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相关论文: Tilted Hybrid Inflation

200 篇论文

Recently, it has been found that complete resolution of the Hubble tension might point to a scale-invariant Harrison-Zeldovich spectrum of primordial scalar perturbation, i.e. $n_s=1$ for $H_0\sim 73$km/s/Mpc. We show that for well-known…

宇宙学与河外天体物理 · 物理学 2022-12-14 Gen Ye , Jun-Qian Jiang , Yun-Song Piao

The curvaton and the inhomogeneous reheating scenarios for the generation of the cosmological curvature perturbation on large scales represent an alternative to the standard slow-roll scenario where the observed density perturbations are…

天体物理学 · 物理学 2009-11-10 L. Pilo , A. Riotto , A. Zaffaroni

A field kinetic coupling with the Einstein tensor leads to a gravitationally enhanced friction during inflation, by which even steep potentials with theoretically natural model parameters can drive cosmic acceleration. In the presence of…

宇宙学与河外天体物理 · 物理学 2015-06-03 Shinji Tsujikawa

In this paper we will analyze generic predictions of an inflection-point model of inflation with Hubble-induced corrections and study them in light of the Planck data. Typically inflection-point models of inflation can be embedded within…

高能物理 - 唯象学 · 物理学 2013-07-29 Sayantan Choudhury , Anupam Mazumdar , Supratik Pal

We review the main aspects of the warm inflation scenario, focusing on the inflationary dynamics and the predictions related to the primordial spectrum of perturbations, to be compared with the recent cosmological observations. We study in…

高能物理 - 唯象学 · 物理学 2010-04-21 Mar Bastero-Gil , Arjun Berera

Extending our previous work on the robustness of inflation to perturbations in the scalar field, we investigate the effects of perturbations in the transverse traceless part of the extrinsic curvature on the evolution of an inhomogeneous…

高能物理 - 理论 · 物理学 2018-06-12 Katy Clough , Raphael Flauger , Eugene A. Lim

The tensor fraction $r\simeq 0.16$ found by BICEP2 corresponds to a Hubble parameter $H\simeq 1.0\times 10^{14}\GeV$ during inflation. This has two implications for the (single-field) slow-roll inflation hypothesis. First, the inflaton…

高能物理 - 唯象学 · 物理学 2015-06-19 David H. Lyth

We consider a class of multi-component hybrid inflation models whose evolution may be analytically solved under the slow-roll approximation. We call it multi-brid inflation (or $n$-brid inflation where $n$ stands for the number of inflaton…

天体物理学 · 物理学 2009-10-09 Misao Sasaki

The cosmological curvature perturbation may be generated when some `curvaton' field, different from the inflaton, oscillates in a background of unperturbed radiation. In its simplest form the curvaton paradigm requires the Hubble parameter…

高能物理 - 理论 · 物理学 2008-11-26 David H. Lyth

We investigate density perturbations in the chain inflation scenario, where the inflaton undergoes successive tunneling transitions along one field direction. First we show that when the bubble walls associated with such a phase transition…

高能物理 - 理论 · 物理学 2015-05-28 James M. Cline , Guy D. Moore , Yi Wang

It is pointed out that hybrid inflation can be implemented with the inflaton field rolling away from the origin instead of towards it. This `inverted' hybrid inflation has a spectral index $ n < 1 $, in contrast with ordinary hybrid…

高能物理 - 唯象学 · 物理学 2008-11-26 David H. Lyth , Ewan D. Stewart

A double hybrid inflationary scenario in non-minimal supergravity which can predict values of the tensor-to-scalar ratio up to about 0.05 is presented. Larger values of this ratio would require unacceptably large running of the scalar…

高能物理 - 唯象学 · 物理学 2015-10-27 G. Lazarides , C. Panagiotakopoulos

In this paper, we explore a novel observational signature of gravitational corrections during slow-roll inflation. We study the coupling of the inflaton field to higher-curvature tensors in models with a minimal breaking of conformal…

高能物理 - 理论 · 物理学 2016-02-17 Daniel Baumann , Hayden Lee , Guilherme L. Pimentel

We argue that in models of inflation with two scalar fields and non-canonical kinetic terms there is a possibility of obtaining a red tilt of the power spectrum of curvature perturbations from noncanonicality-induced interactions between…

高能物理 - 理论 · 物理学 2015-03-17 Sera Cremonini , Zygmunt Lalak , Krzysztof Turzynski

Most models of inflation have small parameters, either to guarantee sufficient inflation or the correct magnitude of the density perturbations. In this paper we show that, in supersymmetric theories with weak scale supersymmetry breaking,…

高能物理 - 唯象学 · 物理学 2007-05-23 Lisa Randall , Marin Soljacic , Alan Guth

Hybrid Higgs inflation model is a hybrid type of the so-called Higgs inflation model with the conventional non-minimal $\xi$ coupling to a scalar curvature $R$ and new Higgs inflation model with the derivative coupling to the Einstein…

广义相对论与量子宇宙学 · 物理学 2020-05-20 Seiga Sato , Kei-ichi Maeda

We discuss metric perturbations produced during a period of inflation in the early universe where two scalar fields evolve. The final scalar perturbation spectrum can be calculated in terms of the perturbed expansion along neighbouring…

天体物理学 · 物理学 2007-05-23 David Wands , Juan Garcia-Bellido

We explore extensions of hybrid inflationary models in the context of supersymmetric D-term inflation. We point out that a large variety of inflationary scenarios can be encountered when the field content is extended. It is not only…

高能物理 - 唯象学 · 物理学 2008-11-26 Francis Bernardeau , Tristan Brunier

We realize and study a model of hybrid inflation in the context of softly broken supersymmetry. The inflaton is taken to be a flat direction in the superfield space and, due to unsuppressed couplings, its soft supersymmetry breaking mass…

高能物理 - 唯象学 · 物理学 2016-08-25 Laura Covi

Recent arguments show that some curvaton field may generate the cosmological curvature perturbation. As the curvaton is independent of the inflaton field, there is a hope that the fine-tunings of inflation models can be cured by the…

高能物理 - 唯象学 · 物理学 2009-11-10 Tomohiro Matsuda