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相关论文: Cosmological evolutions of $F(R)$ nonlinear massiv…

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Inspired by the $f(R)$ non-linear massive gravity, we propose a new kind of modified gravity model, namely $f(T)$ non-linear massive gravity, by adding the dRGT mass term reformulated in the vierbein formalism, to the $f(T)$ theory. We then…

广义相对论与量子宇宙学 · 物理学 2025-03-28 You Wu , Zu-Cheng Chen , Jiaxin Wang , Hao Wei

We study cosmological evolutions of the generalized model of nonlinear massive gravity in which the graviton mass is given by a rolling scalar field and is varying along time. By performing dynamical analysis, we derive the critical points…

高能物理 - 理论 · 物理学 2015-06-12 De-Jun Wu , Yifu Cai , Yun-Song Piao

The theory of nonlinear massive gravity can be extended into the F(R) form as developed in Phys.Rev.D90, 064051 (2014). Being free of the Boulware-Deser ghost, such a construction has the additional advantage of exhibiting no linear…

宇宙学与河外天体物理 · 物理学 2014-10-08 Yi-Fu Cai , Emmanuel N. Saridakis

In this paper, we investigate and analyze the cosmological dynamics of the universe, with an effect of modified $f(R)$ gravity emerging at cosmological scale. We choose the Einstein frame as a physical frame. We consider phase portraits of…

天体物理学 · 物理学 2007-05-23 Daris Samart

In this work a new non-minimally coupled model is presented, where a generic function $f(R)$ of the scalar curvature factors the usual Einstein-Hilbert action functional, motivated by relevant results obtained from similar models. Its…

广义相对论与量子宇宙学 · 物理学 2016-11-22 R. P. L. Azevedo , J. Páramos

The paper deals with $f(R)$ gravity theory in the background of inhomogeneous FLRW--type space time model. With proper choice of the inhomogeneous metric function it is possible to have an emergent scenario for the $f(R)$--cosmology.…

广义相对论与量子宇宙学 · 物理学 2018-11-14 Dipanjana Das , Sourav Dutta , Subenoy Chakraborty

We study the evolution of linear cosmological perturbations in f(R) models of accelerated expansion in the physical frame where the gravitational dynamics are fourth order and the matter is minimally coupled. These models predict a rich and…

天体物理学 · 物理学 2008-11-26 Yong-Seon Song , Wayne Hu , Ignacy Sawicki

In this article, we examine the dynamical evolution of flat FRW cosmological model in $f(R, L_m)$ gravity theory. We consider the general form of $f(R, L_m)$ defined as $f(R, L_m) = \Lambda + \frac{\alpha}{2} R + \beta L_m^n$, where…

广义相对论与量子宇宙学 · 物理学 2025-02-14 Aman Shukla , Rakesh Raushan , Raghavendra Chaubey

The paper deals with cosmology in modified f(T) gravity theory. With some phenomenological choices for the function f(T) it is possible to have cosmological solutions describing different phases of the evolution of the Universe for the…

广义相对论与量子宇宙学 · 物理学 2020-11-03 Akash Bose , Subenoy Chakraborty

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 review the status of the theory of dRGT massive gravity, and some of its extensions, as applied to cosmology and the cosmological constant problem.

宇宙学与河外天体物理 · 物理学 2017-01-12 Kurt Hinterbichler

A number of dynamical system formulations have been proposed over the last few years to analyse cosmological solutions in $f(R)$ gravity. The aim of this article is to provide a brief introduction to the different approaches, presenting…

广义相对论与量子宇宙学 · 物理学 2022-05-06 Saikat Chakraborty , Peter K. S. Dunsby , Kelly Macdevette

We investigate the cosmological behavior of mimetic F(R) gravity. This scenario is the F(R) extension of usual mimetic gravity classes, which are based on re-parametrizations of the metric using new, but not propagating, degrees of freedom,…

广义相对论与量子宇宙学 · 物理学 2015-04-22 Genly Leon , Emmanuel N. Saridakis

The actual accelerated expansion of the universe continues being a mystery in physics. Some models had been proposed for this explanations, among them the dark energy, which however has problems of experimental character as well as…

广义相对论与量子宇宙学 · 物理学 2012-11-13 Alejandro Guarnizo

We discuss the production and evolution of cosmological gravitons showing how the cosmological background affects their dynamics. Besides, the detection of cosmological gravitons could constitute an extremely important signature to…

广义相对论与量子宇宙学 · 物理学 2017-05-03 Salvatore Capozziello , Mariafelicia De Laurentis , Shin'ichi Nojiri , Sergei D. Odintsov

In this paper we study scalar perturbations of the metric for nonlinear $f(R)$ models. We consider the Universe at the late stage of its evolution and deep inside the cell of uniformity. We investigate the astrophysical approach in the case…

宇宙学与河外天体物理 · 物理学 2014-09-04 Maxim Eingorn , Jan Novák , Alexander Zhuk

In this letter, we investigate the cosmic expansion scenario of the universe in the framework of $f(R,L_m)$ gravity theory. We consider a non-linear $f(R,L_m)$ model, specifically, $f(R,L_m)=\frac{R}{2}+L_m^n + \beta$, where $n$ and $\beta$…

广义相对论与量子宇宙学 · 物理学 2023-11-02 Lakhan V. Jaybhaye , Raja Solanki , Sanjay Mandal , P. K. Sahoo

In this paper, we study the cosmological viability conditions, the phase-space dynamics, and the cosmological evolution of f(R) gravity. In contrast to most previous works in the literature, which analyzed the background dynamics of f(R)…

宇宙学与河外天体物理 · 物理学 2015-06-16 Jun-Qi Guo , Andrei V. Frolov

We perform a detailed dynamical analysis of various cosmological scenarios in extended (varying-mass) nonlinear massive gravity. Due to the enhanced freedom in choosing the involved free functions, this cosmological paradigm allows for a…

宇宙学与河外天体物理 · 物理学 2013-06-05 Genly Leon , Joel Saavedra , Emmanuel N. Saridakis

In this paper, we derive the field equations of modified Gauss-Bonnet gravity termed as $f(R,G)$ gravity for the non-flat Friedmann-Robertson-Walker (FRW) spacetime. We utilize the dynamical system approach to study the cosmic dynamics of…

广义相对论与量子宇宙学 · 物理学 2025-01-22 Ashutosh Singh
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