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相关论文: Is Cosmic Acceleration Really Recent?

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Possibly the most peculiar expectation of the standard fine-tuned cosmological paradigm is that cosmic acceleration is to only be a very recent (z<1) phenomenon, with the universe being required to be decelerating at all higher redshifts.…

天体物理学 · 物理学 2016-08-30 Philip D. Mannheim

One of the strongest arguments against the cosmological constant as an explanation of the current epoch of accelerated cosmic expansion is the existence of an earlier, dynamical acceleration, i.e. inflation. We examine the likelihood that…

宇宙学与河外天体物理 · 物理学 2014-11-21 Eric V. Linder

The discovery that the cosmic expansion is accelerating has been followed by an intense theoretical and experimental response in physics and astronomy. The discovery implies that our most basic notions about how gravity work are violated on…

宇宙学与河外天体物理 · 物理学 2010-01-15 Robert R. Caldwell , Marc Kamionkowski

A possible slowing down of the cosmic expansion is investigated through a cosmographic approach. By expanding the luminosity distance to fourth order and fitting the SN Ia data from the most recent compilations (Union, Constitution and…

宇宙学与河外天体物理 · 物理学 2015-03-17 Antonio C. C. Guimarães , José Ademir S. Lima

The discovery that the Universe is accelerating in its expansion has brought the basic concept of cosmic expansion into question. An analysis of the evolution of this concept suggests that the paradigm that was finally settled into prior to…

物理学史与哲学 · 物理学 2014-09-12 Daryl Janzen

A general-relativistic theory of cosmology, the dynamical variables of which are those of Hubble's, namely distances and redshifts, is presented. The theory describes the universe as having a three-phase evolution with a decelerating…

天体物理学 · 物理学 2007-05-23 S. Behar , M. Carmeli

The standard big bang cosmology has been greatly successful in explaining many observational aspects of the real universe. However, two particular diffficulties faced by it are the so-called ``horizon'' and ``flatness'' problems. By…

综合物理 · 物理学 2007-05-23 Abhas Mitra

The "standard" model of cosmology is founded on the basis that the expansion rate of the universe is accelerating at present --- as was inferred originally from the Hubble diagram of Type Ia supernovae. There exists now a much bigger…

宇宙学与河外天体物理 · 物理学 2016-10-24 Jeppe Trøst Nielsen , Alberto Guffanti , Subir Sarkar

We investigate a fourth order model of gravity, having a free length parameter, and no cosmological constant or dark energy. We consider cosmological evolution of a flat Friedmann universe in this model for the case that the length…

广义相对论与量子宇宙学 · 物理学 2015-10-14 Shreya Banerjee , Nilesh Jayswal , Tejinder P. Singh

We investigate the prospects for determining the accelerating history of the Universe from upcoming measurements of the expansion rate $H(z)$. In our analyses, we use Monte Carlo simulations based on $w$CDM models to generate samples with…

宇宙学与河外天体物理 · 物理学 2012-04-22 J. C. Carvalho , J. S. Alcaniz

Recent observations of distant supernovae imply, in defiance of expectations, that the universe growth is accelerating, contrary to what has always been assumed that the expansion is slowing down due to gravity. In this paper a…

天体物理学 · 物理学 2007-05-23 M. Carmeli , S. Behar

We investigate the properties of a cosmological scenario which undergoes a gravitational phase transition at late times. In this scenario, the Universe evolves according to general relativity in the standard, hot Big Bang picture until a…

天体物理学 · 物理学 2013-05-29 Robert R. Caldwell , William Komp , Leonard Parker , Daniel A. T. Vanzella

We have considered a cosmological model with a phenomenological model for the cosmological constant of the form $\Lambda=\bt\fr{\ddot R}{R}$, $ \bt$ is a constant. For age parameter consistent with observational data the Universe must be…

广义相对论与量子宇宙学 · 物理学 2017-08-23 Arbab I. Arbab

The possibility of having an extension of the cosmological standard model with a Hubble expansion rate $H$ constrained to a finite interval is considered. Two periods of accelerated expansion arise naturally when the Hubble expansion rate…

天体物理学 · 物理学 2010-04-14 J. L. Cortes , J. Indurain

The present standard model of cosmology, $\Lambda$CDM, contains some intriguing coincidences. Not only are the dominant contributions to the energy density approximately of the same order at the present epoch, but we note that contrary to…

宇宙学与河外天体物理 · 物理学 2015-05-18 Pim van Oirschot , Juliana Kwan , Geraint F. Lewis

The most exciting future observation in cosmology will feature a monitoring of the cosmic expansion in real time, unlike anything that has ever been attempted before. This campaign will uncover crucial physical properties of the various…

广义相对论与量子宇宙学 · 物理学 2022-12-14 Fulvio Melia

Theoretical approaches to explaining the observed acceleration of the universe are reviewed. We briefly discuss the evidence for cosmic acceleration, and the implications for standard General Relativity coupled to conventional sources of…

宇宙学与河外天体物理 · 物理学 2009-09-28 Alessandra Silvestri , Mark Trodden

There is now overwhelming observational evidence that our Universe is accelerating in its expansion. I discuss how modified gravitational models can provide an explanation for this observed late-time cosmic acceleration. We consider…

天体物理学 · 物理学 2008-11-26 Damien A. Easson

The cosmic acceleration is one of the most significant cosmological discoveries over the last century. The two categories of explanation are exotic component (dark energy) and modified gravity. We constrain the two types of model by a joint…

天体物理学 · 物理学 2008-07-20 Hongsheng Zhang , Heng Yu , Hyerim Noh , Zong-Hong Zhu

Constancy of the speed of light together with the Hubble law lead in a doctrine of expanding universe to a conclusion that universe evolution is not only an expansion of space but also a deceleration of the course of physical time (Taganov,…

综合物理 · 物理学 2008-07-28 Igor N. Taganov
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