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相关论文: $\beta$-function formalism for inflationary models…

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Attractor inflation is a particularly robust framework for developing inflationary models that are insensitive to the details of the potential. Such models are most often considered in the metric formulation of gravity. However, non-minimal…

广义相对论与量子宇宙学 · 物理学 2021-11-03 Alexandros Karam , Sotirios Karamitsos , Margus Saal

We study symmetry-breaking inflation within the framework of metric-affine gravity. By introducing a non-minimal coupling, $\beta(\phi)\tilde{\cal R}$, between the Holst invariant and the inflaton, both small-field and large-field…

广义相对论与量子宇宙学 · 物理学 2025-05-28 Ioannis D. Gialamas , Antonio Racioppi

Once quantum corrections are taken into account, the strong coupling limit of the $\xi$-attractor models (in metric gravity) might depart from the usual Starobinsky solution and move into linear inflation. Furthermore, it is well known that…

宇宙学与河外天体物理 · 物理学 2018-07-18 Antonio Racioppi

We introduce a novel non-minimal coupling between gravity and the inflaton sector. Remarkably, for large values of this coupling all models asymptote to a universal attractor. This behavior is independent of the original scalar potential…

高能物理 - 理论 · 物理学 2015-06-17 Renata Kallosh , Andrei Linde , Diederik Roest

Classifying inflationary scenarios according to their scaling properties is a powerful way to connect theory with observations. A useful tool to make such a classification is the beta-function formalism. By describing inflation in terms of…

宇宙学与河外天体物理 · 物理学 2019-10-02 Francesco Cicciarella , Joel Mabillard , Mauro Pieroni , Angelo Ricciardone

We investigate the predictions of inflation models with a non-minimal coupling to gravity for inflationary observables such as the spectral index and tensor-to-scalar ratio in a general setting. We argue that, depending on the relation…

宇宙学与河外天体物理 · 物理学 2022-04-13 Tatsuki Kodama , Tomo Takahashi

In this work, we study constant-roll inflation driven by a scalar field with non-minimal derivative coupling to gravity, via the Einstein tensor. This model contains a free parameter, $\eta$, which quantifies the non-minimal derivative…

广义相对论与量子宇宙学 · 物理学 2019-10-23 A. Oliveros , Hernán E. Noriega

We consider two classes of non-minimally coupled inflation models; those with a quadratic coupling of the inflaton to gravity, and the `Universal Attractor' models where the coupling is connected to the potential. We make a detailed…

宇宙学与河外天体物理 · 物理学 2015-06-22 David C. Edwards , Andrew R. Liddle

We investigate models in which the inflaton emerges as a composite field of a four dimensional, strongly interacting and nonsupersymmetric gauge theory featuring purely fermionic matter. We show that it is possible to obtain successful…

高能物理 - 唯象学 · 物理学 2011-05-12 Phongpichit Channuie , Jakob Jark Joergensen , Francesco Sannino

We study a new anisotropic inflation model, with an inflaton field nonminimally coupled with the gravity and a vector field. We find that the anisotropic attractor solution exists not only in the weak curvature coupling limit, but more…

广义相对论与量子宇宙学 · 物理学 2015-06-19 Bin Chen , Zhuang-wei Jin

Recently we identified a new class of (super)conformally invariant theories which allow inflation even if the scalar potential is very steep in terms of the original conformal variables. Observational predictions of a broad class of such…

高能物理 - 理论 · 物理学 2015-06-16 Renata Kallosh , Andrei Linde

Motivated by the recent `Higgs-inflation' scenario based on a single inflaton field, we consider more generic two-field inflation with non-minimal coupling term. The generic analytic expressions are derived for cosmological observables with…

高能物理 - 唯象学 · 物理学 2015-03-13 Jinsu Kim , Yoonbai Kim , Seong Chan Park

We propose a new mechanism for inflationary model building in the framework of metric-affine gravity. Such a mechanism involves an inflaton non-minimally coupled with the Holst invariant. If the non-minimal coupling function has a zero…

广义相对论与量子宇宙学 · 物理学 2026-04-21 Antonio Racioppi

In this paper, we explore the inflationary dynamics of the $\beta$-exponential potential model, where a scalar field couples to quadratic $(R + R^2)$ gravity. In this model, the inflaton is the field that determines the size of the extra…

广义相对论与量子宇宙学 · 物理学 2026-01-15 Ozan Sargın

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

Models of inflation in which the Higgs field is non-minimally coupled to gravity lead, after a recaling of the metric, to a complicated expression for the potential of the inflaton field. Nevertheless, this potential produces the desired…

高能物理 - 理论 · 物理学 2022-06-08 Noureddine Mohammedi

The slow-roll approximation to inflation is ultimately justified by the presence of inflationary attractors for the orbits of the solutions of the dynamical equations in phase space. There are many indications that the inflaton field…

广义相对论与量子宇宙学 · 物理学 2011-08-11 Valerio Faraoni

The supersymmetric extension of "Starobinsky" $R+\alpha R^2$ models of inflation is particularly simple in the "new minimal" formalism of supergravity, where the inflaton has no scalar superpartners. This paper is devoted to matter…

高能物理 - 理论 · 物理学 2015-06-22 S. Ferrara , M. Porrati

Inflationary slow-roll dynamics in Einstein gravity with a non-minimal scalar-curvature coupling can be equivalent to that in the certain f(R) gravity theory. We review the correspondence and extend it to N=1 supergravity. The non-minimal…

高能物理 - 理论 · 物理学 2015-06-04 Sergei V. Ketov , Alexei A. Starobinsky

This work is focused on the study of early time cosmology and in particular on the study of inflation. After an introduction on the standard Big Bang theory, we discuss the physics of CMB and we explain how its observations can be used to…

广义相对论与量子宇宙学 · 物理学 2016-11-14 Mauro Pieroni
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