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相关论文: Conditions for observable bi and tri-spectra in tw…

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We calculate the conditions required to produce a large local trispectrum during two-field slow-roll inflation. This is done by extending and simplifying the 'heatmap' approach developed by Byrnes et al. The conditions required to generate…

宇宙学与河外天体物理 · 物理学 2014-03-10 Joseph Elliston , Laila Alabidi , Ian Huston , David J. Mulryne , Reza Tavakol

We investigate the non-Gaussian signatures of ultra slow-roll inflation. The bispectrum and the trispectrum are calculated with general initial conditions. The trispectrum is of local shape, as in the case of the bispectrum. We show that…

高能物理 - 理论 · 物理学 2015-06-15 Qing-Guo Huang , Yi Wang

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 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 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 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 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 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 evaluate the dimensionless non-Gaussianity parameter $h_{_{\rm NL}}$, that characterizes the amplitude of the tensor bispectrum, numerically for a class of two field inflationary models such as double inflation, hybrid inflation and…

宇宙学与河外天体物理 · 物理学 2017-07-26 Rathul Nath Raveendran , L. Sriramkumar

Focusing on the local type primordial non-Gaussianities, we study the bispectrum and trispectrum during a non-minimal slow-roll inflation. We use the so-called $\delta N$ formalism to investigate the super-horizon evolution of the…

宇宙学与河外天体物理 · 物理学 2018-08-28 Kosar Asadi , Kourosh Nozari

We study the slow-roll regime of two field inflation, in which the two fields are also coupled through their kinetic terms. Such Lagrangians are motivated by particle physics and by scalar-tensor theories studied in the Einstein frame. We…

天体物理学 · 物理学 2009-11-11 Fabrizio Di Marco , Fabio Finelli

Theories beyond the standard model such as string theory motivate low energy effective field theories with several scalar fields which are not only coupled through a potential but also through their kinetic terms. For such theories we…

天体物理学 · 物理学 2010-10-27 Ki-Young Choi , Lisa M. H. Hall , Carsten van de Bruck

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

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 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

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 study slow-roll inflation with a Gauss-Bonnet term that is coupled to an inflaton field nonminimally. We investigate the inflationary solutions for a specific type of the nonminimal coupling to the Gauss-Bonnet term and inflaton…

广义相对论与量子宇宙学 · 物理学 2014-10-08 Seoktae Koh , Bum-Hoon Lee , Wonwoo Lee , Gansukh Tumurtushaa

We develop an integral form for the bispectrum in general single-field inflation whose domain of validity includes models of inflation where the background evolution is not constrained to be slowly varying everywhere. Our integral form…

宇宙学与河外天体物理 · 物理学 2018-09-18 Peter Adshead , Wayne Hu , V Miranda

We use transport techniques to calculate the trispectrum produced in multiple-field inflationary models with canonical kinetic terms. Our method allows the time evolution of the local trispectrum parameters, tauNL and gNL, to be tracked…

宇宙学与河外天体物理 · 物理学 2012-10-23 Gemma J. Anderson , David J. Mulryne , David Seery

Ultra slow-roll inflation has recently been used to challenge the non-Gaussianity consistency relation. We show that this inflationary scenario belongs to a one parameter class of models and we study its properties and observational…

宇宙学与河外天体物理 · 物理学 2013-05-30 Jerome Martin , Hayato Motohashi , Teruaki Suyama
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