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相关论文: Non Gaussianity of General Multiple-Field Inflatio…

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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

In this work, we present a method for implementing the $\delta N$ formalism to study the primordial non-Gaussianity produced in multiple three-form field inflation. Using a dual description relating three-form fields to noncanonical scalar…

宇宙学与河外天体物理 · 物理学 2016-11-09 K. Sravan Kumar , David J. Mulryne , Nelson J. Nunes , João Marto , Paulo Vargas Moniz

We show that theories of inflation with multiple, rapidly turning fields can generate large amounts of non-Gaussianity. We consider a general theory with two fields, an arbitrary field-space metric, and a potential that supports sustained,…

宇宙学与河外天体物理 · 物理学 2024-06-21 Oksana Iarygina , M. C. David Marsh , Gustavo Salinas

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 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

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

In the present paper, we study the non-Gaussianity of multiple-field inflation model using the method of the field equation. We start from reviewing the background and the perturbation theory of multiple-field inflation, and then derive the…

天体物理学 · 物理学 2008-04-04 Shi-Wen Li , Wei Xue

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

Using $\delta N$ formalism, in the context of a generic multi-field inflation driven on a non-flat field space background, we revisit the analytic expressions of the various cosmological observables such as scalar/tensor power spectra,…

高能物理 - 理论 · 物理学 2014-10-07 Xin Gao , Tianjun Li , Pramod Shukla

We perform a general study of the primordial scalar non-Gaussianities in multi-field inflationary models in Einstein gravity. We consider models governed by a Lagrangian which is a general function of the scalar fields and their first…

天体物理学 · 物理学 2009-06-23 Xian Gao

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

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 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 construct explicit models of multi-field inflation in which the primordial metric fluctuations do not necessarily obey Gaussian statistics. These models are realizations of mechanisms in which non-Gaussianity is first generated by a…

天体物理学 · 物理学 2008-11-26 Francis Bernardeau , Jean-Philippe Uzan

A $\delta N$ formalism is used to study the non-Gaussianity of the primordial curvature perturbation on an uniform density hypersurfaces generated by the warm inflation for the first time. After introducing the framework of the warm…

广义相对论与量子宇宙学 · 物理学 2016-04-01 Xiao-Min Zhang , Hong-Yang Ma , Peng-Cheng Chu , Jun-Ting Liu , Jian-Yang Zhu

We consider a class of multi-component hybrid inflation models whose evolution may be analytically solved under the slow-roll approximation. We call it multi-brid inflation (or $n$-brid inflation where $n$ stands for the number of inflaton…

天体物理学 · 物理学 2009-10-09 Misao Sasaki

This article investigates the generation of non-Gaussianity during inflation. In the context of multi-field inflation, we detail a mechanism that can create significant primordial non-Gaussianities in the adiabatic mode while preserving the…

高能物理 - 唯象学 · 物理学 2009-11-07 Francis Bernardeau , Jean-Philippe Uzan

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

While detection of the "local form" bispectrum of primordial perturbations would rule out all single-field inflation models, multi-field models would still be allowed. We show that multi-field models described by the $\delta N$ formalism…

广义相对论与量子宇宙学 · 物理学 2011-07-28 Naonori S. Sugiyama , Eiichiro Komatsu , Toshifumi Futamase

We use the long-wavelength formalism to compute the bispectral non-Gaussianity produced in two-field inflation. We find an exact result that is used as the basis of numerical studies, and an explicit analytical slow-roll expression for…

宇宙学与河外天体物理 · 物理学 2015-03-17 Eleftheria Tzavara , Bartjan van Tent
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