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相关论文: Conditions for large non-Gaussianity in two-field …

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We review models which generate a large non-Gaussianity of the local form. We first briefly consider three models which generate the non-Gaussianity either at or after the end of inflation; the curvaton scenario, modulated (p)reheating and…

宇宙学与河外天体物理 · 物理学 2015-03-13 Christian T. Byrnes , Ki-Young Choi

We give a concise formula for the non-Gaussianity of the primordial curvature perturbation generated on super-horizon scales in multi-scalar inflation model without assuming slow-roll conditions. This is an extension of our previous work.…

天体物理学 · 物理学 2013-01-11 Shuichiro Yokoyama , Teruaki Suyama , Takahiro Tanaka

The general expression for the second order large scale curvature perturbation in the form of a functional over a background solution is derived. The explicit expressions was obtained for two special forms of the inflationary potential. In…

宇宙学与河外天体物理 · 物理学 2013-02-26 N. A. Koshelev

We use the long-wavelength formalism to investigate the level of bispectral non-Gaussianity produced in two-field inflation models with standard kinetic terms. Even though the Planck satellite has so far not detected any primordial…

宇宙学与河外天体物理 · 物理学 2017-05-17 Gabriel Jung , Bartjan van Tent

We study the non-Gaussianity generated during multiple-field inflation. We provide an exact expression for the bispectrum parameter f_NL which is valid beyond the slow-roll regime, valid for certain classes of inflationary models. We then…

宇宙学与河外天体物理 · 物理学 2011-11-04 Christian T. Byrnes , Gianmassimo Tasinato

We study the generation of non-Gaussianity in models of hybrid inflation with two inflaton fields, (2-brid inflation). We analyse the region in the parameter and the initial condition space where a large non-Gaussianity may be generated…

天体物理学 · 物理学 2010-04-30 Christian T. Byrnes , Ki-Young Choi , Lisa M. H. Hall

We study the bispectrum of the curvature perturbation on uniform energy density hypersurfaces in models of inflation with two scalar fields evolving simultaneously. In the case of a separable potential, it is possible to compute the…

天体物理学 · 物理学 2009-11-11 Filippo Vernizzi , David Wands

We compute analytic expressions for the non-linearity parameters characterizing the bi- and tri-spectrum of primordial curvature perturbations generated during an inflationary epoch of the early universe driven by an arbitrary number of…

高能物理 - 理论 · 物理学 2011-11-04 Diana Battefeld , Thorsten Battefeld

Recently we studied inflation models in which the inflaton potential is characterized by an underlying approximate global symmetry. In the first work we pointed out that in such a model curvature perturbations are generated after the end of…

天体物理学 · 物理学 2008-11-26 Edward W. Kolb , Antonio Riotto , Alberto Vallinotto

We consider a simple inflation model with a complex scalar field coupled to gravity non-minimally. Both the modulus and the angular directions of the complex scalar are slowly rolling, leading to two-field inflation. The modulus direction…

高能物理 - 唯象学 · 物理学 2015-05-28 Jinn-Ouk Gong , Hyun Min Lee

We compute the amplitude of the non-Gaussianities in inflationary models with multiple, uncoupled scalar fields. This calculation thus applies to all models of assisted inflation, including N-flation, where inflation is driven by multiple…

天体物理学 · 物理学 2010-10-27 Thorsten Battefeld , Richard Easther

Two-field slow-roll inflation is the most conservative modification of a single-field model. The main motivations to study it are its entropic mode and non-Gaussianity. Several years ago, for a two-field model with additive separable…

宇宙学与河外天体物理 · 物理学 2010-12-24 Tower Wang

We analyze the non-Gaussianity for primordial curvature perturbations generated in multi-scalar slow-roll inflation model including the model with non-separable potential by making use of $\delta N$ formalism. Many authors have investigated…

天体物理学 · 物理学 2009-06-23 Shuichiro Yokoyama , Teruaki Suyama , Takahiro Tanaka

We investigate non-Gaussianity in general multiple-field inflation using the formalism we developed in earlier papers. We use a perturbative expansion of the non-linear equations to calculate the three-point correlator of the curvature…

天体物理学 · 物理学 2009-11-13 G. I. Rigopoulos , E. P. S. Shellard , B. J. W. van Tent

We consider a model of two-field inflation, containing an ordinary scalar field and a DBI field. We work beyond the slow-roll approximation, but we assume a separable Hubble parameter. We then derive the form of potential in this framework…

宇宙学与河外天体物理 · 物理学 2016-05-25 Kourosh Nozari , Kosar Asadi

A model of multi-component hybrid inflation, dubbed multi-brid inflation, in which various observable quantities including the non-Gaussianity parameter f_{NL} can be analytically calculated was proposed recently. In particular, for a…

天体物理学 · 物理学 2009-10-09 Atsushi Naruko , Misao Sasaki

We derive semi-analytic formulae for the local bispectrum and trispectrum in general two-field inflation and provide a simple geometric recipe for building observationally allowed models with observable non-Gaussianity. We use the \delta N…

宇宙学与河外天体物理 · 物理学 2015-03-17 Courtney M. Peterson , Max Tegmark

In the context of Type IIB LARGE volume orientifold setup equipped with poly-instanton corrections, the standard single-field poly-instanton inflation driven by a 'Wilson' divisor volume modulus is generalized by the inclusion of respective…

高能物理 - 理论 · 物理学 2013-03-28 Xin Gao , Pramod Shukla

In the present paper, certain inflation models are shown to have large non-Gaussianity in special cases. Namely, finite length inflation models with an effective higher derivative interaction, in which slow-roll inflation is adopted as…

宇宙学与河外天体物理 · 物理学 2010-04-26 Shiro Hirai , Tomoyuki Takami

We investigate non-Gaussianity in general single field models without assuming slow-roll conditions or the exact scale-invariance of the scalar power spectrum. The models considered include general single field inflation (e.g. DBI and…

宇宙学与河外天体物理 · 物理学 2011-05-13 Johannes Noller , Joao Magueijo
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