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相关论文: Attractor Behaviour in Multifield Inflation

200 篇论文

We study the phenomenology of the Higgs-Dilaton model in the context of Einstein-Cartan gravity, focusing on the separate impact of the Holst and Nieh-Yan terms on the inflationary observables. Using analytical and numerical techniques, we…

广义相对论与量子宇宙学 · 物理学 2022-05-18 Matteo Piani , Javier Rubio

We reconsider an inflationary model that inflaton field is non-minimally coupled to gravity. We study parameter space of the model up to the second ( and in some cases third ) order of the slow-roll parameters. We calculate inflation…

广义相对论与量子宇宙学 · 物理学 2014-11-21 Kourosh Nozari , S. Shafizadeh

In this work, we study the $f(R)$ models of inflation in the context of gravity's rainbow theory. We choose three types of $f(R)$ models: $f(R)=R+\alpha (R/M)^{n},\,f(R)=R+\alpha R^{2}+\beta R^{2}\log(R/M^{2})$ and the Einstein-Hu-Sawicki…

广义相对论与量子宇宙学 · 物理学 2020-09-02 Areef Waeming , Phongpichit Channuie

We emphasize the importance of effects from heavy fields on supergravity models of inflation. We study, in particular, the backreaction of stabilizer fields and geometric moduli in the presence of supersymmetry breaking. Many effects do not…

高能物理 - 理论 · 物理学 2015-10-12 Emilian Dudas , Clemens Wieck

We study a model of quintessential inflation constructed in $R^2$ modified gravity with a non-minimally coupled scalar field, in the Palatini formalism. Our non-minimal inflaton field is characterised by a simple exponential potential. We…

广义相对论与量子宇宙学 · 物理学 2022-04-21 Konstantinos Dimopoulos , Alexandros Karam , Samuel Sánchez López , Eemeli Tomberg

We compute the amplitude of the non-Gaussianities in inflationary models with multiple, uncoupled scalar fields. This calculation thus applies to all models of assisted inflation, including N-flation, where inflation is driven by multiple…

天体物理学 · 物理学 2010-10-27 Thorsten Battefeld , Richard Easther

We study inflationary models in which the effective potential of the inflaton field does not have a minimum, but rather gradually decreases at large $\phi$. In such models the inflaton field does not oscillate after inflation, and its…

高能物理 - 唯象学 · 物理学 2009-09-29 Gary Felder , Lev Kofman , Andrei Linde

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 investigate the inflation for the quartic hilltop model via a certain type of modified gravity. Precisely, we analyze the $F(\phi) T$ term in the Einstein's gravity to examine the quartic hilltop inflation model. $T$ is the trace of the…

广义相对论与量子宇宙学 · 物理学 2025-07-28 Feyzollah Younesizadeh , Davoud Kamani

During inflation, higher derivative terms in the gravitational action may play a significant role. Building on new stable formulations of four-derivative scalar-tensor theories, we study the impact of these corrections in the case where the…

广义相对论与量子宇宙学 · 物理学 2025-05-26 Sam E. Brady , Katy Clough , Pau Figueras , Áron D. Kovács

We present the model-independent studies of non attractor inflation in the context of effective field theory (EFT) of inflation. Within the EFT approach two independent branches of non-attractor inflation solutions are discovered in which a…

高能物理 - 理论 · 物理学 2015-08-06 Mohammad Akhshik , Hassan Firouzjahi , Sadra Jazayeri

Fibre inflation is a specific string theory construction based on the Large Volume Scenario that produces an inflationary plateau. We outline its relation to $\alpha$-attractor models for inflation, with the cosmological sector originating…

高能物理 - 理论 · 物理学 2018-04-04 Renata Kallosh , Andrei Linde , Diederik Roest , Alexander Westphal , Yusuke Yamada

Using the universal X superfield that measures in the UV the violation of conformal invariance we build up a model of multifield inflation. The underlying dynamics is the one controlling the natural flow of this field in the IR to the…

高能物理 - 理论 · 物理学 2011-07-19 Luis Alvarez-Gaume , Cesar Gomez , Raul Jimenez

We consider models of inflation with U(1) gauge fields and charged scalar fields including symmetry breaking potential, chaotic inflation and hybrid inflation. We show that there exist attractor solutions where the anisotropies produced…

宇宙学与河外天体物理 · 物理学 2011-02-18 Razieh Emami , Hassan Firouzjahi , S. M. Sadegh Movahed , Moslem Zarei

We investigate inflation and its scalar perturbation driven by a massive scalar field in the unimodular theory of gravity. We introduce a parameter $\xi$ with which the theory is invariant under general unimodular coordinate…

广义相对论与量子宇宙学 · 物理学 2015-03-04 Inyong Cho , Naveen K. Singh

The string $\alpha^\prime$-correction to the usual Einstein action comprises a Gauss-Bonnet integrand multiplied by non-trivial functions of the modulus field $\chi$ and/or the dilaton field $\phi$. We discuss how the presence of such terms…

高能物理 - 理论 · 物理学 2007-05-23 Ishwaree P Neupane

The simplicity of the CMB data, so well described by single-field inflation, raises the question whether there might be an equally simple multi-field realization consistent with the observations. We explore the idea that an approximate…

高能物理 - 理论 · 物理学 2019-07-04 Ana Achucarro , Yvette Welling

Recent years have seen the introduction of various multi-field inflationary scenarios in which the curvature and geodesics of the scalar manifold play a crucial role. We outline a simple description that unifies these different proposals…

广义相对论与量子宇宙学 · 物理学 2020-08-14 Perseas Christodoulidis , Diederik Roest , Evangelos I. Sfakianakis

A new model for inflation using modified gravity in the Palatini formalism is constructed. Here non-minimal coupling of scalar field h with the curvature R as a general function f(R,h) is considered. Explicit inflation models for some…

广义相对论与量子宇宙学 · 物理学 2021-05-19 Nayan Das , Sukanta Panda

We investigate a class of inflationary models in modified gravity theories which contain a non-minimal coupling between gravity and a scalar field $\phi$ (inflaton) as $f(R,T)=R \bigl(1+\alpha+ \kappa^4 \beta T \bigr)+\kappa^2\gamma T $…

广义相对论与量子宇宙学 · 物理学 2024-12-03 Payel Sarkar , Ashmita , Prasanta Kumar Das
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