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相关论文: On two string axions as inflaton

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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…

高能物理 - 唯象学 · 物理学 2016-02-03 Kenji Kadota , Tatsuo Kobayashi , Hajime Otsuka

We explore the possibility of obtaining inflation in weakly coupled heterotic string theory, where the model dependent axions are responsible for driving inflation. This model can be considered as a certain extrapolation of…

高能物理 - 理论 · 物理学 2010-10-27 Martin E. Olsson

We construct a string-inspired nonsingular cosmological scenario in which an inflaton field is driven up the potential before the graceful exit by employing a low-energy string effective action with an orbifold compactification. This sets…

高能物理 - 理论 · 物理学 2015-06-26 Yun-Song Piao , Shinji Tsujikawa , Xinmin Zhang

We study string inspired two-field models of large-field inflation based on axion monodromy in the presence of an interacting heavier modulus. This class of models has enough structure to approximate at least part of the backreaction…

高能物理 - 理论 · 物理学 2020-02-12 Francisco G. Pedro , Alexander Westphal

In type IIB Fibre Inflation models the inflaton is a Kaehler modulus which is kinetically coupled to the corresponding axion. In this setup the curvature of the field space induces tachyonic isocurvature perturbations normal to the…

高能物理 - 理论 · 物理学 2022-09-21 Michele Cicoli , Veronica Guidetti , Francesco Muia , Francisco G. Pedro , Gian Paolo Vacca

We study the effects of the interaction terms between the inflaton fields on the inflationary dynamics in multi-field models. With power law type potential and interactions, the total number of e-folds may get considerably reduced and can…

高能物理 - 理论 · 物理学 2014-11-18 Jinn-Ouk Gong

We study a possible origin of the anomalous suppression of the power spectrum at large angular scales in the cosmic microwave background within the framework of explicit string inflationary models where inflation is driven by a closed…

高能物理 - 理论 · 物理学 2015-06-17 Michele Cicoli , Sean Downes , Bhaskar Dutta

Precise measurements of the microwave background anisotropy have confirmed the inflationary picture of approximately scale invariant, Gaussian primordial adiabatic density perturbations. However, there are some anomalies that suggest a…

宇宙学与河外天体物理 · 物理学 2013-05-29 Chien-Yao Tseng , Mark B. Wise

Inflationary models driven by a large number of axion fields are discussed in the context of type IIB compactifications with N=1 supersymmetry. The inflatons arise as the scalar modes of the R-R two-forms evaluated on vanishing two-cycles…

高能物理 - 理论 · 物理学 2008-06-13 Thomas W. Grimm

We study general class of small-field axion inflations which are the mixture of polynomial and sinusoidal functions suggested by the natural and axion monodromy inflations. The axion decay constants leading to the successful axion…

高能物理 - 唯象学 · 物理学 2017-04-24 Tatsuo Kobayashi , Akane Oikawa , Naoya Omoto , Hajime Otsuka , Ikumi Saga

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…

高能物理 - 理论 · 物理学 2007-05-23 R. Holman , Jimmy A. Hutasoit

We investigate the effects of large inhomogeneities in both the inflaton field and its momentum. We find that in general, large kinetic perturbations reduce the number of e-folds of inflation. In particular, we observe that inflationary…

宇宙学与河外天体物理 · 物理学 2025-01-13 Matthew Elley , Josu C. Aurrekoetxea , Katy Clough , Raphael Flauger , Panagiotis Giannadakis , Eugene A. Lim

We study multifield contributions to the scalar power spectrum in an ensemble of six-field inflationary models obtained in string theory. We identify examples in which inflation occurs by chance, near an approximate inflection point, and we…

宇宙学与河外天体物理 · 物理学 2015-06-05 Liam McAllister , Sébastien Renaux-Petel , Gang Xu

We study the dynamics of axion-like fields in F-theory and suggest that they can serve as inflatons in models of natural inflation. The axions arise from harmonic three-forms on the F-theory compactification space and parameterize a complex…

高能物理 - 理论 · 物理学 2021-12-21 Thomas W. Grimm

We study adiabatic and isocurvature perturbation spectra produced by a period of cosmological inflation driven by two scalar fields. We show that there exists a model-independent consistency condition for all two-field models of slow-roll…

天体物理学 · 物理学 2009-11-07 David Wands , Nicola Bartolo , Sabino Matarrese , Antonio Riotto

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…

宇宙学与河外天体物理 · 物理学 2025-07-04 Alireza Talebian , Hassan Firouzjahi

We study a string theory inspired model for hybrid inflation in the context of a brane-antibrane system partially compactified on a compact submanifold of (a caricature of) a Calabi-Yau manifold. The interbrane distance acts as the…

高能物理 - 理论 · 物理学 2018-02-14 Debajyoti Choudhury , Debashis Ghoshal , Dileep P. Jatkar , Sudhakar Panda

The recent BICEP2 measurements of B-modes indicate a large tensor-to-scalar ratio in inflationary cosmology, which points towards trans-Planckian evolution of the inflaton. We propose possible string-theory realizations thereof. Schemes for…

高能物理 - 理论 · 物理学 2015-06-19 Ralph Blumenhagen , Erik Plauschinn

I investigate multi-field inflationary models with fields that decay during inflation, leading to staggered inflation. This feature is natural in many models motivated by string theory, for instance if inflatons are related to interbrane…

天体物理学 · 物理学 2010-01-08 Thorsten Battefeld

A string theory based inflationary model is developed where the inflaton interacts with a multitude of massive string level states causing dissipation of vacuum energy. Inflation terminates in a warm Universe without the need for reheating.

高能物理 - 唯象学 · 物理学 2009-10-31 Arjun Berera , Thomas W. Kephart
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