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相关论文: Screening $\Lambda$ in a new modified gravity mode…

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A good definition for the energy momentum tensor of gravity (EMTG) in General Relativity (GR) is a hard, if not impossible, task. On the other hand, in its teleparallel version, known as The Teleparallel Equivalent of General Relativity…

广义相对论与量子宇宙学 · 物理学 2018-12-18 J. B. Formiga

In this work, we analyze the Einstein-scalar-Gauss-Bonnet (EsGB) theory of gravity in a cosmological context using the formalism of dynamical systems. We obtain the equations of motion of the theory and introduce an appropriate set of…

广义相对论与量子宇宙学 · 物理学 2025-09-23 Miguel A. S. Pinto , João Luís Rosa

We demonstrate a new method to constrain gravity on the largest cosmological scales by combining measurements of cosmic microwave background (CMB) lensing and the galaxy velocity field. $E_G$ is a statistic, constructed from a gravitational…

宇宙学与河外天体物理 · 物理学 2016-08-09 Anthony R. Pullen , Shadab Alam , Siyu He , Shirley Ho

This paper investigates the flat Friedmann-Lema$\hat{\imath}$tre-Robertson-Walker (FLRW) cosmological model using a suitable parameterization represented as a differential equation concerning the energy density of the scalar field,…

广义相对论与量子宇宙学 · 物理学 2024-04-30 J. K. Singh , Shaily , Harshna Balhara , Sushant G. Ghosh , Sunil D. Maharaj

A type of exponential correction to General Relativity gives viable modified gravity model of dark energy. The model behaves as $R-2\Lambda$ at large curvature where an effective cosmological constant appears, but it becomes zero in flat…

广义相对论与量子宇宙学 · 物理学 2022-01-13 L. N. Granda

In ``On restricting to one-loop order the radiative effects in quantum gravity" (Brandt, Frenkel, and McKeon, 2020) \cite{Brandt2020}, a Lagrange multiplier (LM) field is introduced into the Einstein-Hilbert action, removing all multi-loop…

高能物理 - 理论 · 物理学 2025-09-09 Farrukh A. Chishtie

In this work, we extend the standard cosmological model within the quadratic energy-momentum squared gravity (qEMSG) framework, introducing a nonminimal interaction between the usual material field ($T_{\mu\nu}$) and its accompanying…

宇宙学与河外天体物理 · 物理学 2026-03-26 Ozgur Akarsu , Mariam Bouhmadi-López , Nihan Katirci , N. Merve Uzun

Over the last decades, tests on the standard model of cosmology, the so-called $\Lambda$CDM model, have been widely analysed and compared with many different models for describing dark energy. Modified gravities have played an important…

广义相对论与量子宇宙学 · 物理学 2024-12-13 Sergei D. Odintsov , Diego Sáez-Chillón Gómez , German S. Sharov

Cosmography can be considered as a sort of a model-independent approach to tackle the dark energy/modified gravity problem. In this review, the success and the shortcomings of the $\Lambda$CDM model, based on General Relativity and standard…

广义相对论与量子宇宙学 · 物理学 2019-04-09 Salvatore Capozziello , Rocco D'Agostino , Orlando Luongo

In this study, we examine the energy-momentum squared modified theory of gravity, where the squared term $T_{\mu\nu}T^{\mu\nu}$ is incorporated into the conventional gravitational Lagrangian. This modification aims to account for dark…

广义相对论与量子宇宙学 · 物理学 2025-02-03 H. R. Fazlollahi , H. Velten , H. Shojaie

In this paper, we introduce the post-Minkowskian approximation of Energy-Momentum-Squared Gravity (EMSG). This approximation is used to study the gravitational energy flux in the context of EMSG. As an application of our results, we…

广义相对论与量子宇宙学 · 物理学 2022-02-14 Elham Nazari , Mahmood Roshan , Ivan De Martino

We investigate the post-Newtonian (PN) dynamics of energy-momentum squared gravity (EMSG), with particular emphasis on the possibility of self-acceleration in $N$-body systems. A central challenge in matter-type modified gravity theories,…

广义相对论与量子宇宙学 · 物理学 2026-05-12 Elham Nazari

We study the generalized version of energy-momentum squared gravity (EMSG) in the Palatini formalism. This theory allows the existence of a scalar constructed with energy-momentum tensor as $T_{\alpha\beta}T^{\alpha\beta}$ in the generic…

广义相对论与量子宇宙学 · 物理学 2020-09-28 Elham Nazari , Farahnaz Sarvi , Mahmood Roshan

We present updated observational constraints on the spatially flat $\phi$CDM model, where dark energy is described by a minimally coupled scalar field $\phi$ with an inverse power-law potential $V=V_0 \phi^{-\alpha}$. Using Planck 2018 CMB…

宇宙学与河外天体物理 · 物理学 2025-10-01 Chan-Gyung Park , Bharat Ratra

Cosmological tensions can arise within $\Lambda$CDM scenario amongst different observational windows, which may indicate new physics beyond the standard paradigm if confirmed by measurements. In this article, we report how to alleviate both…

宇宙学与河外天体物理 · 物理学 2020-08-06 Sheng-Feng Yan , Pierre Zhang , Jie-Wen Chen , Xin-Zhe Zhang , Yi-Fu Cai , Emmanuel N. Saridakis

We reconstruct the $\Lambda$CDM model for $f(T,\mathcal{T})$ Theory, where $T$ is the torsion scalar and $\mathcal{T}$ the trace of the energy-momentum tensor. The result shows that the action of $\Lambda$CDM is a combination of a linear…

广义相对论与量子宇宙学 · 物理学 2016-05-19 Ednaldo L. B. Junior , Manuel E. Rodrigues , Ines G. Salako , Mahouton J. S. Houndjo

Einstein-Gauss-Bonnet (EGB) model is recently restudied in order to analyze new consequences in gravitation, modifying appropriately the Einstein-Hilbert action. The consequences in EGB cosmology are mainly geometric, with higher order…

宇宙学与河外天体物理 · 物理学 2021-03-02 Miguel A. García-Aspeitia , A. Hernández-Almada

The exponential $f(R)$ gravity model provides a theoretically well-motivated extension of General Relativity, introducing a modified gravitational dynamics at late times consistent with a dynamical dark energy scenario, while recovering the…

广义相对论与量子宇宙学 · 物理学 2025-11-11 Simone D'Onofrio , Sergei Odintsov , Tiziano Schiavone

The screened modified gravity (SMG) is a unified theoretical framework, which describes the scalar-tensor gravity with screening mechanism. Based on the gravitational-wave (GW) waveform derived in our previous work \citep{liu2018waveforms},…

广义相对论与量子宇宙学 · 物理学 2020-02-28 Rui Niu , Xing Zhang , Tan Liu , Jiming Yu , Bo Wang , Wen Zhao

This paper explores models of the FLRW universe that incorporate a time-varying cosmological term $\Lambda(t)$. Specifically, we assume a power-law form for the cosmological term as a function of the scale factor: $\Lambda(t)=\Lambda_{0}…

宇宙学与河外天体物理 · 物理学 2024-05-14 M. Koussour , N. Myrzakulov , J. Rayimbaev