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The standard model of cosmology considers the existence of two components of unknown nature, ``dark matter'' and ``dark energy'', which determine the cosmological evolution. Their nature remains unknown, and other models can also be…

天体物理学 · 物理学 2007-05-23 A. Arbey

In the standard model of cosmology, dark matter and dark energy are presently the two main contributors to the total energy in the Universe. However, these two dark components are still of unknown nature, and many alternative explanations…

天体物理学 · 物理学 2009-06-25 A. Arbey

The standard model of cosmology suggests the existence of two components, "dark matter" and "dark energy", which determine the fate of the Universe. Their nature is still under investigation, and no direct proof of their existences has…

天体物理学 · 物理学 2009-07-09 A. Arbey

The standard model of cosmology relies on the existence of two components, "dark matter" and "dark energy", which dominate the expansion of the Universe. There is no direct proof of their existence, and their nature is still unknown. Many…

宇宙学与河外天体物理 · 物理学 2014-11-20 Alexandre Arbey

Observational evidence indicating that the expansion of the universe is accelerating has surprised cosmologists in recent years. Cosmological models have sought to explain this acceleration by incorporating `dark energy', of which the…

天体物理学 · 物理学 2010-03-26 Luke Barnes , Matthew J. Francis , Geraint F. Lewis , Eric V. Linder

Recent measurements suggest our universe has a substantial dark energy component, which is usually interpreted in terms of a cosmological constant. Here we examine how much the form of this dark energy can be modified while still retaining…

高能物理 - 唯象学 · 物理学 2009-11-07 Duane A. Dicus , Wayne W. Repko

Dark energy in the universe is assumed to be vacuum energy. The energy-momentum of vacuum is described by a scale-dependent cosmological constant. The equations of motion imply for the density of matter (dust) the sum of the usual matter…

综合物理 · 物理学 2008-11-09 Walter Petry

Recent cosmological and astrophysical observations point out that the Universe is in accelerating expansion and filled up with non-luminous matter. In order to explain the observed large scale structures and this accelerating behavior one…

宇宙学与河外天体物理 · 物理学 2013-04-23 S. Capozziello , G. Lambiase

The accelerated expansion of the Universe is one of the main discoveries of the past decades, indicating the presence of an unknown component: the dark energy. Evidence of its presence is being gathered by a succession of observational…

宇宙学与河外天体物理 · 物理学 2021-04-13 V. Motta , Miguel A. García-Aspeitia , A. Hernández-Almada , J. Magaña , Tomás Verdugo

In this article, we review a series of recent theoretical results regarding a conventional approach to the dark energy (DE) concept. This approach is distinguished among others for its simplicity and its physical relevance. By compromising…

宇宙学与河外天体物理 · 物理学 2016-04-20 Kostas Kleidis , Nikolaos K. Spyrou

Cosmological observations are normally fit under the assumption that the dark sector can be decomposed into dark matter and dark energy components. However, as long as the probes remain purely gravitational, there is no unique decomposition…

宇宙学与河外天体物理 · 物理学 2009-11-05 Martin Kunz , Andrew R Liddle , David Parkinson , Changjun Gao

A cosmological model of dark energy interacting with dark matter and another general component of the universe is investigated. We found general constraints on these models imposing an accelerated expansion. The same is also studied in the…

高能物理 - 唯象学 · 物理学 2008-11-26 Norman Cruz , Samuel Lepe , Francisco Pena

Dark matter and dark energy are essential in the description of the late Universe, since at least the epoch of equality. On the other hand, the inflation is also necessary and demands a "dark" component, usually associated to a scalar field…

宇宙学与河外天体物理 · 物理学 2013-08-08 Jorge L. Cervantes-Cota , Alejandro Aviles , Josue De-Santiago

It is now well accepted that both Dark Matter and Dark Energy are required in any successful cosmological model. Although there is ample evidence that both Dark components are necessary, the conventional theories make no prediction for the…

天体物理学 · 物理学 2007-05-23 Douglas Scott , Ali Frolop

Two exotic elements have been introduced into the standard cosmological model: non-baryonic dark matter and dark energy. The success in converting a hypothesis into a solid theory depends strongly on whether we are able to solve the…

宇宙学与河外天体物理 · 物理学 2020-01-08 Martin Lopez-Corredoira

As cosmology has entered a phase of precision experiments, the content of the universe has been established to contain interesting and not yet fully understood components, namely dark energy and dark matter. While the cause and exact nature…

高能物理 - 唯象学 · 物理学 2015-06-25 Lars Bergstrom

Dark energy is one of the mysteries of modern science. It is unlike any known form of matter or energy and has been detected so far only by its gravitational effect of repulsion. Owing to its effects being discernible only at very very…

宇宙学与河外天体物理 · 物理学 2009-08-25 Aruna Kesavan

The vacuum is filled with complex scalar fields, such as the Higgs field. These fields serve as order parameters for superfluidity (quantum phase coherence over macroscopic distances), making the entire universe a superfluid. We review a…

广义相对论与量子宇宙学 · 物理学 2013-11-18 Kerson Huang

A new model for the universe filled with a generalized Chaplygin fluid is considered which unitarily describes as a single vacuum entity both a quintessence scalar field and a cosmological constant, so unifying the notion of dark energy.…

天体物理学 · 物理学 2008-11-26 Pedro F. Gonzalez-Diaz

We investigate how the nature of dark energy affects the determination of the curvature of the universe from recent observations. For this purpose, we consider the constraints on the matter and dark energy density using observations of type…

天体物理学 · 物理学 2008-11-26 Kazuhide Ichikawa , Masahiro Kawasaki , Toyokazu Sekiguchi , Tomo Takahashi
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