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相关论文: Conspirative cosmology with variable constants

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A Five dimensional Kaluza-Klein space-time is considered in the presence of a perfect fluid source with variable G and $\Lambda$. An expanding universe is found by using a relation between the metric potential and an equation of state. The…

广义相对论与量子宇宙学 · 物理学 2011-03-07 R. K. Tiwari , Farook Rahaman , Saibal Ray

This paper deals with the cancellation mechanism, which identifies the energy density of space-time expansion in an empty universe with the zero-point energy density and avoids the scale discrepancy with the observed energy density…

综合物理 · 物理学 2018-06-12 Christian Henke

The prevailing cosmological model with the lambda-term, in which the space is flat, is studied (section 1). The corresponding age of the Universe (t0) is calculated (assuming a Hubble constant consistent with the measurements of the Hubble…

天体物理学 · 物理学 2009-09-29 Evangelos Chaliasos

We consider tensor-vector theories with varying the space-time-matter coupling constant (varying Einstein velocity) in a spatially flat FRW universe. We examine the dynamics of this model by dynamical system method assuming a \Lambda CDM…

综合物理 · 物理学 2015-06-11 Azam Izadi , Ali Shojai , Mojtaba Nouradini

It has been suggested that by increasing the speed of light during the early universe various cosmological problems of standard big bang cosmology can be overcome, without requiring an inflationary phase. However, we find that as the Planck…

广义相对论与量子宇宙学 · 物理学 2009-10-31 D. H. Coule

A linear cosmological perturbation theory of an almost homogeneous and isotropic perfect fluid Universe with dynamically evolving Newton constant $G$ and cosmological constant $\Lambda$ is presented. A gauge-invariant formalism is developed…

天体物理学 · 物理学 2014-10-13 A. Bonanno , M. Reuter

The idea that the vacuum energy density $\rho_{\Lambda}$ could be time dependent is a most reasonable one in the expanding Universe; in fact, much more reasonable than just a rigid cosmological constant for the entire cosmic history. Being…

广义相对论与量子宇宙学 · 物理学 2015-07-08 Harald Fritzsch , Joan Sola

A cosmological constant, Lambda, is the most natural candidate to explain the origin of the dark energy (DE) component in the Universe. However, due to experimental evidence that the equation of state (EOS) of the DE could be evolving with…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Joan Sola , Hrvoje Stefancic

We tackle the problem of the accelerating universe by reconsidering the most general form of the metric when the speed of light is allowed to evolve with time in a homogeneous and isotropic universe. A new varying speed of light (VSL) model…

广义相对论与量子宇宙学 · 物理学 2007-07-17 Corrado Appignani

In the standard cosmological model, the Universe consists mainly of two invisible substances: vacuum energy with constant mass-density rho_v=\Lambda/(8pi G) (where Lambda is a `cosmological constant' originally proposed by Einstein and G is…

宇宙学与河外天体物理 · 物理学 2015-06-18 Matthew G. Walker , Abraham Loeb

If the fine structure constant $\alpha =e^2/(\hbar c)$ were to change, then a number of interpretations would be possible, attributing this change either to variations in the electron charge, the dielectric constant of the vacuum, the speed…

天体物理学 · 物理学 2009-10-31 John D. Barrow , Joao Magueijo

Big Bang models of the Universe predict rapid domination by curvature, a paradox known as the flatness problem. Solutions to this problem usually leave the Universe exactly flat for every practical purpose. Explaining a nearly but not…

天体物理学 · 物理学 2009-10-31 John D. Barrow , Joao Magueijo

We study a gravitational model in which scale transformations play the key role in obtaining dynamical $G$ and $\Lambda$. We take a scale non-invariant gravitational action with a cosmological constant and a gravitational coupling constant.…

广义相对论与量子宇宙学 · 物理学 2015-05-13 F. Darabi

A new kind of evolution for cyclic models in which the Hubble parameter oscillates and keeps positive has been explored in a specific $f(R,T)$ gravity reconstruction. A singularity-free cyclic universe with negative varying cosmological…

广义相对论与量子宇宙学 · 物理学 2019-02-11 Nasr Ahmed , Sultan Z. Alamri

We derive a model of dark energy which evolves with time via the scale factor. The equation of state $\omega=(1-2\alpha)/(1+2\alpha)$ is studied as a function of a parameter $\alpha$ introduced in this model. In addition to the recent…

广义相对论与量子宇宙学 · 物理学 2017-06-20 Hemza Azri , A. Bounames

A new varying-$c$ cosmological model constructed using two additional assumptions, which was introduced in our previous work, is briefly reviewed and the dynamic equation of the model is derived distinctly from a semi-Newtonian approach.…

广义相对论与量子宇宙学 · 物理学 2010-09-28 Hossein Shojaie , Mehrdad Farhoudi

In the present work, we consider the cosmological constant model $\Lambda\propto\alpha^{-6}$, which is well motivated from three independent approaches. As is well known, the hint of varying fine structure constant $\alpha$ was found in…

广义相对论与量子宇宙学 · 物理学 2017-01-10 Hao Wei , Xiao-Bo Zou , Hong-Yu Li , Dong-Ze Xue

New corrections to General Relativity are considered in the context of modified $f(R)$ gravity, that satisfy cosmological and local gravity constraints. The proposed models behave asymptotically as $R-2\Lambda$ at large curvature and show…

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

In this article we will consider several phenomenological models for the Universe with varying $G$ and $\Lambda(t)$, where $G$ is the gravitational "constant" and $\Lambda(t)$ is a varying cosmological "constant". Two-component fluid model…

广义相对论与量子宇宙学 · 物理学 2015-09-16 M. Khurshudyan

We have considered a cosmological model of the FRW universe with variable $G$ and $\Lambda$. The solutions have been obtained for flat model with particular form of cosmological constant. The cosmological parameters have also been obtained…

广义相对论与量子宇宙学 · 物理学 2011-03-31 Mubasher Jamil , Ujjal Debnath