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相关论文: Are we survivors of the sudden past singularity?

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We discuss combined constraints, coming from the cosmic microwave background shift parameter $\mathcal{R}$, baryon acoustic oscillations (BAO) distance parameter $\mathcal{A}$, and from the latest type Ia supernovae data, imposed on…

宇宙学与河外天体物理 · 物理学 2013-01-11 Tomasz Denkiewicz , Mariusz P. Dabrowski , Hoda Ghodsi , Martin A. Hendry

We discuss the constraints coming from current observations of type Ia supernovae on cosmological models which allow sudden future singularities of pressure (with the scale factor and the energy density regular). We show that such a sudden…

天体物理学 · 物理学 2008-12-18 Mariusz P. Dabrowski , Tomasz Denkiewicz , Martin A. Hendry

Following the observational evidence for cosmic acceleration which may exclude a possibility for the universe to recollapse to a second singularity, we review alternative scenarios of its future evolution. Although the de Sitter asymptotic…

天体物理学 · 物理学 2009-11-11 Mariusz P. Dabrowski

In the present paper we raise the question whether initial cosmological singularity can be proved from the cosmological tests. The classical general relativity predict the existence of singularity in the past if only some energy conditions…

天体物理学 · 物理学 2009-11-11 Marek Szydlowski , Wlodzimierz Godlowski , Adam Krawiec , Jacek Golbiak

In this work we analyze the possibility of sudden cosmological singularities, also known as type-II singularities, in the background of a Friedmann-Lema\^itre-Robertson-Walker (FLRW) geometry in an extension of General Relativity (GR) known…

广义相对论与量子宇宙学 · 物理学 2024-12-03 João Luís Rosa , Tom Zlosnik

We review recent work on the existence and nature of cosmological singularities that can be formed during the evolution of generic as well as specific cosmological spacetimes in general relativity. We first discuss necessary and sufficient…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Spiros Cotsakis

Despite impressive phenomenological successes, cosmological models are incomplete without an understanding of what happened at the big bang singularity. Depending on the model, one would like to understand how appropriate initial conditions…

高能物理 - 理论 · 物理学 2010-01-26 Ben Craps

The discovery of accelerated expansion of the universe opened the possibility of new scenarios for the doom of our spacetime, besides aeternal expansion and a final contraction. In this paper we review the chances which may await our…

广义相对论与量子宇宙学 · 物理学 2022-03-01 L. Fernández-Jambrina , R. Lazkoz

Various physical properties of cosmological models in (1+1) dimensions are investigated. We demonstrate how a hot big bang and a hot big crunch can arise in some models. In particular, we examine why particle horizons do not occur in matter…

广义相对论与量子宇宙学 · 物理学 2010-04-06 K. C. K. Chan , R. B. Mann

With the recent progresses on the Type II supernovae, we attempt to investigate whether there does exist new physics beyond the standard cosmological paradigm, i.e., the cosmological constant $\Lambda$ plus cold dark matter ($\Lambda$CDM).…

宇宙学与河外天体物理 · 物理学 2019-06-26 Deng Wang

Due to the accelerated expansion of the universe, the possibility of formation of singularities has changed from the classical Big Bang and Big Crunch singularities to include a number of new scenarios. In recent papers it has been shown…

广义相对论与量子宇宙学 · 物理学 2021-12-15 L. Fernández-Jambrina

We discuss recent evidence for an accelerating Universe from measurements of type Ia supernovae at high redshift, and describe tests of various systematic effects such as extinction and evolution that could be biasing the cosmological…

天体物理学 · 物理学 2007-05-23 Saurabh Jha , the High-Z Supernova Search Team

In this dissertation we study two well known gravitational scenarios in which singularities may appear; the final state of gravitational collapse and the late time evolution of the universe. In the first scenario, we study a spherically…

广义相对论与量子宇宙学 · 物理学 2014-05-22 Yaser Tavakoli

In this work we consider a family of cosmological models featuring future singularities. This type of cosmological evolution is typical of dark energy models with an equation of state violating some of the standard energy conditions (e.g.…

广义相对论与量子宇宙学 · 物理学 2016-12-21 Jose Beltran Jimenez , Ruth Lazkoz , Diego Saez-Gomez , Vincenzo Salzano

We investigate future singularities originating from the anisotropy in the Universe. We formulate a new class of singularities in the homogeneous and anisotropic universe, comparing them with the known singularities in the homogeneous and…

广义相对论与量子宇宙学 · 物理学 2024-09-09 Taishi Katsuragawa , Shin'ichi Nojiri , Sergei D. Odintsov

A particular class of flat Emergent Universe scenario is studied in light of recent observational data. Observationally permissible ranges of values are obtained for the model parameters. The class of model studied here can accommodate…

广义相对论与量子宇宙学 · 物理学 2011-09-16 S. Ghose , B. C. Paul

The article is dedicated to one of the most undeservedly overlooked properties of the cosmological models: the behaviour at, near and due to a jump discontinuity. It is most interesting that while the usual considerations of the…

宇宙学与河外天体物理 · 物理学 2018-07-10 Artyom V. Yurov , Artyom V. Astashenok , Valerian A. Yurov

- Constraining the cosmological parameters and understanding Dark Energy have tremendous implications for the nature of the Universe and its physical laws. - The pervasive limit of systematic uncertainties reached by cosmography based on…

This work explains how the presence of a Type-IV singularity (a mild singularity) can influence the dynamics of a bouncing universe. In particular, we examine bounce cosmology that appears with a Type-IV singularity in the context of a…

广义相对论与量子宇宙学 · 物理学 2022-05-24 Sergei D. Odintsov , Tanmoy Paul

Based on the largest homogeneously reduced set of Type Ia supernova luminosity data currently available -- the Union2 sample -- we reconstruct the expansion history of the Universe in a model-independent approach. Our method tests the…

宇宙学与河外天体物理 · 物理学 2015-05-30 S. Benitez-Herrera , F. Roepke , W. Hillebrandt , C. Mignone , M. Bartelmann , J. Weller
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