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If the inflaton is a pseudo-scalar axion, the axion shift symmetry can protect the flatness of its potential from too large radiative corrections. This possibility, known as natural inflation, requires an axion scale which is greater than…

High Energy Physics - Phenomenology · Physics 2009-11-10 Jihn E. Kim , Hans Peter Nilles , Marco Peloso

We propose a model for inflation consisting of an axionic scalar field coupled to a set of three non-Abelian gauge fields. Our model's novel requirement is that the gauge fields begin inflation with a rotationally invariant vacuum…

High Energy Physics - Theory · Physics 2012-07-06 Peter Adshead , Mark Wyman

An attractive candidate for the inflaton is an axion slowly rolling down a flat potential protected by a perturbative shift symmetry. Realisations of this idea within large field, natural and monomial inflation have been disfavoured by…

Cosmology and Nongalactic Astrophysics · Physics 2016-04-20 Susha Parameswaran , Gianmassimo Tasinato , Ivonne Zavala

The inflationary paradigm has enjoyed phenomenological success, however, a compelling particle physics realization is still lacking. The key obstruction is that the requirement of a suitably flat scalar potential is sensitive to…

High Energy Physics - Phenomenology · Physics 2011-05-12 Neil Barnaby , Marco Peloso

Multiple axions form a landscape in the presence of various shift symmetry breaking terms. Eternal inflation populates the axion landscape, continuously creating new universes by bubble nucleation. Slow-roll inflation takes place after the…

High Energy Physics - Phenomenology · Physics 2015-04-14 Tetsutaro Higaki , Fuminobu Takahashi

We show that inflation with a quadratic potential occurs naturally in theories where an axion-like field mixes with a 4-form. Such an axion is massive, with the mass which arises from the mixing being protected by the axion shift symmetry.…

High Energy Physics - Theory · Physics 2009-04-14 Nemanja Kaloper , Lorenzo Sorbo

Natural (axionic) inflation can accommodate sizeable primordial tensor modes but suffers from the necessity of trans-Planckian variations of the inflaton field. This problem can be solved via the mechanism of aligned axions…

High Energy Physics - Theory · Physics 2014-09-01 Rolf Kappl , Sven Krippendorf , Hans Peter Nilles

We discuss inflation models within supersymmetry and supergravity frameworks with a landscape of chiral superfields and one $U(1)$ shift symmetry which is broken by non-perturbative symmetry breaking terms in the superpotential. We label…

High Energy Physics - Phenomenology · Physics 2018-04-18 Pran Nath , Maksim Piskunov

We propose a landscape of many axions, where the axion potential receives various contributions from shift symmetry breaking effects. We show that the existence of the axion with a super-Planckian decay constant is very common in the axion…

High Energy Physics - Theory · Physics 2014-07-22 Tetsutaro Higaki , Fuminobu Takahashi

Slow-roll inflation is a successful paradigm. However we find that even a small coupling of the inflaton to other light fields can dramatically alter the dynamics and predictions of inflation. As an example, the inflaton can generically…

High Energy Physics - Phenomenology · Physics 2023-09-19 Kim V. Berghaus , Peter W. Graham , David E. Kaplan

A novel framework is proposed for embedding the natural inflation into the type IIA superstrings compactified on a Calabi-Yau (CY) three-fold. Inflaton is identified with axion of the Universal Hypermultiplet (UH). The other UH scalars…

High Energy Physics - Theory · Physics 2014-10-15 Sergei V. Ketov

Axions play a central role in many realizations of large field models of inflation and in recent alternative mechanisms for generating primordial tensor modes in small field models. If these axions couple to gauge fields, the coupling…

Cosmology and Nongalactic Astrophysics · Physics 2016-10-14 Ricardo Z. Ferreira , Jonathan Ganc , Jorge Noreña , Martin S. Sloth

Multi-natural inflation is studied in the context of warm inflation. We study the warm multi-natural inflation scenario with both linear and cubic temperature-dependent dissipation coefficients. The model is motivated by axion-like…

High Energy Physics - Phenomenology · Physics 2025-09-01 Asuka Ito , Rudnei O. Ramos

In the so-called natural inflation, an axion-like inflaton is assumed to have a cosine-type periodic potential. This is not the case in a very simple model in which the axion-like inflaton is coupled to an SU(N) (or other) pure Yang-Mills,…

High Energy Physics - Theory · Physics 2015-06-19 Kazuya Yonekura

We consider a model of inflation in which the inflaton field is a rolling axion with a potential which is flat enough to support an intermediate phase of USR inflation. Because of the Chern-Simons interaction, one polarization of the gauge…

Cosmology and Nongalactic Astrophysics · Physics 2025-07-04 Alireza Talebian , Hassan Firouzjahi

We construct a natural inflation model in supergravity where the inflaton is identified with a modulus field possessing a shift symmetry. The superpotential for the inflaton is generated by meson condensation due to strong dynamics with…

High Energy Physics - Phenomenology · Physics 2015-06-22 Keisuke Harigaya , Masahiro Ibe , Tsutomu T. Yanagida

We revisit models of natural inflation and show that the single-field effective theory described by the potential $V(a)\sim \cos\frac{a}{f}$ breaks down as the inflaton $a$ makes large-field excursions, even for values of $f$ smaller than…

High Energy Physics - Theory · Physics 2021-01-13 Mohamed M. Anber , Stephen Baker

We study an extension of the natural inflation model comprising a non-Abelian gauge sector coupled to the axion-inflaton kinetic term. We show how such non-minimal coupling serves as a source of friction for the rolling inflaton granting…

Cosmology and Nongalactic Astrophysics · Physics 2024-12-02 Martino Michelotti , Rodrigo Gonzalez Quaglia , Ema Dimastrogiovanni , Matteo Fasiello , Diederik Roest

The original axion natural inflation model predicts a tensor-to-scalar ratio exceeding experimental limits. Conversely, in aligned axion inflation, inflation can proceed along trajectories emerging from near a saddle point of the two-field…

Cosmology and Nongalactic Astrophysics · Physics 2025-10-21 Federico Greco

A safe way to reheat the universe, in models of natural and quadratic inflation, is through shift symmetric couplings between the inflaton $\phi$ and the Standard Model (SM), since they do not generate loop corrections to the potential…

Cosmology and Nongalactic Astrophysics · Physics 2018-04-04 Ricardo Z. Ferreira , Alessio Notari
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