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相关论文: Delta-N Formalism for Curvaton with Modulated Deca…

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The curvaton reheating mechanism in a non-minimal derivative coupling to gravity for any non-oscillating (NO) model is studied. In this framework, we analyze the energy density during the kinetic epoch and we find that this energy has a…

广义相对论与量子宇宙学 · 物理学 2016-10-05 Ramon Herrera , Joel Saavedra , Cuauhtemoc Campuzano

We focus on the evolution of curvature perturbation on superhorizon scales by adopting the spatial gradient expansion and show that the nonlinear theory, called the beyond $\delta N$-formalism as the next-leading order in the expansion. As…

宇宙学与河外天体物理 · 物理学 2014-03-05 Yu-ichi Takamizu

In this paper we analyse three models of the early universe, for which the respective mechanisms for generating the curvature perturbation are considered disparate. We find that in fact the mechanisms are very similar, and hence explain why…

宇宙学与河外天体物理 · 物理学 2010-12-01 Laila Alabidi , Karim A. Malik , Christian T. Byrnes , Ki-Young Choi

In this work we investigate curvature perturbations and non-Gaussianity arising from Higgs modulated reheating in the early Universe. We employ three different methods -- the period-averaging (PA) method, the exact method, and the…

宇宙学与河外天体物理 · 物理学 2025-11-25 Weiyi Deng , Chengcheng Han , Zhanhong Lei , Jin Min Yang

We review recent developments in the theory of inflation and cosmological perturbations produced from inflation. After a brief introduction of the standard, single-field slow-roll inflation, and the curvature and tensor perturbations…

宇宙学与河外天体物理 · 物理学 2012-10-31 Misao Sasaki

We study non-linear primordial adiabatic and isocurvature perturbations and their non-Gaussianity. After giving a general formulation in the context of an extended delta N-formalism, we analyse in detail two illustrative examples. The first…

天体物理学 · 物理学 2010-04-30 David Langlois , Filippo Vernizzi , David Wands

We discuss generation of non-Gaussianity in density perturbation through the super-horizon evolution during inflation by using the so-called $\delta N$ formalism. We first provide a general formula for the non-linearity parameter generated…

宇宙学与河外天体物理 · 物理学 2014-11-20 Takahiro Tanaka , Teruaki Suyama , Shuichiro Yokoyama

The perturbation of a light field might affect preheating and hence generate a contribution to the spectrum and non-gaussianity of the curvature perturbation \zeta. The field might appear directly in the preheating model (curvaton-type…

高能物理 - 唯象学 · 物理学 2011-03-18 Kazunori Kohri , David H. Lyth , Cesar A. Valenzuela-Toledo

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…

天体物理学 · 物理学 2009-11-11 Karim A. Malik , David H. Lyth

In the framework of formal deformation quantization, we apply our formal moment map construction on the space of almost complex structures to recover the Donaldson-Fujiki moment map picture of the Hermitian scalar curvature. In the…

辛几何 · 数学 2022-11-10 Laurent La Fuente-Gravy

The $\delta N$ formalism has been the major computational tool to study the superhorizon evolution of the scalar type perturbation sourced by scalar fields. Recently, this formalism was generalized to compute an arbitrary scalar, vector,…

广义相对论与量子宇宙学 · 物理学 2024-09-30 Takahiro Tanaka , Yuko Urakawa

We show that in the single component situation all perturbation variables in the comoving gauge are conformally invariant to all perturbation orders. Generally we identify a special time slicing, the uniform-conformal transformation…

广义相对论与量子宇宙学 · 物理学 2015-05-28 Jinn-Ouk Gong , Jai-chan Hwang , Wan Il Park , Misao Sasaki , Yong-Seon Song

According to the equivalence principal, the long wavelength perturbations must not have any dynamical effect on the short scale physics up to ${\cal O} (k_L^2/k_s^2)$. Their effect can be always absorbed to a coordinate transformation…

宇宙学与河外天体物理 · 物理学 2018-08-29 Ali Akbar Abolhasani , Misao Sasaki

We argue that the curvaton decay takes place most naturally by way of a broad parametric resonance. The mechanism is analogous to resonant inflaton decay but does not require any tuning of the curvaton coupling strength to other scalar…

天体物理学 · 物理学 2014-11-18 K. Enqvist , S. Nurmi , G. I. Rigopoulos

Modulated (p)reheating is thought to be an alternative mechanism for producing super-horizon curvature perturbations in CMB. But large non-gaussianity and iso-curvature perturbations produced by this mechanism rule out its acceptability as…

宇宙学与河外天体物理 · 物理学 2016-06-22 Arindam Mazumdar , Kamakshya Prasad Modak

We study the contribution to the primordial curvature perturbation on observational scales generated by the reheating field in massless preheating. To do so we use lattice simulations and a recent extension to the $\delta N$ formalism. The…

宇宙学与河外天体物理 · 物理学 2019-09-04 Shailee V. Imrith , David J. Mulryne , Arttu Rajantie

We study non-gaussianity effects, using the $\delta N$ formalism, in a multi-field inflationary model consisting of K\"ahler moduli derived from type IIB string compactification in the large volume limit. The analytical work in this paper…

高能物理 - 理论 · 物理学 2010-10-19 Per Berglund , Guoqin Ren

We investigate the curvaton dynamics and the non-linearity parameters in curvaton model with potential slightly deviating from the quadratic form in detail. The non-linearity parameter $g_{NL}$ will show up due to the curvaton…

高能物理 - 理论 · 物理学 2009-03-27 Qing-Guo Huang , Yi Wang

We analyse the primordial density perturbation when it is generated by a `curvaton' field different from the inflaton. In some cases this perturbation may have large isocurvature components, fully correlated or anti-correlated with the…

天体物理学 · 物理学 2009-07-09 David H. Lyth , Carlo Ungarelli , David Wands

We compute the super-Hubble evolution of non-Gaussianity of primordial curvature perturbations in two-field inflation models by employing two formalisms: delta N and covariant formalisms. Although two formalisms treat the evolution of…

宇宙学与河外天体物理 · 物理学 2013-05-30 Yuki Watanabe