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相关论文: Cosmology in the Universe with distance dependent …

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After decades of successful hot big-bang paradigm, Cosmology still lacks a framework in which the early inflationary phase of the universe smoothly matches the radiation epoch and evolves to the present `quasi' de Sitter spacetime. No less…

宇宙学与河外天体物理 · 物理学 2015-06-16 S. Basilakos , J. A. S. Lima , J. Solà

Multifield models, arising from multiple scalars interacting with gravity, provide a rich theoretical framework for addressing fundamental problems in modern cosmology. A key role in this regard is played by the so called rapid turn regime,…

高能物理 - 理论 · 物理学 2026-01-06 Lilia Anguelova

A cosmological model is formulated in the context of a scalar-tensor theory of gravity in which the entire cosmic background evolution is due to a complex scalar field evolving in Minkowski spacetime, such that its (dimensional) modulus is…

综合物理 · 物理学 2019-09-24 Meir Shimon

We consider a class of cosmological models in which the universe is filled with a (non-electric) charge density that repels itself by means of a force carried by a vector boson with a tiny mass. When the vector's mass depends upon other…

高能物理 - 唯象学 · 物理学 2009-11-07 Martina Brisudova , William H. Kinney , Richard Woodard

Current astronomical observations are successfully explained by the present cosmological paradigm based on the concordance model ($\Lambda_0$CDM + Inflation). However, such a scenario is composed of a heterogeneous mix of ingredients for…

广义相对论与量子宇宙学 · 物理学 2018-08-29 J. A. S Lima , Douglas Singleton

The idea that the cosmological term, Lambda, should be a time dependent quantity in cosmology is a most natural one. It is difficult to conceive an expanding universe with a strictly constant vacuum energy density, namely one that has…

宇宙学与河外天体物理 · 物理学 2015-03-18 Joan Sola

An exploratory study of the cosmology of moduli in string theory. Moduli are argued to be natural inflaton fields and lead to a robust inflationary cosmology in which inflation takes place at the top of domain walls. The amplitude of…

高能物理 - 理论 · 物理学 2016-09-06 T. Banks , M. Berkooz , G. Moore , S. H. Shenker , P. J. Steinhardt

We propose a time-varying cosmological constant with a fixed equation of state, which evolves mainly through its interaction with the background during most of the long history of the universe. However, such interaction does not exist in…

宇宙学与河外天体物理 · 物理学 2009-08-18 Murli Manohar Verma

We investigate cosmology with complex scalar field. It is shown that such models can describe two stages of inflation and the oscillatory regime. Thus we don't need both quintessence and $\Lambda$-term. It is enough to have single complex…

高能物理 - 理论 · 物理学 2007-05-23 A. V. Yurov

Cosmology is operating now on a well established and tightly constraining empirical basis. The relativistic LambdaCDM hot big bang theory is consistent with all the present tests; it has become the benchmark. But the many open issues in…

宇宙学与河外天体物理 · 物理学 2014-11-20 P. J. E. Peebles

Cosmological consequences of a string-motivated dark energy scenario featuring a scalar field coupled to the Gauss-Bonnet invariant are investigated. We study the evolution of the universe in such a model, identifying its key properties.…

天体物理学 · 物理学 2008-11-26 Tomi Koivisto , David F. Mota

We consider cosmology in the Einstein-aether theory (the generally covariant theory of gravitation coupled to a dynamical timelike Lorentz-violating vector field) with a linear aether-Lagrangian. The 3+1 spacetime splitting approach is used…

天体物理学 · 物理学 2008-11-26 Baojiu Li , David F. Mota , John D. Barrow

Modern cosmology is based on the cosmological principle, which states that the Universe is statistically homogeneous and isotropic. When applied in its strict -- rather than statistical -- sense, the cosmological principle leads to the…

宇宙学与河外天体物理 · 物理学 2025-09-03 Pierre Fleury

A variety of observations indicate that the universe is dominated by dark energy with negative pressure, one possibility for which is a cosmological constant. If the dark energy is a cosmological constant, a fundamental question is: Why has…

天体物理学 · 物理学 2008-11-26 Maqbool Ahmed , Scott Dodelson , Patrick B. Greene , Rafael Sorkin

During the last ten years astrophysical cosmology has brought three remarkable results of deep impact for fundamental physics: the existence of non-baryonic dark matter, the (nearly) flatness of space, the domination of the density of the…

天体物理学 · 物理学 2007-05-23 Alain Blanchard

We use the phase plane analysis technique of Madsen and Ellis to consider a universe with a true cosmological constant as well as a cosmological "constant" that is decaying. Time symmetric dynamics for the inflationary era allows eternally…

宇宙学与河外天体物理 · 物理学 2016-04-27 George F. R. Ellis , Emma Platts , David Sloan , Amanda Weltman

We review a cosmology in which particles are fluctuationally created from a background Zero Point Field. This cosmology is consistent with recent observations of an ever expanding and accelerating universe, as also the recently confirmed…

综合物理 · 物理学 2015-06-26 B. G. Sidharth

We study cosmological implications of a Lorentz invariance violating DGP-inspired braneworld scenario. A minimally coupled scalar field and a single, fixed-norm, Lorentz-violating timelike vector field within an interactive picture provide…

广义相对论与量子宇宙学 · 物理学 2009-02-12 Kourosh Nozari , S. Davood Sadatian

Using the dS/QFT correspondence in the context of inflation allows for the study of interesting, otherwise inaccessible physics. In particular, by studying inflation via its dual field theory at the boundary of the de Sitter space, it may…

宇宙学与河外天体物理 · 物理学 2011-08-08 Mafalda Dias

These four lectures cover four topics in modern cosmology: the cosmological constant, the cosmic microwave background, inflation, and cosmology as a probe of physics at the Planck scale. The underlying theme is that cosmology gives us a…

天体物理学 · 物理学 2007-05-23 William H. Kinney