modifications of the curvature perturbation spectrum) depending on the parameter . In the present paper we will show that the generation of curvature perturbation at horizon crossing due to the axial coupling has a universal form and remains unmodified in terms of the xi parameter even if the axion, sigma, is not identified with the inflaton. As a consequence, it does not appear to be possible to generate CMB tensor perturbations through this mechanism, larger than the vacuum ones, without violating the observational constraints unless we combine this mechanism with a curvaton or if the sigma field becomes heavy and decays during inflation. Even in this last case there are non-trivial constraints coming from the slow-roll evolution of the curvature perturbation on super horizon scales which should be taken into account. We also comment on implications for inflationary models where axions play an important role as, for example, models of natural inflation where more than one axion are included and models where the curvaton is an axion.
OriginalsprogEngelsk
TidsskriftJournal of High Energy Physics
Udgave nummer12
Antal sider22
ISSN1126-6708
DOI
StatusUdgivet - 2014

Bibliografisk note

ISI Document Delivery No.: AY2ZZ Times Cited: 1 Cited Reference Count: 54 Ferreira, Ricardo Z. Sloth, Martin S. Lundbeck foundation We would like to thank Guido D'Amico, Nemanja Kaloper, Antonio Riotto and David Wands for their comments on the draft. In addition we would like to thank Shinji Mukohyama, Ryo Namba, Marco Peloso, Gary Shiu, and Lorenzo Sorbo for clarifying comments about their scenarios and discussions. We would also like to thank the Lundbeck foundation for financial support. 1 SPRINGER NEW YORK J HIGH ENERGY PHYS

Emneord

  • Cosmology of Theories beyond the SM Effective field theories NATURAL INFLATION PERTURBATIONS

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