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We discuss the signatures of non-Gaussianity in the curvaton model where the potential includes also a non-quadratic term. In such a case the non-linearity parameter f_NL can become very small, and we show that non-Gaussianity is then…

Astrophysics · Physics 2011-07-13 Kari Enqvist , Tomo Takahashi

We study the axion-type curvaton model, with emphasis on the large field regime where analytic results are very difficult to obtain. We evaluate the tensor-scalar ratio $r$ using WMAP normalization and the non-linearity parameters $f_{NL}$…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-18 Pravabati Chingangbam , Qing-Guo Huang

We demonstrate novel features in the behavior of the second and third order non-linearity parameters of the curvature perturbation, namely, $f_{NL}$ and $g_{NL}$, arising from non-linear motion of curvaton field. We investigate two classes…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-28 Pravabati Chingangbam , Qing-Guo Huang

The evolution of the curvature perturbation is highly non-trivial for curvaton models with self-interactions and is very sensitive to the parameter values. The final perturbation depends also on the curvaton decay rate $\Gamma$. As a…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 Kari Enqvist

We investigate non-Gaussianities in self-interacting curvaton models treating both renormalizable and non-renormalizable polynomial interactions. We scan the parameter space systematically and compute numerically the non-linearity…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-13 Kari Enqvist , Sami Nurmi , Olli Taanila , Tomo Takahashi

We show that the local type non-Gaussianity in a class of curvaton models is suppressed, i.e. the non-linearity parameters f_{NL} and those related with higher order statistics can be at most O(1), even if the curvaton energy density is…

Cosmology and Nongalactic Astrophysics · Physics 2014-06-25 Kyohei Mukaida , Kazunori Nakayama , Masahiro Takimoto

We characterise the primordial perturbations produced due to both inflaton and curvaton fluctuations in models where the curvaton has a quadratic, cosine or hyperbolic potential, and the inflaton potential is characterised by the usual…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 José Fonseca , David Wands

We investigate density perturbations sourced by a curvaton with a generic energy potential. The key feature of a curvaton potential which deviates from a quadratic is that the curvaton experiences a non-uniform onset of its oscillation.…

Cosmology and Nongalactic Astrophysics · Physics 2011-12-12 Masahiro Kawasaki , Takeshi Kobayashi , Fuminobu Takahashi

We revise the Non-Gaussianity of canonical curvaton scenario with a generalized $\delta N$ formalism, in which it could handle the generic potentials. In various curvaton models, the energy density is dominant in different period including…

Cosmology and Nongalactic Astrophysics · Physics 2021-03-18 Lei-Hua Liu , Bin Liang , Ya-Chen Zhou , Xiao-Dan Liu , Wu-Long Xu , Ai-Chen Li

We consider curvaton models with potentials that depart slightly from the quadratic form. We show that although such a small departure does not modify significantly the Gaussian part of the curvature perturbation, it can have a pronounced…

Astrophysics · Physics 2008-11-26 Kari Enqvist , Sami Nurmi

We study the curvaton scenario using gauge-invariant second order perturbation theory and solving the governing equations numerically. Focusing on large scales we calculate the non-linearity parameter f_nl in the two-fluid curvaton model…

Astrophysics · Physics 2009-11-11 Karim A. Malik , David H. Lyth

We investigate how the background evolution affects the curvature perturbations generated by the curvaton, assuming a curvaton potential that may deviate slightly from the quadratic one, and parameterizing the background fluid density as…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 Kari Enqvist , Tomo Takahashi

In this paper, we will use $\delta \mathcal{N}$-formalism to calculate the primordial curvature perturbation for the curvaton model with a Lagrange multiplier field. We calculate the non-linearity parameters $f_{NL}$ and $g_{NL}$ in the…

Cosmology and Nongalactic Astrophysics · Physics 2012-09-27 Chao-Jun Feng , Xin-Zhou Li

In general a weakly self-interacting curvaton field is expected and the curvaton potential takes the polynomial form. The curvaton potential can be dominated by the self-interaction term during the period of inflation if the curvaton field…

High Energy Physics - Theory · Physics 2011-02-07 Qing-Guo Huang

We show how to build a curvaton inflationary model motivated by scale-dependent non-Gaussianities of cosmological perturbations. In particular, we study the change of sign in the $f_{NL}$ parameter as a function of the curvaton field value…

Cosmology and Nongalactic Astrophysics · Physics 2021-03-31 L. F. Guimarães , F. T. Falciano

We discuss observational consequences of the curvaton scenario, which naturally appears in the context of the simplest model of chaotic inflation in supergravity. The non-gaussianity parameter f_NL in this scenario can take values in the…

High Energy Physics - Theory · Physics 2015-05-20 Vittoria Demozzi , Andrei Linde , Viatcheslav Mukhanov

We discuss non-Gaussianity and baryonic isocurvature fluctuations in the curvaton scenario, assuming that the baryon asymmetry of the universe originates only from the decay products of the inflaton. When large non-Gaussianity is realized…

High Energy Physics - Phenomenology · Physics 2009-02-02 Takeo Moroi , Tomo Takahashi

We study non-Gaussianity of density perturbations generated by an axionic curvaton, focusing on the case that the curvaton sits near the hilltop of the potential during inflation. Such hilltop curvatons can generate a red-tilted density…

Cosmology and Nongalactic Astrophysics · Physics 2013-03-15 Masahiro Kawasaki , Takeshi Kobayashi , Fuminobu Takahashi

The generation of non-gaussianity is studied in a three fluid curvaton model. By utilizing second order perturbation theory we derive general formulae for the large scale temperature fluctuation and non-gaussianity parameter, $f_{NL}$, that…

Astrophysics · Physics 2009-07-30 Tuomas Multamaki , Jani Sainio , Iiro Vilja

We present a systematic study of the amplitude of the primordial perturbation in curvaton models with self-interactions, treating both renormalizable and non-renormalizable interactions. In particular, we consider the possibility that the…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-13 Kari Enqvist , Sami Nurmi , Gerasimos Rigopoulos , Olli Taanila , Tomo Takahashi
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