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Geometrical structure of homogeneous isotropic models in the frame of the metric-affine gauge theory of gravity (MAGT) is analyzed. By using general form of gravitational Lagrangian including both a scalar curvature and various invariants…

广义相对论与量子宇宙学 · 物理学 2007-05-23 A. V. Minkevich , A. S. Garkun

The inhomogeneous distribution of matter in the non-linear regime of galaxies, clusters of galaxies and voids is described by an exact, spherically symmetric inhomogeneous solution of Einstein's gravitational field equations, corresponding…

天体物理学 · 物理学 2009-11-11 J. W. Moffat

The standard procedure to explain the accelerated expansion of the Universe is to assume the existence of an exotic component with negative pressure, generically called dark energy. Here, we propose a new accelerating flat cosmology without…

宇宙学与河外天体物理 · 物理学 2025-02-21 P. W. R. Lima , J. A. S. Lima , J. F. Jesus

Different models of the cosmic substratum which pretend to describe the present stage of accelerated expansion of the Universe like the $\Lambda$CDM model or a Chaplygin gas, can be seen as special realizations of a holographic dark energy…

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

We investigate the evolution of cosmological perturbations in models of dark energy described by a time-like unit normalized vector field specified by a general function $\mathcal{F}(\mathcal{K})$, so-called Generalized Einstein-Aether…

宇宙学与河外天体物理 · 物理学 2017-10-04 Richard A. Battye , Francesco Pace , Damien Trinh

Phenomena currently attributed to Dark Matter (DM) and Dark Energy (DE) are merely a result of the interplay between gravitational energy density, caused by the contraction of space by matter, and space dilation, caused by the energy…

天体物理学 · 物理学 2008-10-23 Shlomo Barak , Elia M. Leibowitz

The theory of cosmological perturbations is extended to spacetimes displaying isotropic expansion but anisotropic curvature. The perturbed Einstein equation and Boltzmann equations for massless and massive particles are derived in a general…

广义相对论与量子宇宙学 · 物理学 2014-05-08 T. G. Zlosnik

In order to explain the late-time cosmological acceleration, we propose a new pure geometric gravity based on Deser-Woodard theory, in which the expansion of a matter-dominated universe can be accelerating. This new theory behaves as well…

广义相对论与量子宇宙学 · 物理学 2018-10-31 Shuxun Tian

Motivated by the quantum description of gauge theories, we study the cosmological effects of relaxing the Hamiltonian and momentum constraints in general relativity and Gauss' law in electromagnetism. We show that the unconstrained theories…

高能物理 - 唯象学 · 物理学 2024-05-13 Loris Del Grosso , David E Kaplan , Tom Melia , Vivian Poulin , Surjeet Rajendran , Tristan L Smith

We review some modified gravity models which describe the gravitational dark energy and the possibility of cosmic speed-up. The new consistent version of such theory which contains inverse and HD curvature terms as well as new type of…

高能物理 - 理论 · 物理学 2009-09-17 Shin'ichi Nojiri , Sergei D. Odintsov

We consider scalar field models of dark energy interacting with dark matter through a coupling proportional to the contraction of the four-derivative of the scalar field with the four-velocity of the dark matter fluid. The coupling is…

广义相对论与量子宇宙学 · 物理学 2018-02-07 Jibitesh Dutta , Wompherdeiki Khyllep , Nicola Tamanini

General equations of the unified field theory, obtained using the curved and torsional space-time, are presented. They contain only independent geometrical parameters (metric and connections) of the metric-affine space, and describe the…

综合物理 · 物理学 2026-01-22 Alex Karpelson

Dark energy is a fundamental constituent of our universe, its status in the cosmological field equation should be equivalent to that of gravity. Here we construct a dark energy and matter gravity coupling (DEMC) model of cosmology in a way…

综合物理 · 物理学 2015-01-14 Ti-Pei Li

We propose a cosmological model in the framework of the Poincar\'e gauge theory of gravity (PG). The gravitational Lagrangian is quadratic in curvature and torsion. In our specific model, the Lagrangian contains (i) the curvature scalar $R$…

广义相对论与量子宇宙学 · 物理学 2011-02-25 Peter Baekler , Friedrich W. Hehl , James M. Nester

Gauge bosons associated to new gauge symmetries under which the standard model particles are not charged are predicted in many extensions of the standard model of particles and interactions. We show that under very general conditions, the…

高能物理 - 唯象学 · 物理学 2013-10-01 J. A. R. Cembranos , A. L. Maroto , S. J. Nunez Jareno

We consider a novel model of gravity with a scalar field described by the Lagrangian with higher order derivative terms in a cosmological context. The model has the same solution for the homogeneous and isotropic universe as in the model…

广义相对论与量子宇宙学 · 物理学 2019-07-04 Nahomi Kan , Kiyoshi Shiraishi

A new realization of the matter Lagrangian is introduced which models the dark energy component as a non-standard combination of thermodynamics quantities of the baryonic matter. We will prove that the present realization is independent of…

广义相对论与量子宇宙学 · 物理学 2026-01-28 Shahab Shahidi , Sedigheh Farahzad

In a recent article, Kleidis and Spyrou (2015) proposed that both dark matter (DM) and dark energy (DE) can be treated as a single component, if accommodated in the context of a polytropic DM fluid with thermodynamical content. Depending…

宇宙学与河外天体物理 · 物理学 2017-10-25 Kostas Kleidis , Nikolaos K. Spyrou

We study a uniform and isotropic cosmology with a decaying vacuum energy density, in the realm of a model with a time varying gravitational "constant". We show that, for late times, such a cosmology is in accordance with the observed values…

广义相对论与量子宇宙学 · 物理学 2016-11-09 Saulo Carneiro

The concept of the scalar graviton as the source of the dark matter and dark energy of the gravitaional origin is applied to study the evolution of the isotropic homogeneous Universe. A realistic self-consistent solution to the modified…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Yu. F. Pirogov