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The solution to the current extending Universe problem, and the description of all stages of evolution compels scientists to consider various cosmological models. Scalar - tensor models are rather simple and also allow us to clearly define…

广义相对论与量子宇宙学 · 物理学 2015-06-23 K. E. Osetrin , A. N. Makarenko , Yu. A. Rybalov

A new model of nonlinear electrodynamics with a dimensional parameter $\beta$ coupled to gravity is considered. We show that an accelerated expansion of the universe takes place if the nonlinear electromagnetic field is the source of the…

广义相对论与量子宇宙学 · 物理学 2016-01-26 S. I. Kruglov

A model of an emergent universe is obtained in brane world. Here the bulk energy is in the form of cosmological constant, while the brane consists of the Chaplygin gas with the modified equation of state such as $p=A\rho-B/\rho$. Initially…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Asit Banerjee , Tanwi Bandyopadhyay , Subenoy Chakraborty

We present an emergent universe scenario making use of a new solution of the Starobinsky model. The solution belongs to a one parameter family of solutions, where the parameter is determined by the number and the species (spin-values) of…

广义相对论与量子宇宙学 · 物理学 2007-05-23 S. Mukherjee , B. C. Paul , S. D. Maharaj , A. Beesham

The energy-momentum tensor coming from one-parameter effective Yang- Mills theory is here used to describe the matter-energy content of the homogeneous and isotropic Friedmann cosmology in its early stages. The behavior of all solutions is…

广义相对论与量子宇宙学 · 物理学 2010-02-25 Vitorio A. De Lorenci

We introduce a class of $2d$ sigma models which are parameterized by a function of one variable. In addition to the physical field $g$, these models include an auxiliary field $v_\alpha$ which mediates interactions in a prescribed way. We…

高能物理 - 理论 · 物理学 2025-01-22 Christian Ferko , Liam Smith

In order to draw out the essential behavior of the universe, investigations of early universe cosmology often reduce the complex system to a simple integrable system. Inflationary models are of this kind as they focus on simple scalar field…

天体物理学 · 物理学 2009-10-28 Neil J. Cornish , Janna J. Levin

We consider a non singular origin for the Universe starting from an Einstein static Universe, the so called "emergent universe" scenario, in the framework of a theory which uses two volume elements $\sqrt{-{g}}d^{4}x$ and $\Phi d^{4}x$,…

广义相对论与量子宇宙学 · 物理学 2015-05-27 E. I. Guendelman

Different characteristic of matter influencing the evolution of the Universe has been simulated by means of a nonlinear spinor field. Using the nonlinear spinor field corresponding to different types of perfect fluid or dark energy as a…

广义相对论与量子宇宙学 · 物理学 2015-05-01 Bijan Saha

In the present work, the flat FLRW Universe has been modelled with cosmic matter in the form of diffusive barotropic fluid. The diffusive fluid undergoes dissipation due to diffusion mechanism in the form of cosmological scalar field. From…

广义相对论与量子宇宙学 · 物理学 2023-02-22 Subhayan Maity , Subenoy Chakraborty

This is a short overview of the ekpyrotic/cyclic model of the universe, an alternative to the standard big bang inflationary paradigm.

天体物理学 · 物理学 2007-05-23 Justin Khoury

An oscillating universe model is discussed, in which the singularity of the initial state of the universe is avoided by postulating an upper limit on spacetime curvature. This also results in the devising of the simplest possible structure…

综合物理 · 物理学 2008-12-02 V. N. Yershov

A model of an emergent universe is obtained in brane world. Here the bulk energy is in the form of cosmological constant, while the brane consists of a fluid satisfying an equation of state of the form $p_{b}={1/3} \rho_{b}$, which is…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Asit Banerjee , Tanwi Bandyopadhyay , Subenoy Chakraborty

A nonsingular emergent universe cosmology can be realized by a nonconventional spinor field as first developed in \cite{Cai:2012yf}. We study the mechanisms of generating scale-invariant primordial power spectrum of curvature perturbation…

高能物理 - 理论 · 物理学 2014-03-11 Yi-Fu Cai , Youping Wan , Xinmin Zhang

A model of nonlinear electrodynamics with a dimensional parameter $\beta$ is considered. Electromagnetic fields are the source of the gravitation field and inflation of the universe. We imply that the universe is filled by stochastic…

广义相对论与量子宇宙学 · 物理学 2017-05-08 S. I. Kruglov

A new model of nonlinear electromagnetic fields possessing a dimensional parameter $\beta$ is proposed. Electromagnetic fields are considered as the source of the gravitation field and accelerated expansion of the universe is driven by…

广义相对论与量子宇宙学 · 物理学 2016-03-25 S. I. Kruglov

In this work, Emergent Universe scenario has been developed in general homogeneous anisotropic model and for the inhomogeneus LTB model. In the first case, it is assumed that the matter in the universe has two components - one is perfect…

广义相对论与量子宇宙学 · 物理学 2011-11-10 Sudeshna Mukerji , Nairwita Mazumder , Ritabrata Biswas , Subenoy Chakraborty

In this work it is investigated the evolution of a Universe where a scalar field, non-minimally coupled to space-time curvature, plays the role of quintessence and drives the Universe to a present accelerated expansion. A non-relativistic…

广义相对论与量子宇宙学 · 物理学 2009-11-11 J. B. Binder , G. M. Kremer

Although the current galaxy models yield calculations consistent with much of the data, many irregularities exist, exceptions have been found to the current models, the $\Lambda$CDM model apparently fails on galaxy scales, dark matter…

天体物理学 · 物理学 2007-05-23 John C. Hodge

In this paper, we consider a nonminimal coupling model between gravity and nonlinear electrodynamics with cosmological constant. This cosmological model is designed to account for both the inflationary epoch of the early universe and the…

广义相对论与量子宇宙学 · 物理学 2024-10-10 Chilwatun Nasiroh , Ramy F. Izzah , Fiki T. Akbar , Bobby E. Gunara