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相关论文: Anisotropic Inflation with Non-Abelian Gauge Kinet…

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In presence of Gauss-Bonnet corrections, we study anisotropic inflation aided by a massless $SU(2)$ gauge field where both the gauge field and the Gauss-Bonnet term are non-minimally coupled to the inflaton. In this scenario, under…

高能物理 - 理论 · 物理学 2017-01-18 Sayantani Lahiri

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

In [arXiv:1102.1513] we introduced an inflationary scenario, Non-Abelian Gauge Field Inflation or gauge-flation for short, in which slow-roll inflation is driven by non-Abelian gauge field minimally coupled to gravity. We present a more…

高能物理 - 唯象学 · 物理学 2015-03-18 A. Maleknejad , M. M. Sheikh-Jabbari

In axion gauge field inflation an axion-like particle driving cosmic inflation is coupled to the Chern-Simons density of an Abelian or non-Abelian gauge group. In the case of a non-Abelian gauge group, this can lead to the formation of a…

宇宙学与河外天体物理 · 物理学 2019-09-24 Valerie Domcke , Stefan Sandner

We study an inflationary scenario in supergravity model with a gauge kinetic function. We find exact anisotropic power-law inflationary solutions when both the potential function for an inflaton and the gauge kinetic function are…

高能物理 - 理论 · 物理学 2011-03-10 Sugumi Kanno , Jiro Soda , Masa-aki Watanabe

Inflationary models are usually based on dynamics of one or more scalar fields coupled to gravity. In this work we present a new class of inflationary models, gauge-flation or non-Abelian gauge field inflation, where slow-roll inflation is…

高能物理 - 唯象学 · 物理学 2015-03-18 A. Maleknejad , M. M. Sheikh-Jabbari

We study anisotropic inflation in non-minimal derivative coupling model where the scalar field non-minimally coupled to the $U(1)$ gauge fields and derivative of the scalar field non-minimally coupled to the Einstein tensor. Within the…

高能物理 - 理论 · 物理学 2022-11-29 Parviz Goodarzi

We present a review of vector field models of inflation and, in particular, of the statistical anisotropy and non-Gaussianity predictions of models with SU(2) vector multiplets. Non-Abelian gauge groups introduce a richer amount of…

宇宙学与河外天体物理 · 物理学 2015-05-18 Emanuela Dimastrogiovanni , Nicola Bartolo , Sabino Matarrese , Antonio Riotto

We study curvature perturbations in the anisotropic inflationary model with a complex scalar field charged under a $U(1)$ gauge field in Bianchi I universe. Due to Abelian Higgs mechanism, the gauge field receives an additional longitudinal…

高能物理 - 理论 · 物理学 2015-06-12 Razieh Emami , Hassan Firouzjahi

Correlated adiabatic and isocurvature perturbation modes are produced during inflation through an oscillation mechanism when extra scalar degrees of freedom other than the inflaton field are present. We show that this correlation…

高能物理 - 唯象学 · 物理学 2009-11-07 N. Bartolo , S. Matarrese , A. Riotto

We study anisotropic inflation in the Brans-Dicke gravity in the presence of an abelian gauge field where the gauge field is non-minimally coupled to the inflaton. We show that the degree of anisotropy, under slow-roll approximations, is…

广义相对论与量子宇宙学 · 物理学 2017-11-03 M. Tirandari , Kh. Saaidi

We examine cosmological perturbations in a dynamical theory of inflation in which an Abelian gauge field couples directly to the inflaton, breaking conformal invariance. When the coupling between the gauge field and the inflaton takes a…

宇宙学与河外天体物理 · 物理学 2010-10-13 Timothy R. Dulaney , Moira I. Gresham

We study an inflationary scenario with a two-form field to which an inflaton couples non-trivially. First, we show that anisotropic inflation can be realized as an attractor solution and that the two-form hair remains during inflation. A…

宇宙学与河外天体物理 · 物理学 2013-05-16 Junko Ohashi , Jiro Soda , Shinji Tsujikawa

Recent observations opened up a new window on the inflationary model building. As it was firstly reported by the WMAP data, there may be some indications of statistical anisotropy on the CMB map, although the statistical significance of…

宇宙学与河外天体物理 · 物理学 2015-11-06 Razieh Emami

The shift-symmetric coupling of a pseudo-scalar particle driving inflation to gauge fields provides a unique way of probing cosmic inflation. We show for an SU(2) gauge group how a classical isotropic background gauge field develops from…

高能物理 - 唯象学 · 物理学 2019-04-24 Valerie Domcke , Ben Mares , Francesco Muia , Mauro Pieroni

Anisotropic inflation is an interesting model with an U(1) gauge field and it predicts the statistical anisotropy of the curvature perturbation characterized by a parameter $g_*$. However, we find that the background gauge field does not…

宇宙学与河外天体物理 · 物理学 2018-02-14 Tomohiro Fujita , Ippei Obata

In this paper we study non-abelian gauge field inflation (gauge-flation) model in the context of intermediate and logamediate scenario. Important parameters of this model are presented for these two cases. Numerical study shows that the…

广义相对论与量子宇宙学 · 物理学 2014-01-08 M. R. Setare , V. Kamali

We develop a possibility of generating tensor non-Gaussianity in a kind of anisotropic inflation, where a $U(1)$ gauge field is kinetically coupled to a spectator scalar field. Owing to this coupling, the coherent mode of the electric field…

宇宙学与河外天体物理 · 物理学 2021-03-31 Takashi Hiramatsu , Kai Murai , Ippei Obata , Shuichiro Yokoyama

Recently, a new class of inflationary models, so called \emph{gauge-flation} or non-Abelian gauge field inflation has been introduced where the slow-roll inflation is driven by a non-Abelian gauge field $\textbf{A}$ with the field strength…

高能物理 - 理论 · 物理学 2014-10-01 F. Darabi , A. Parsiya

In this paper we study some models where non-Abelian gauge vector fields endowed with a SU(2) group representation are the unique source of inflation and dark energy. These models were first introduced under the name of gaugeflation and…

广义相对论与量子宇宙学 · 物理学 2020-10-13 Alejandro Guarnizo , J. Bayron Orjuela-Quintana , César A. Valenzuela-Toledo
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