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相关论文: General $f(R)$ and conformal inflation from minima…

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The method of a conformal transformation is applied to a general class of single field inflation models with non-minimal coupling to gravity and non-standard kinetic terms, in order to reduce the cosmological perturbative calculation to the…

广义相对论与量子宇宙学 · 物理学 2012-03-19 Takahiro Kubota , Nobuhiko Misumi , Wade Naylor , Naoya Okuda

We discuss a model of gravity with conformal symmetry appearing in the simplest extension of General Relativity with the Poincar\'e algebra terms. The nonlinear realization of symmetry causes the existence of five scalar fields. Therefore…

广义相对论与量子宇宙学 · 物理学 2021-11-18 S. Alexeyev , D. Krichevskiy

We study cosmological perturbations in generalized Einstein scenarios and show the equivalence of inflationary observables both in the Jordan frame and the Einstein frame. In particular the consistency relation relating the tensor-to-scalar…

天体物理学 · 物理学 2010-11-23 Shinji Tsujikawa , Burin Gumjudpai

In this work we study a modified version of $f(R)$ gravity in which higher order kinetic terms of a scalar field are added in the action of vacuum $f(R)$ gravity. This type of theory is a type of $k$-essence $f(R)$ gravity, and it belongs…

广义相对论与量子宇宙学 · 物理学 2019-03-27 S. Nojiri , S. D. Odintsov , V. K. Oikonomou

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

In the context of Palatini gravity, $F(R+X)$ models, with X the inflaton kinetic term, are characterized by the appealing property of generating asymptotically flat inflaton potentials, exactly like the more commonly studied Palatini $F(R)$…

广义相对论与量子宇宙学 · 物理学 2025-12-22 N. Bostan , R. H. Dejrah , C. Dioguardi , A. Racioppi

We investigate the inflationary attractors in models of inflation inspired from general conformal transformation of general scalar-tensor theories to the Einstein frame. The coefficient of the conformal transformation in our study depends…

广义相对论与量子宇宙学 · 物理学 2019-07-31 Khamphee Karwan , Phongpichit Channuie

It is likely that the Higgs potential of the Standard Model is unstable, turning negative at $\phi < \Lambda \sim 10^{10}$ GeV. Here we consider whether it is possible to have Higgs Inflation on the positive stable region of the potential…

高能物理 - 唯象学 · 物理学 2023-09-14 John McDonald

In this paper, we worked in the framework of an inflationary $f(R,T)$ theory, in the presence of a canonical scalar field. More specifically, the $f(R,T)=\gamma R+2\kappa\alpha T$ gravity. The values of the dimensionless parameters $\alpha$…

广义相对论与量子宇宙学 · 物理学 2023-08-01 V. K. Oikonomou , Konstantinos-Rafail Revis , Ilias C. Papadimitriou , Maria-Myrto Pegioudi

We construct models of inflation with many randomly interacting fields and use these to study the generation of cosmological observables. We model the potentials as multi-dimensional Gaussian random fields (GRFs) and identify powerful…

宇宙学与河外天体物理 · 物理学 2018-02-28 Theodor Bjorkmo , M. C. David Marsh

In the general framework of Metric-Affine theories of gravity, where the metric and the connection are independent variables, we consider actions quadratic in the Ricci scalar curvature and the Holst invariant (the contraction of the…

广义相对论与量子宇宙学 · 物理学 2023-03-21 Ioannis D. Gialamas , Kyriakos Tamvakis

In this paper we study some classes of $\alpha$-attractors models in the Jordan frame and we find the corresponding $F(R)$ gravity theory. We study analytically the problem at leading order and we investigate whether the attractor picture…

广义相对论与量子宇宙学 · 物理学 2017-01-04 S. D. Odintsov , V. K. Oikonomou

Since the building-blocks of supersymmetric models include chiral superfields containing pairs of effective scalar fields, a two-field approach is particularly appropriate for models of inflation based on supergravity. In this paper, we…

高能物理 - 唯象学 · 物理学 2015-06-23 John Ellis , Marcos A. G. Garcia , Dimitri V. Nanopoulos , Keith A. Olive

The generality of inflation in closed FRW Universe is studied for the models with a scalar field on a brane and with a complex scalar field. The results obtained are compared with the previously known results for the model with a scalar…

广义相对论与量子宇宙学 · 物理学 2009-11-07 S. A. Pavluchenko , N. Yu. Savchenko , A. V. Toporensky

In this paper, we study two inflationary models, namely, monomial inflation and the simplest $\alpha$-attractor inflation, within extra-dimensional frameworks. We consider three extra-dimensional setups: Dark Dimension, which embeds one…

高能物理 - 唯象学 · 物理学 2026-01-07 Nicolás Bernal , Catarina Cosme , Andrea Donini , Nuria Rius

In a series of recent papers Kallosh, Linde, and collaborators have provided a unified description of single-field inflation with several types of potentials, ranging from power law to supergravity, in terms of just one parameter $\alpha$.…

高能物理 - 理论 · 物理学 2016-02-03 Massimiliano Rinaldi , Luciano Vanzo , Sergio Zerbini , Giovanni Venturi

We explore two saddle point inflationary scenarios in the context of higher order corrections related to different generalisations of general relativity. Firstly, we deal with Jordan frame Starobinsky potential, for which we identify a…

高能物理 - 理论 · 物理学 2016-02-17 Michal Artymowski , Zygmunt Lalak , Marek Lewicki

We elaborate on the predictions of the imaginary Starobinsky model of inflation coupled to matter, where the inflaton is identified with the imaginary part of the inflaton multiplet suggested by the Supergravity embedding of a pure R + R^2…

高能物理 - 理论 · 物理学 2016-01-20 Sergio Ferrara , Alex Kehagias , Antonio Riotto

We consider global issues in minimal supergravity models where a single field inflaton potential emerges. In a particular case we reproduce the Starobinsky model and its description dual to a certain formulation of R+R^2 supergravity. For…

高能物理 - 理论 · 物理学 2015-06-18 Sergio Ferrara , Pietro Fre , Alexander S. Sorin

Various scenarios of the initial inflation of the universe are distinguished by the choice of a scalar field {\em potential} $U(\phi)$ which simulates a {\it temporarily} non--vanishing {\em cosmological term}. Our new method, which…

广义相对论与量子宇宙学 · 物理学 2009-10-22 Fjodor V. ~Kusmartsev , Eckehard W. ~Mielke , Yuri N. ~Obukhov , Franz E. ~Schunck