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Related papers: On Natural Inflation and Moduli Stabilisation in S…

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Moduli fields, which parameterize perturbative flat directions of the potential in supersymmetric theories, are natural candidates to act as inflatons. An inflationary potential on moduli space can result if the scale of dynamical SUSY…

High Energy Physics - Theory · Physics 2009-10-28 Scott Thomas

We study the inflation scenarios, in the framework of superstring theory, where the inflaton is an axion producing the adiabatic curvature perturbations while there exists another light axion producing the isocurvature perturbations. We…

High Energy Physics - Phenomenology · Physics 2016-02-03 Kenji Kadota , Tatsuo Kobayashi , Hajime Otsuka

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

A model of natural inflation with an effectively trans-Planckian decay constant can be easily achieved by the "phase locking" mechanism while keeping field values in the effective field theory within the Planck scale. We give detailed…

High Energy Physics - Phenomenology · Physics 2015-06-22 Keisuke Harigaya , Masahiro Ibe

High-scale string inflationary models are in well-known tension with low-energy supersymmetry. A promising solution involves models where the inflaton is the volume of the extra dimensions so that the gravitino mass relaxes from large…

High Energy Physics - Theory · Physics 2016-01-20 Michele Cicoli , Francesco Muia , Francisco Gil Pedro

We propose a new mechanism that adapts to string theory a perturbative method for stabilizing moduli without leaving the domain of perturbative control, thereby evading the `Dine-Seiberg' problem. The only required nonperturbative…

High Energy Physics - Theory · Physics 2022-07-13 C. P. Burgess , F. Quevedo

We prove that inflation is forbidden in the most well understood class of semi-realistic type IIA string compactifications: Calabi-Yau compactifications with only standard NS-NS 3-form flux, R-R fluxes, D6-branes and O6-planes at large…

High Energy Physics - Theory · Physics 2009-10-07 Mark P. Hertzberg , Shamit Kachru , Washington Taylor , Max Tegmark

Pseudo-Goldstone bosons (pGBs) can provide technically natural inflatons, as has been comparatively well-explored in the simplest axion examples. Although inflationary success requires trans-Planckian decay constants, f > Mp, several…

High Energy Physics - Theory · Physics 2015-09-01 C. P. Burgess , Diederik Roest

We construct a model of inflation in string theory after carefully taking into account moduli stabilization. The setting is a warped compactification of Type IIB string theory in the presence of D3 and anti-D3-branes. The inflaton is the…

High Energy Physics - Theory · Physics 2014-11-18 Norihiro Iizuka , Sandip P. Trivedi

We find a general model of {\em single-field} inflation within the context of type IIB string theory compactified on large volume Calabi-Yau orientifolds with $h^{2,1} > h^{1,1} = 2$. The inflaton is the axion part of the complexified…

High Energy Physics - Theory · Physics 2007-05-23 R. Holman , Jimmy A. Hutasoit

It is tempting to inflate along one of the many flat directions that arise in supersymmetric theories. The required flatness of the potential to obtain sufficient inflation and to not overproduce density fluctuations occurs naturally.…

High Energy Physics - Phenomenology · Physics 2009-10-28 Katherine Freese , Tony Gherghetta , Hideyuki Umeda

We investigate the possibility that spiral inflation can be realized using the near-conifold flux potentials for the complex structure moduli in type IIB string theory compactified on a Calabi-Yau manifold. Using the explicit form of the…

High Energy Physics - Theory · Physics 2013-08-05 Pontus Ahlqvist , Brian Greene , David Kagan

Large field excursions are required in a number of axion models of inflation. These models also possess global cosmic strings, around which the axion follows a path mirroring the inflationary trajectory. Cosmic strings are thus an…

High Energy Physics - Theory · Physics 2017-05-23 Matthew J. Dolan , Patrick Draper , Jonathan Kozaczuk , Hiren Patel

It is widely believed that string theory easily allows for a QCD axion in the cosmologically favoured mass range. The required small decay constant, $f_a\ll M_P$, can be implemented by using a large compactification volume. This points to…

High Energy Physics - Theory · Physics 2022-10-19 Michele Cicoli , Arthur Hebecker , Joerg Jaeckel , Manuel Wittner

In this paper we obtain a model of Natural Inflation from string theory with a Planckian decay constant. We investigate D-brane dynamics in the background of the warped resolved conifold (WRC) throat approximation of Type IIB string…

High Energy Physics - Theory · Physics 2015-03-02 Zachary Kenton , Steven Thomas

We present a type IIB 4D string model with stabilised moduli which is able to describe the history of the universe from inflation to quintessence. The underlying Calabi-Yau volume is controlled by two moduli which are stabilised by…

High Energy Physics - Theory · Physics 2024-07-08 Michele Cicoli , Francesc Cunillera , Antonio Padilla , Francisco G. Pedro

In this talk we describe recent progress in construction of inflationary models in the context of string theory with flux compactification and moduli stabilization. We also discuss a possibility to test string theory by cosmological…

High Energy Physics - Theory · Physics 2010-04-06 Renata Kallosh

Based on the flux-scaling scenario we study a model consisting on Type IIB string theory compactified on a Calabi-Yau manifold with a frozen complex structure in the presence of generic fluxes. The model contains (meta)stable Minkowski and…

High Energy Physics - Theory · Physics 2021-07-28 Cesar Damian , Oscar Loaiza-Brito

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 in type IIB string theory driven by the volume modulus can be realized in the context of the racetrack-based Kallosh-Linde model (KL) of moduli stabilization. Inflation here arises through the volume modulus…

High Energy Physics - Theory · Physics 2009-09-29 Andrei Linde , Alexander Westphal