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相关论文: Evolution of an effective Hubble constant in $f(R)…

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We analyse the $f(R)$ gravity in the so-called Jordan frame, as implemented to the isotropic Universe dynamics. The goal of the present study is to show that, according to recent data analyses of the supernovae Ia Pantheon sample, it is…

广义相对论与量子宇宙学 · 物理学 2023-04-12 Tiziano Schiavone , Giovanni Montani , Flavio Bombacigno

In this work, two models of metric $f(R)$ gravity in the Jordan frame are investigated as a dynamical description of the late-time cosmic expansion using binned Type Ia Supernovae data. The aim is to provide an explanation for the effective…

广义相对论与量子宇宙学 · 物理学 2026-04-15 A. Valletta , G. Montani , M. G. Dainotti , E. Fazzari

We consider a dynamic scenario for characterizing the late Universe evolution, aiming to mitigate the Hubble tension. Specifically, we consider a metric $f(R)$ gravity in the Jordan frame which is implemented to the dynamics of a flat…

广义相对论与量子宇宙学 · 物理学 2024-08-06 Giovanni Montani , Nakia Carlevaro , Mariaveronica De Angelis

We introduce a theoretical framework to interpret the Hubble tension, based on the combination of a metric $f(R)$ gravity with a dynamical dark energy contribution. The modified gravity provides the non-minimally coupled scalar field…

广义相对论与量子宇宙学 · 物理学 2023-11-07 Giovanni Montani , Mariaveronica De Angelis , Flavio Bombacigno , Nakia Carlevaro

We examine a modified late-Universe dynamics where dark energy decays into dark matter, within the framework of metric $f(R)$-gravity in the Jordan frame. After a detailed analysis of the modified $\Lambda \text{CDM}$ model, we introduce a…

宇宙学与河外天体物理 · 物理学 2025-06-19 Giovanni Montani , Mariaveronica De Angelis , Maria Giovanna Dainotti

The Hubble constant tension problem is analysed in the framework of a class of modified gravity, the so-called $F(R)$ gravity. To do so, we explore two models: an exponential and a power-law $F(R)$ gravities, which includes an early dark…

广义相对论与量子宇宙学 · 物理学 2021-03-24 Sergei D. Odintsov , Diego Sáez-Chillón Gómez , German S. Sharov

The reconstruction of f(R)-gravity is showed by using an auxiliary scalar field in the context of cosmological evolution, this development provide a way of reconstruct the form of the function f (R) for a given evolution of the Hubble…

高能物理 - 理论 · 物理学 2009-07-22 Diego Sáez-Gómez

In this work, we obtain measurements of the Hubble constant in the context of modified gravity theories. We set up our theoretical framework by considering viable cosmological $f(R)$ and $f(T)$ models, and we analyzed them through the use…

宇宙学与河外天体物理 · 物理学 2020-05-07 Rocco D'Agostino , Rafael C. Nunes

$f(R)$ gravity models belong to an important class of modified gravity models where the late time cosmic accelerated expansion is considered as the manifestation of the large scale modification of the force of gravity. $f(R)$ gravity models…

广义相对论与量子宇宙学 · 物理学 2013-08-27 Umananda Dev Goswami , Kabita Deka

In this work, we consider four $f(R)$ gravity models -- the Hu-Sawicki, Starobinsky, Exponential and Tsujikawa models -- and use a range of cosmological data, together with Markov Chain Monte Carlo sampling techniques, to constrain the…

宇宙学与河外天体物理 · 物理学 2022-01-05 Christine R. Farrugia , Joseph Sultana , Jurgen Mifsud

We study the evolution of linear perturbations in metric f(R) models of gravity and identify a potentially observable characteristic scale-dependent pattern in the behavior of cosmological structures. While at the background level viable…

天体物理学 · 物理学 2014-11-18 Levon Pogosian , Alessandra Silvestri

A novel function for modified gravity is proposed, $f(R, T)=R+\lambda R^2+2\beta\ln(T)$, with constants $\lambda$ and $\beta$, scalar curvature $R$, and the trace of stress energy tensor $T$, satisfying $T=\rho-3p>0$. Subsequently, two…

综合物理 · 物理学 2020-06-16 Emilio Elizalde , Nisha Godani , Gauranga C. Samanta

Extremely large surveys with future experiments like Euclid and the SKA will soon allow us to access perturbation modes close to the Hubble scale, with wavenumbers $k \sim \mathcal{H}$. If a modified gravity theory is responsible for cosmic…

宇宙学与河外天体物理 · 物理学 2015-11-03 Tessa Baker , Philip Bull

The mismatch between different independent measurements of the expansion rate of the Universe is known as the Hubble constant ($H_0$) tension, and it is a serious and pressing problem in cosmology. We investigate this tension considering…

宇宙学与河外天体物理 · 物理学 2022-05-17 Tiziano Schiavone , Giovanni Montani , Maria Giovanna Dainotti , Biagio De Simone , Enrico Rinaldi , Gaetano Lambiase

In recent years, modifications to General Relativity (GR) have been explored to address cosmological observations, particularly in the context of late-time cosmic acceleration. Among these, modifications based on the Teleparallel Equivalent…

宇宙学与河外天体物理 · 物理学 2025-08-29 Saurabh Verma , Archana Dixit , Anirudh Pradhan , M. S. Barak

We focus on weak inhomogeneous models of the Universe at low redshifts, described by the Lema\^itre-Tolman-Bondi (LTB) metric. The principal aim of this work is to compare the evolution of inhomogeneous perturbations in the $\Lambda$CDM…

宇宙学与河外天体物理 · 物理学 2023-04-20 Tiziano Schiavone , Giovanni Montani

We solve the field equations of modified gravity for $f(R)$ model in metric formalism. Further, we obtain the fixed points of the dynamical system in phase space analysis of $f(R)$ models, both with and without the effects of radiation.…

广义相对论与量子宇宙学 · 物理学 2018-01-26 Murli Manohar Verma , Bal Krishna Yadav

This paper investigates the cosmological implications of the modified gravity framework known as $f(R,\Sigma, T)$ gravity, focusing on its potential to unify and extend current cosmological models. The theory, introduced by Bakry and…

广义相对论与量子宇宙学 · 物理学 2025-03-04 N. Myrzakulov , S. H. Shekh , Anirudh Pradhan

We analyze the Taylor expansion of metric $f(R)$ gravity in the Jordan frame around the General Relativity limit. By relating the scalar--tensor representation to the original $f(R)$ formulation, we derive constraints on the expansion…

广义相对论与量子宇宙学 · 物理学 2026-04-28 Giovanni Montani , Andrea Valletta

A modified theory of gravity with the function $F(R) = R\exp(\alpha R)$ instead of Ricci scalar $R$ in the Einstein$-$Hilbert action is considered and analyzed. The action of the model is converted into Einstein$-$Hilbert action at small…

广义相对论与量子宇宙学 · 物理学 2013-09-30 S. I. Kruglov
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