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We investigate a new mechanism to create large curvature perturbations on small scales due to parameter resonance in a single-field inflationary model with a small periodic structure upon the potential. After reentering the horizon, the…

宇宙学与河外天体物理 · 物理学 2020-06-17 Rong-Gen Cai , Zong-Kuan Guo , Jing Liu , Lang Liu , Xing-Yu Yang

The impact of particle production during inflation on the primordial curvature perturbation spectrum is investigated both analytically and numerically. We obtain an oscillatory behavior on small scales, while on large scales the spectrum is…

广义相对论与量子宇宙学 · 物理学 2009-02-23 Antonio Enea Romano , Misao Sasaki

We develop methods to calculate the curvature power spectrum in models where features in the inflaton potential nonlinearly excite modes and generate high frequency features in the spectrum. The first nontrivial effect of excitations…

宇宙学与河外天体物理 · 物理学 2018-09-18 V Miranda , Wayne Hu , Chen He , Hayato Motohashi

Inflation is often described through the dynamics of a scalar field, slow-rolling in a suitable potential. Ultimately, this inflaton must be identified as the expectation value of a quantum field, evolving in a quantum effective potential.…

高能物理 - 唯象学 · 物理学 2021-05-11 Jens O. Andersen , Magdalena Eriksson , Anders Tranberg

The behaviour of quantum metric perturbations produced during inflation is considered at the stage after the second Hubble radius crossing. It is shown that the classical correlation between amplitude and momentum of a perturbation mode,…

广义相对论与量子宇宙学 · 物理学 2010-04-06 Claus Kiefer , Julien Lesgourgues , David Polarski , Alexei A. Starobinsky

We study primordial tensor power-spectra generated during inflation in bimetric gravity. More precisely, we examine a homogeneous expanding spacetime in a minimal bimetric model with an inflaton and calculate tensor perturbations on the…

高能物理 - 理论 · 物理学 2015-09-18 Yuki Sakakihara , Jiro Soda

We use a numerical code to compute the density perturbations generated during an inflationary epoch which includes a spontaneous symmetry breaking phase transition. A sharp step in the inflaton potential generates $k$ dependent oscillations…

天体物理学 · 物理学 2009-11-06 Jennifer Adams , Bevan Cresswell , Richard Easther

We develop a variant of the generalized slow roll approach for calculating the curvature power spectrum that is well-suited for order unity deviations in power caused by sharp features in the inflaton potential. As an example, we show that…

宇宙学与河外天体物理 · 物理学 2010-07-07 Cora Dvorkin , Wayne Hu

We study an inflationary scenario where thermal inflation is followed by fast-roll inflation. This is a rather generic possibility based on the effective potentials of spontaneous symmetry breaking in the context of particle physics models.…

高能物理 - 唯象学 · 物理学 2008-11-26 Jinn-Ouk Gong

We exploit a new numerical technique for evaluating the tree order contributions to the primordial scalar and tensor power spectra for scalar potential models of inflation. Among other things we use the formalism to develop a good analytic…

宇宙学与河外天体物理 · 物理学 2017-09-06 D. J. Brooker , N. C. Tsamis , R. P. Woodard

We investigate possible signatures of a pre-inflationary anisotropic phase in two-point and three-point correlation functions of the curvature perturbation for high-momentum modes which exit the horizon after isotropization. In this…

高能物理 - 理论 · 物理学 2015-05-28 Anindya Dey , Sonia Paban

We investigate the formation of large peaks in the inflationary curvature power spectrum from double-well potentials. In such scenarios, the initial CMB spectrum is created at large field values. Subsequently, the inflaton will cross one of…

宇宙学与河外天体物理 · 物理学 2023-09-06 Alexandros Karam , Niko Koivunen , Eemeli Tomberg , Antonio Racioppi , Hardi Veermäe

In this work we determine the power spectrum of the gravitational potential of the primordial fluctuations for an inflationary model whose \emph{inflaton} is a non-canonical scalar field of the tachyon-type. The respective background field…

广义相对论与量子宇宙学 · 物理学 2015-06-12 Rudinei C. de Souza , Gilberto M. Kremer

The first year of observations by the Planck satellite mission shows that the cosmic microwave background (CMB) fluctuations are consistent with gaussian statistics in the primordial perturbations, a key prediction of the simplest models of…

宇宙学与河外天体物理 · 物理学 2015-10-19 Ana Achucarro , Vicente Atal , Pablo Ortiz , Jesus Torrado

We carried out numerical calculations of a contribution of the waterfall field to the primordial curvature perturbation (on uniform density hypersurfaces) $\zeta$, which is produced during waterfall transition in hybrid inflation scenario.…

宇宙学与河外天体物理 · 物理学 2011-11-17 Edgar Bugaev , Peter Klimai

We have calculated the third order moments of scalar curvature perturbations in configuration space for different inflationary models. We developed a robust numerical technique to compute the bispectrum for different models that have some…

高能物理 - 理论 · 物理学 2015-08-26 M. Junaid , D. Pogosyan

We study the generation of a localized peak in the primordial spectrum of curvature perturbations from a transient dissipative phase during inflation, leading to a large population of primordial black holes. The enhancement of the power…

宇宙学与河外天体物理 · 物理学 2024-02-16 Guillermo Ballesteros , Marcos A. G. García , Alejandro Pérez Rodríguez , Mathias Pierre , Julián Rey

We report first study of complex field inflation. Although understood as a specific two-field inflation, a complex field inflation is able to make more robust model predictions on primordial curvature perturbation. Explicitly we discuss the…

宇宙学与河外天体物理 · 物理学 2022-02-22 Ruopeng Zhang , Sibo Zheng

During the inflationary epoch,geometry of the universe may be described by quasi-de Sitter space. On the other hand,maximally extended de Sitter metric in the comoving coordinates accords with a special FLRW model with positive spatial…

广义相对论与量子宇宙学 · 物理学 2016-01-20 A. A. Asgari , A. H. Abbassi

We give the initial spectrum of quantized gravitational waves in the context of the one-bubble open inflationary universe scenario. In determining the quantum state after the bubble nucleation we adopt the prescription to require the…

天体物理学 · 物理学 2009-10-09 Takahiro Tanaka , Misao Sasaki
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