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相关论文: On coincidence problem and attractor solutions in …

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We propose a new dark energy model for solving the cosmological fine-tuning and coincidence problems. A default assumption is that the fine-tuning problem disappears if we do not interpret dark energy as vacuum energy. The key idea to…

宇宙学与河外天体物理 · 物理学 2020-03-27 S. X. Tián

We study the Universe at the late stage of its evolution and deep inside the cell of uniformity. At such a scale the Universe is highly inhomogeneous and filled with discretely distributed inhomogeneities in the form of galaxies and groups…

广义相对论与量子宇宙学 · 物理学 2016-08-25 Mariam Bouhmadi-López , João Morais , Alexander Zhuk

In this paper we present exact solutions to the so-called Elko spinors for three models of expanding universe, namely the de Sitter, linear and the radiation type evolution. The study was restrict to flat, homogeneous and isotropic…

高能物理 - 理论 · 物理学 2014-03-07 J. M. Hoff da Silva , S. H. Pereira

Dynamic dark energy (DDE) models are often designed to solve the cosmic coincidence (why, just now, is the dark energy density $\rho_{de}$, the same order of magnitude as the matter density $\rho_m$?) by guaranteeing $\rho_{de} \sim \rho_m$…

天体物理学 · 物理学 2008-11-26 Chas A. Egan , Charles H. Lineweaver

A new phenomenological dark energy model, originally associated to the large-scale structure formation and considered as a solution to the fine-tuning and coincidence problems related to the cosmological constant, was analyzed within the…

广义相对论与量子宇宙学 · 物理学 2026-03-05 A. Kazım Çamlıbel

Various astronomical observations point towards the evidence for dark energy. One of the most mysterious problem is the coincidence problem: why dark energy becomes dominant only recently. We present a scenario based on extended…

天体物理学 · 物理学 2009-11-06 Takeshi Chiba

We examine cyclic phantom models for the universe, in which the universe is dominated sequentially by radiation, matter, and a phantom dark energy field, followed by a standard inflationary phase. Since this cycle repeats endlessly, the…

宇宙学与河外天体物理 · 物理学 2013-05-30 Hui-Yiing Chang , Robert J. Scherrer

We study cosmological dynamics of an extended gravitational theory that gravity is coupled non-minimally with derivatives of a dark energy component and there is also a phenomenological interaction between the dark energy and dark matter.…

广义相对论与量子宇宙学 · 物理学 2016-05-20 Kourosh Nozari , Noushin Behrouz

We investigate a cosmological model in which dark energy, represented by a quintessential scalar field, is coupled to a dark-matter perfect fluid in the spatially flat Friedmann-Robertson-Walker Universe. This allows an energy exchange in…

广义相对论与量子宇宙学 · 物理学 2023-08-22 Yousef Bisabr

Recently, Geng et al. proposed to allow a non-minimal coupling between quintessence and gravity in the framework of teleparallel gravity, motivated by the similar one in the framework of General Relativity (GR). They found that this…

广义相对论与量子宇宙学 · 物理学 2012-06-04 Hao Wei

While observational cosmology has shown tremendous growth over the last decade, deep mysteries continue to haunt our theoretical understanding of the ingredients of the concordance cosmological model, which are mainly `dark'. More than 95…

宇宙学与河外天体物理 · 物理学 2013-06-10 Ram Gopal Vishwakarma

The coincidence problems and other dynamical features of dark energy are studied in cosmological models with variable cosmological parameters and in models with the composite dark energy. It is found that many of the problems usually…

天体物理学 · 物理学 2008-11-26 Javier Grande , Joan Sola , Hrvoje Stefancic

In the present article we study the process of particle creation for Elko spinor fields as a consequence of expansion of the universe. We study the effect driven by a expanding background that is asymptotically minkowskian in the past and…

高能物理 - 理论 · 物理学 2018-07-10 S. H. Pereira , R. C. Lima

A cosmological theory that predicts a late-time accelerated attractor with a constant dark matter to dark energy ratio can be said to solve the Coincidence Problem. Such cosmologies are naturally generated in the context of non-standard…

天体物理学 · 物理学 2009-11-11 James L. Crooks , Paul H. Frampton

The coincidence problem of late cosmic acceleration gets significantly alleviated when a suitable interaction between matter and dark energy, either of phantom type or not, enters the picture. We show that a class of models featuring this…

天体物理学 · 物理学 2007-05-23 German Olivares , Diego Pavon , Fernando Atrio-Barandela

We study the coincidence problem of late cosmic acceleration by assuming that the present ratio between dark matter and dark energy is a slowly varying function of the scale factor. As dark energy component we consider two different…

天体物理学 · 物理学 2009-11-13 Sergio del campo , Ramon Herrera , Diego Pavon

We consider the oscillating dark energy with periodic equation of state in two equivalent formulations: ideal fluid or scalar-tensor theory. It is shown that such dark energy suggests the natural way for the unification of early-time…

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

We analyse the trapping of eigenspinors of the charge conjugation operator with dual helicity (Elko), in thin and thick string-like models with codimension-2. Elko spinor fields describe mass dimension one fermions in four dimensions (and,…

高能物理 - 理论 · 物理学 2017-05-17 D. M. Dantas , Roldao da Rocha , C. A. S. Almeida

The coincidence problem is studied in the effective Yang-Mills condensate dark energy model. As the effective YM Lagrangian is completely determined by quantum field theory, there is no adjustable parameter in this model except the energy…

天体物理学 · 物理学 2010-11-11 Wen Zhao , Yang Zhang

We investigate the quintom model of dark energy in the generalized case where the corresponding canonical and phantom fields possess O($N$) symmetries. Assuming exponential potentials we find that this O$(N)$ quintom paradigm exhibits novel…

高能物理 - 理论 · 物理学 2008-11-26 M. R. Setare , E. N. Saridakis