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Cosmological models based on f(R)-gravity may exhibit a natural acceleration mechanism without introducing a dark energy component. In this paper, we investigate cosmological consequences of the so-called Hu-Sawicki f(R)-gravity in the…

宇宙学与河外天体物理 · 物理学 2012-12-13 B. Santos , M. Campista , J. Santos , J. S. Alcaniz

One of the most favourable extensions of General Relativity is the $f(R)$ gravity. $f(R)$ gravity in Palatini formalism can be a realistic alternative to the dark energy problem. In this work we study a recently introduced dark energy…

广义相对论与量子宇宙学 · 物理学 2022-05-20 Dhruba Jyoti Gogoi , Umananda Dev Goswami

Modified gravity, known as $f(R)$ gravity, has presently been applied to Cosmology as a realistic alternative to dark energy. For this kind of gravity the expansion of the Universe may accelerate while containing only baryonic and cold dark…

宇宙学与河外天体物理 · 物理学 2012-05-01 N. Pires , J. Santos , J. S. Alcaniz

Although several models of $f(R)$ theories of gravity within the Palatini approach have been studied already, the interest was concentrated on those that have an effect on the late-time evolution of the universe, by the inclusion for…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Thomas P. Sotiriou

We investigate f(R) theories of gravity within the Palatini approach and show how one can determine the expansion history, H(a), for an arbitrary choice of f(R). As an example, we consider cosmological constraints on such theories arising…

天体物理学 · 物理学 2008-11-26 M. Amarzguioui , O. Elgaroy , D. F. Mota , T. Multamaki

We investigate the modified gravity theories in terms of the effective dark energy models. We compare the cosmic expansion history and the linear growth in different models. We also study the evolution of linear cosmological perturbations…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Seokcheon Lee

We study the formation of large-scale structure in universes dominated by dark matter and driven to accelerated expansion by f(R) gravity in the Palatini formalism. If the dark matter is cold, practically all of these models are ruled out…

天体物理学 · 物理学 2008-11-26 Tomi Koivisto

We discuss recent results on the cosmology of extended theories of gravity formulated in the Palatini approach, i.e., assuming that metric and connection are independent fields. In particular, we focus on the attempts to explain the cosmic…

广义相对论与量子宇宙学 · 物理学 2012-07-23 Gonzalo J. Olmo

We compute the complete post-Newtonian limit of the Palatini form of f(R) gravities using a scalar-tensor representation. By comparing the predictions of these theories with laboratory and solar system experiments, we find a set of…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Gonzalo J. Olmo

Using an approach that treats the Ricci scalar itself as a degree of freedom, we analyze the cosmological evolution within an f(R) model that has been proposed recently (exponential gravity) and that can be viable for explaining the…

广义相对论与量子宇宙学 · 物理学 2012-11-02 Luisa Jaime , Marcelo Salgado , Leonardo Patino

We make a systematic study of the cosmological dynamics for a number of f(R) gravity theories in Palatini formalism. We find a number of interesting results: (i) models based on theories of the type (a) f(R)=R-beta R^n and (b) f(R)=R+alpha…

天体物理学 · 物理学 2008-11-26 Stephane Fay , Reza Tavakol , Shinji Tsujikawa

We investigate the viability of f(R) theories in the framework of the Palatini approach as solutions to the problem of the observed accelerated expansion of the universe. Two physically motivated popular choices for f(R) are considered:…

天体物理学 · 物理学 2009-11-10 S. Capozziello , V. F. Cardone , M. Francaviglia

Here we analysed a particular type of $F(R)$ gravity, the so-called exponential gravity which includes an exponential function of the Ricci scalar in the action. Such term represents a correction to the usual Hilbert-Einstein action. By…

广义相对论与量子宇宙学 · 物理学 2018-01-17 Sergei D. Odintsov , Diego Saez-Chillon Gomez , German S. Sharov

f(R) gravity theories in the Palatini formalism has been recently used as an alternative way to explain the observed late-time cosmic acceleration with no need of invoking either dark energy or extra spatial dimension. However, its…

广义相对论与量子宇宙学 · 物理学 2012-12-07 Janilo Santos , Crislane de Souza Santos

The observed accelerated expansion of the Universe at present epoch can be explained by some of the $f(R)$ models without invoking the existence of dark energy or any other such exotic component in cosmic fluid. The $f(R)$ models in…

宇宙学与河外天体物理 · 物理学 2024-05-09 Kumar Ravi

We investigate a f(R) modification of gravity that is exponential in the Ricci scalar R to explain cosmic acceleration. The steepness of this dependence provides extra freedom to satisfy solar system and other curvature regime constraints.…

宇宙学与河外天体物理 · 物理学 2010-01-07 Eric V. Linder

A class of modified gravity, known as $f(R)$-gravity, has presently been applied to Cosmology as a realistic alternative to dark energy. In this paper we use the most recent Type-Ia Supernova (SNe Ia) data, the so-called \emph{Union} sample…

天体物理学 · 物理学 2014-11-18 J. Santos , J. S. Alcaniz , F. C. Carvalho , N. Pires

We study new FRW type cosmological models of modified gravity treated on the background of Palatini approach. These models are generalization of Einstein gravity by the presence of a scalar field non-minimally coupled to the curvature. The…

广义相对论与量子宇宙学 · 物理学 2012-03-13 A. Borowiec , M. Kamionka , A. Kurek , M. Szydlowski

The approach of dynamical systems is a useful tool to investigate the cosmological history that follows from modified theories of gravity. It provides qualitative information on the typical background solutions in a parametrized family of…

广义相对论与量子宇宙学 · 物理学 2022-01-12 João C. Lobato , Isabela S. Matos , Maurício O. Calvão , Ioav Waga

The current accelerated universe could be produced by modified gravitational dynamics as it can be seen in particular in its Palatini formulation. We analyze here a specific non-linear gravity-scalar system in the first order Palatini…

广义相对论与量子宇宙学 · 物理学 2010-04-06 Gianluca Allemandi , Andrzej Borowiec , Mauro Francaviglia , Sergei D. Odintsov
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