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相关论文: Large trispectrum in two-field slow-roll inflation

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We find constraints on inflationary dynamics that yield a large local bispectrum and/or trispectrum during two-field slow-roll inflation. This leads to simple relations between the non-Gaussianity parameters, simplifying the…

宇宙学与河外天体物理 · 物理学 2013-02-21 Joseph Elliston

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 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 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 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 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 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

The trispectrum is at least as important as the bispectrum and its size can be characterized by two parameters $\tau_{NL}$ and $g_{NL}$. In this short paper, we focus on the Multi-brid inflation, in particular the two-brid inflation model…

高能物理 - 理论 · 物理学 2009-05-29 Qing-Guo Huang

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 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 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 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 examine the momentum dependence of the bispectrum of two-field inflationary models within the long-wavelength formalism. We determine the sources of scale dependence in the expression for the parameter of non-Gaussianity fNL and study…

宇宙学与河外天体物理 · 物理学 2013-06-26 Eleftheria Tzavara , Bartjan van Tent

We study the level of primordial non-Gaussianity in slow-roll two-field inflation. Using an analytic formula for the nonlinear parameter f_nl in the case of a sum or product separable potential, we find that it is possible to generate…

天体物理学 · 物理学 2011-07-13 Christian T. Byrnes , Ki-Young Choi , Lisa M. H. Hall

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 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

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 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 the evolution of the non-linear curvature perturbation during perturbative reheating, and hence how observables evolve to their final values which we may compare against observations. Our study includes the evolution of the two…

宇宙学与河外天体物理 · 物理学 2013-08-23 Godfrey Leung , Ewan R. M. Tarrant , Christian T. Byrnes , Edmund J. Copeland

We use the delta N-formalism to describe the leading order contributions to the primordial power spectrum, bispectrum and trispectrum in multiple-field models of inflation at leading order in a perturbative expansion. In slow-roll models…

天体物理学 · 物理学 2008-11-26 Christian T. Byrnes , Misao Sasaki , David Wands
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