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相关论文: Growth of matter density perturbations in 4D Einst…

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An alternative theory of gravity that has attracted much attention recently is the novel four-dimensional Einstein-Gauss-Bonnet (4D EGB) gravity. The theory is rescaled by the Gauss-Bonnet (GB) coupling constant $\alpha \rightarrow…

广义相对论与量子宇宙学 · 物理学 2022-03-25 Khadije Jafarzade , Mahdi Kord Zangeneh , Francisco S. N. Lobo

The cosmology of general fourth order corrections to Einstein gravity is considered, both for a homogeneous and isotropic background and for general tensor perturbations. It is explicitly shown how the standard cosmological history can be…

广义相对论与量子宇宙学 · 物理学 2011-03-07 William Nelson

We investigate $f\left( Q\right) $-gravity with a matter-gravity coupling as a geometric dark energy candidate for the description of the late-time cosmic acceleration within a spatially flat Friedmann--Lema\^{\i}tre-Robertson-Walker…

广义相对论与量子宇宙学 · 物理学 2026-03-24 Andronikos Paliathanasis

The striking GW170817 event indicated that the graviton is nearly massless, since the gamma rays emitted from the two neutron stars merging arrived almost simultaneously with the gravitational waves. Thus, the graviton must also be massless…

广义相对论与量子宇宙学 · 物理学 2020-12-02 V. K. Oikonomou , F. P. Fronimos

Regge-Teitelboim embedding gravity is the modified gravity based on a simple string-inspired geometrical principle: our spacetime is considered here as a 4-dimensional surface in a flat bulk. This theory is similar to the recently popular…

广义相对论与量子宇宙学 · 物理学 2020-10-13 S. A. Paston

Theoretical arguments and cosmological observations suggest that Einstein's theory of general relativity needs to be modified at high energies. One of the best motivated higher-curvature extensions of general relativity is…

广义相对论与量子宇宙学 · 物理学 2017-08-04 Laura Sberna

In this paper, we study the $F(R, G)$ gravity model with an interacting model by flat-FRW metric in a viscous fluid. We consider that the universe dominates with components of dark matter and dark energy. This means that the dark matter…

广义相对论与量子宇宙学 · 物理学 2023-03-22 E. Mahichi , Alireza Amani , M. A. Ramzanpour

This thesis focuses on late-time cosmic acceleration within modified theories of gravity, using various observational data sets and statistical analysis. The Universe is assumed to be spatially homogeneous and isotropic and is described by…

广义相对论与量子宇宙学 · 物理学 2025-03-05 Santosh V. Lohakare

We investigate the cosmological perturbations in the context of a Scalar-Tensor-Vector theory of Gravity known as MOG in the literature. Recent investigations show that MOG reproduces a viable background cosmological evolution comparable to…

广义相对论与量子宇宙学 · 物理学 2020-02-18 Sara Jamali , Mahmood Roshan , Luca Amendola

Prompted by the recent more precise determination of the basic cosmological parameters and growing evidence that the matter-energy content of the universe is now dominated by dark energy and dark matter we present the general solution of…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Marek Demianski , Zdzislaw A. Golda , Andrzej Woszczyna

The standard $\Lambda$-CDM predicts a growth of structures which tends to be higher than the values of redshift space distortion (RSD) measurements, if the cosmological parameters are fixed by the CMB data. In this paper we point out that…

宇宙学与河外天体物理 · 物理学 2017-03-08 Antonio De Felice , Shinji Mukohyama

In the 2030s, space-based gravitational-wave (GW) detectors will exhibit unprecedented sensitivity in the millihertz frequency band, greatly expanding the potential for testing theories of gravity compared to ground-based GW detectors.…

广义相对论与量子宇宙学 · 物理学 2024-04-16 Weilong Luo , Chang Liu , Zong-Kuan Guo

In this paper we performed investigation of the spatially-flat cosmological models whose spatial section is product of three- ("our Universe") and extra-dimensional parts. The matter source chosen to be the perfect fluid which exists in the…

广义相对论与量子宇宙学 · 物理学 2019-02-11 Sergey A. Pavluchenko

We study some aspects of dynamical compactification scenario where stabilisation of extra dimensions occurs due to presence the Gauss-Bonnet term and non-zero spatial curvature. In the framework of the model under consideration there exists…

广义相对论与量子宇宙学 · 物理学 2021-05-12 Dmitry Chirkov , Sergey A. Pavluchenko

We study dynamical dark energy models within Einstein's theory by means of matter perturbations and the growth index $\gamma$. Within four-dimensional General Relativity, we assume that dark energy does not cluster, and we adopt a linear…

广义相对论与量子宇宙学 · 物理学 2023-06-07 G. Panotopoulos , G. Barnert , L. E. Campusano

We consider a particular example of dynamical compactification of an anisotropic 7+1 dimensional Universe in Einstein - Gauss - Bonnet gravity. Starting from rather general totally anisotropic initial conditions a Universe in question…

广义相对论与量子宇宙学 · 物理学 2020-04-02 Dmitry Chirkov , Alex Giacomini , Alexey Toporensky

Nonlinear gravitational instability is a crucial way to comprehend the clustering of matter and the formation of nonlinear structures in both the Universe and stellar systems. However, with the exception of a few exact particular solutions…

广义相对论与量子宇宙学 · 物理学 2023-07-10 Chao Liu

We studied the cosmological constraints on the Galileon gravity obtained from observational data of the growth rate of matter density perturbations, the supernovae Ia (SN Ia), the cosmic microwave background (CMB), and baryon acoustic…

宇宙学与河外天体物理 · 物理学 2012-07-03 Koichi Hirano , Zen Komiya , Hisato Shirai

Virtual transitions in a Casimir-like configuration are utilized to probe quantum aspects of four-dimensional Einstein-Gauss-Bonnet (4D EGB) gravity. This study employs a quantum optics-based approach, wherein an Unruh-DeWitt detector…

广义相对论与量子宇宙学 · 物理学 2025-06-04 Syed Masood

Modified gravity (MG) theories predict, in general, that the ratio of gravitational wave (GW) to electromagnetic (EM) luminosity distances, $\Xi$, differs from its general relativity (GR) value of unity at cosmological scales, thus…

广义相对论与量子宇宙学 · 物理学 2021-05-28 Isabela S. Matos , Maurício O. Calvão , Ioav Waga