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Expansion dynamics of the Universe is one of the important subjects in modern cosmology. The dark energy equation of state determines this dynamics so that the Universe is in an accelerating phase. However, the dark matter can also affect…

广义相对论与量子宇宙学 · 物理学 2025-10-08 Zeinab Rezaei

Understanding the late-time acceleration of the Universe is one of the major challenges in cosmology today. In this paper, we present a new scalar field model corresponding to a generalised axion-like potential. In fact, this model can be…

宇宙学与河外天体物理 · 物理学 2025-07-09 Carlos G. Boiza , Mariam Bouhmadi-López

Assuming the universe is spatially homogeneous on the largest scales lays the foundation for almost all cosmology. This idea is based on the Copernican principle, that we are not at a particularly special place in the universe.…

宇宙学与河外天体物理 · 物理学 2015-06-04 Chris Clarkson

Cosmic acceleration can be achieved not only with a sufficiently flat scalar field potential but through kinetic terms coupled to gravity. These derivative couplings impose a shift symmetry on the scalar field, aiding naturalness. We write…

宇宙学与河外天体物理 · 物理学 2011-11-29 Giulia Gubitosi , Eric V. Linder

We use covariant and first-order formalism techniques to study the properties of general relativistic cosmology in three dimensions. The covariant approach provides an irreducible decomposition of the relativistic equations, which allows…

广义相对论与量子宇宙学 · 物理学 2009-11-11 John D. Barrow , Douglas J. Shaw , Christos G. Tsagas

We apply the Induced Matter Model to a five-dimensional metric. For the case with null cosmological constant, we obtain a solution able to describe the radiation-dominated era of the universe. The positive $\Lambda$ case yields a bounce…

广义相对论与量子宇宙学 · 物理学 2019-09-20 M. M. Lapola , P. H. R. S. Moraes , W. de Paula , J. F. Jesus , R. Valentim , M. Malheiro

A mechanism of inflation from higher dimensions compactification is studied. An Early Universe capable of providing exponential growth for some dimensions and exponential contraction for others, giving therefore an explanation for the big…

广义相对论与量子宇宙学 · 物理学 2018-08-29 David Benisty , Eduardo I. Guendelman

In this thesis the cosmological constant is investigated from two points of view. First, we study the influence of a time-dependent cosmological constant on the late-time expansion of the universe. Thereby, we consider several combinations…

高能物理 - 理论 · 物理学 2007-05-23 Florian Bauer

Many studies have been carried out since T.Padmanabhan proposed that the cosmic acceleration can be understood from the perspective that spacetime dynamics is an emergent phenomenon. Motivated by such a new paradigm, we firstly study the de…

广义相对论与量子宇宙学 · 物理学 2015-08-05 Zi-Liang Wang , Wen-Yuan Ai , Hua Chen , Jian-Bo Deng

The accelerating expansion of the universe presents an exciting, fundamental challenge to the standard models of particle physics and cosmology. I highlight some of the outstanding challenges in both developing theoretical models and…

天体物理学 · 物理学 2008-11-26 Eric V. Linder

A huge amount of good quality data converges towards the picture of a spatially flat universe undergoing the today observed phase of accelerated expansion. This new observational trend is commonly addressed as Precision Cosmology. Despite…

广义相对论与量子宇宙学 · 物理学 2008-12-02 S. Capozziello

Observations suggest that nearly seventy per cent of the energy density in the universe is unclustered and exerts negative pressure. Theoretical understanding of this component (`dark energy'), which is driving an accelerated expansion of…

天体物理学 · 物理学 2007-05-23 T. Padmanabhan

We explain an accelerated expansion of the present universe, suggested from observations of supernovae of type Ia at high redshift, by introducing an anti-frictional force that is self-consistently exerted on the particles of the cosmic…

天体物理学 · 物理学 2008-11-26 Winfried Zimdahl , Dominik J. Schwarz , Alexander B. Balakin , Diego Pavon

We show that cosmic acceleration can arise due to very tiny corrections to the usual gravitational action of General Relativity of the form $R^n$, with $n<0$. This eliminates the need for dark energy, though it does not address the…

天体物理学 · 物理学 2009-11-10 Sean M. Carroll , Vikram Duvvuri , Mark Trodden , Michael S. Turner

In 5D relativity, the usual 4D cosmological constant is determined by the extra dimension. If the extra dimension is spacelike, one can get a positive cosmological constant $\Lambda$ and a 4D de Sitter (dS) space. In this paper we present…

广义相对论与量子宇宙学 · 物理学 2017-06-07 Molin Liu , Yingying Shi , Zonghua Zhao , Yu Han

I briefly discuss the challenges presented by attempting to modify general relativity to obtain an explanation for the observed accelerated expansion of the universe. Foremost among these are the questions of theoretical consistency - the…

宇宙学与河外天体物理 · 物理学 2015-05-20 Mark Trodden

Accelerating cosmologies in extra dimensional spaces have been studied. These extra dimensional spaces are products of many spaces. The physical behaviors of accelerating cosmologies are investigated from Einstein's field equation in higher…

天体物理学 · 物理学 2008-10-16 Han Siong Ch'ng

As indicated by Einstein's general relativity, matter and geometry are two faces of a single nature. In our point of view, extra dimensions, as a member of the {\em geometry face}, will be treated as a part of the {\em matter face} when…

天体物理学 · 物理学 2017-08-23 Je-An Gu

In this paper we present an alternative explanation to the acceleration of the universe and the dark energy problems in terms of the Friedmann Thermodynamics. This model has the capability of making definite predictions in-line with the…

天体物理学 · 物理学 2007-05-23 Selcuk Bayin

We make the hypothesis that the velocity of light and the expansion of the universe are two aspects of one single concept connecting space and time in the expanding universe. We show that solving Friedman's equations with that…

天体物理学 · 物理学 2009-06-23 J. -M. Vigoureux , P. Vigoureux , B. Vigoureux
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